text:
\section{Introduction}
According to the principle of equivalence a frame undergoing uniform
accelerated motion is equivalent to a rest frame in presence of a
constant gravitational field \cite{R1,R2,R3}.
Therefore considering that the surface of the
enclosure which is filled up with
either a photon gas or a gas of de Broglie waves is expanding
adiabatically with  uniform  acceleration may be assumed to be
equivalent to a uniformly accelerated reference frame. Then following the principle of equivalence
we may replace it by a rest frame in
presence of a constant gravitational field. We further assume that
the gravitational field is uniform within a width $\Delta H$ inside
the enclosure near the
surface. Further, assuming that the structure of the enclosure is of
spherical in nature,
let $H$ be the corresponding radius.
It is quite obvious that a photon will gain or loose
energy when it travels towards the wall or reflected back from the
wall respectively \cite{R4,R5}. Hence we can say that the
picture will be reversed during the reflection from the wall (see also \cite{R55} for displacement law in the case
of particle production).
Assuming that the wall is
perfectly reflecting, then there will be no absorption of photon energy.
 the photon will be Doppler shifted both
during its incidence and reflection at the wall. However, since the
wall is expanding with uniform acceleration, unlike
the case of expansion of the wall with a uniform velocity, in the
present scenario
the change is not so called apparent. Here the Doppler shift is
associated with the
real change in energy of the photons. It is therefore the gravitational
redshift, not the conventional change in wavelength which occurs when
there is a relative motion between the source and the observer.
The wave will be blue shifted while moving towards the surface and
the reverse is the case, i.e., redshift of the wave during
reflection. We will show that the same is true for the matter wave
associated with the incident and the reflected particles (fermions or
bosons) when the enclosure is filled with either Fermi gas or Bose
gas.

To get a physical
insight of the incidence and the reflection processes, we consider
the prescription of Feynman instead of considering Rindler
space-time coordinate transformations \cite{R1,R3,R6}
(see also \cite{R61,R62,R63}).
These two approaches however, essentially give the
same result. Moreover in our opinion the prescription of Feynman lecture is
more straight forward and is easy to understand physically. Now the Rindler
coordinate transformations are exactly like the Lorentz
transformations in a frame undergoing uniform acceleration, otherwise
in flat Minkowski space-time geometry.

In this article we have also obtained the
modified form of Wien's displacement laws for de Broglie waves. The geometrical structure of the
enclosure is exactly identical as we have considered in the case of photon gas.

In this article we have also studied the
gravitational redshift of photons using the prescription of Friedman and
Friedman et al \cite{R7,R8,R9,R91}. The later
approach is conventionally known as the extended
relativistic dynamics with an upper
limit of acceleration. In this study we have also tried to put forward
some physical meaning to the maximum value of acceleration.

The article is organized in the following manner. In the next
section,
following the prescription of Feynman lecture, we have obtained the
Doppler shift of photons and establish the modified form of Wien's
displacement law following Saha and Srivastava \cite{R10} when the wall of the enclosure is
expanding adiabatically with uniform acceleration.
In section-3 we have
obtained the gravitational redshift factor $z$ following Friedman and
Friedman et al \cite{R7,R8,R9,R91}. In section-4 we have developed the Wien's
displacement laws for the de Broglie waves for both fermion type and
boson type particles. Finally we have given
conclusion of the work.
\section{Wien's Displacement Law in Rindler Space for Photon Gas}
Let us consider a photon of circular frequency $\omega_0$, traveling
towards the wall of the enclosure which is moving outward with a uniform
acceleration $\alpha$. The energy of the incident photon is then
$\varepsilon_0=\hbar \omega_0$. The equivalent moving mass is
therefore $m_0=\varepsilon_0/c^2=\hbar \omega_0/c^2$. Hence the
gain of energy by the photon is $m_0 \alpha \Delta H$, $\Delta H$ is
the distance traversed and $\alpha$ is assumed to be constant within
$\Delta H$ in the sense of principle of equivalence. Then the energy
of the photon at the instant of incidence on the wall is
\begin{equation}
\varepsilon_1=\hbar \omega_0 +\frac{\hbar \omega_0}{c^2}\alpha \Delta
H
\end{equation}
Then the changed value of photon frequency is given by
\begin{equation}
\omega_1=\omega_0\left ( 1+\frac{\alpha \Delta H}{c^2}\right )
\end{equation}
This is the gravitational Doppler shifted frequency of the incident photon. The
same result can also be obtained from Rindler space-time coordinate
transformations. While
reflected back from the wall, the photon is traveling away from the
wall. The photon will therefore loose energy. If $\omega_2$ is the
Doppler shifted frequency of the reflected photon, then the energy of
this photon is given by
\begin{equation}
\hbar \omega_1=\hbar \omega_2 -\frac{\hbar \omega_2}{c^2} \Delta H
\alpha
\end{equation}
Hence
\begin{equation}
\omega_1=\omega_2\left ( 1-\frac{\alpha \Delta H}{c^2}\right )
\end{equation}
Therefore during incidence it is gravitational blue shift, whereas during reflection it is gravitational redshift.
Then combining eqns.(2) and (4), we have
\begin{equation}
\omega_2=\omega_0 \frac{\left (1+\frac{\alpha \Delta H}{c^2} \right
)}
{\left ( 1-\frac{\alpha \Delta H}{c^2} \right )}
\end{equation}
Therefore it is not the same kind of physical picture as discussed in
the book by Saha and Srivastava \cite{R10}.
In the later case the wall is moving with
uniform velocity and the wave gets red-shifted both during incidence
as well as during reflection and we know from the knowledge of optics that
the change is apparent. Whereas in the case of accelerated frame of
reference the energy of the photon changes both during incidence and
reflection. The change of energy is proportional to the constant
gravitational field.
Therefore although the final result gives redshift of the
photon, which is equivalent to gravitational redshift, but
it is quite different from the conventional redshift of photons in
optics. Since either during incidence or reflection
some change in energy of the photon is occurring and it depends on the
strength of constant gravitational field, the change
is real in nature.

Now replacing $\omega_0=\omega=2\pi \nu$ and $\omega_2=\omega+\Delta
\omega= 2\pi (\nu +\Delta \nu)$, we have
\begin{equation}
\nu +\Delta \nu =\nu \frac{\left ( 1+\frac{\alpha \Delta
H}{c^2}\right ) }
{\left ( 1-\frac{\alpha \Delta H}{c^2}\right )}
\end{equation}
Assuming that the factor $\alpha \Delta H/c^2 \ll 1$, we have
\begin{equation}
\frac{\Delta \nu}{\nu} \approx \frac{2\alpha \Delta H}{c^2}
\end{equation}
Hence we can also write
\begin{equation}
\frac{\Delta \lambda}{\lambda} = -\frac{2\alpha \Delta H}{c^2}
\end{equation}
Now the single particle classical Hamiltonian is given by
\begin{equation}
H_0=\left ( 1+\frac{\alpha\Delta H}{c^2}\right )pc=L(\Delta H)pc
=\varepsilon
\end{equation}
where $L(\Delta H)$ is a function of $\Delta H$. Hence following the
standard result of statistical mechanics, the energy density may be
written as \cite{R11}
\begin{equation}
\epsilon =\frac{{\rm{constant}}~T^4}{L^3(\Delta H)}
\end{equation}
For adiabatic expansion of the photon gas
\begin{equation}
PV^{4/3}={\rm{constant}}
\end{equation}
Again for the photon gas
\begin{equation}
P=\frac{1}{3} \epsilon
\end{equation}
Hence
\begin{equation}
\epsilon V^{4/3}={\rm{constant}}
\end{equation}
The above equation can also be expressed as
\begin{equation}
\frac{T^4H^4}{\left (1+\frac{\alpha \Delta H}{c^2}\right )^3}=
{\rm{constant}}
\end{equation}
where we have used $V=4\pi H^3/3$, the volume of the enclosure.
Hence assuming that the factor $\alpha \Delta H/c^2 \ll 1$, we have
\begin{equation}
HT={\rm{constant}}
\end{equation}
Now for the oblique incidence, we can write
\begin{equation}
\frac{\Delta \lambda}{\lambda}=-\frac{2\alpha \Delta H}{c^2}
\cos\theta
\end{equation}
where $\theta$ is the angle of incidence.
This is the change in wavelength per collision. Then following Saha
and Srivastava \cite{R10}, we have the change of wavelength per unit time
\begin{equation}
\frac{\Delta \lambda}{\lambda}= -\frac{\alpha}{c}\frac{\Delta H}{H}
\end{equation}
In the limiting case, we can write
\begin{equation}
\frac{d\lambda}{\lambda}=-\frac{\alpha}{c}\frac{dH}{H}
\end{equation}
Integrating, we have
\begin{equation}
\lambda H^{\omega_c}={\rm{constant}}
\end{equation}
where $\omega_c=\alpha/c$, the frequency of cosmic phonons as
described in \cite{R12}. Then combining eqns.(15) and (19), we have
\begin{equation}
\lambda T^{-\omega_c}={\rm{constant~~ or~~}} \lambda \propto
T^{\omega_c}
\end{equation}
This is the modified version of Wien's displacement law for photon gas in the Rindler space.
It is therefore obvious that $\lambda$ will be quite  large if
$\alpha$ is large enough. This is consistent with the conventional
result on gravitational redshift. Further, the wavelength saturates to a
constant value for $\alpha\longrightarrow 0$.
\section{Gravitational Redshift in Extended Relativistic Dynamics}
Next we consider the prescription of Friedman and Friedman et al
\cite{R7,R8,R9,R91} on
the extended relativistic dynamics and maximal acceleration. Now the
clock hypothesis of Einstein states that the timing of an accelerated
clock is identical with that of a clock at rest in some
un-accelerated frame of reference. It is well known that if the
clock hypothesis is correct, the transformations are Galilean type.
Whereas, if the clock hypothesis is false, then the transformations
are Lorentz type. In the later  case the uniform acceleration of the
frame plays  the role of uniform velocity of Lorentz type
transformations. The maximal value of acceleration plays the role of
velocity of light. In the special theory of relativity the velocity
of light is treated as the upper limit of velocity.

Then following Friedman,
when the clock hypothesis is false,
we have the proper velocity-time
transformations
\begin{eqnarray}
t&=& \gamma \left (t^\prime +\frac{\alpha u_x^\prime}{\alpha_m^2}
\right ) \nonumber \\
u_x&=& \gamma (\alpha t^\prime +u_x^\prime )\nonumber \\
u_y&=&u_y^\prime\nonumber \\
u_z&=& u_z^\prime
\end{eqnarray}
where $\gamma=(1- \alpha^2/\alpha_m^2)^{1/2}$, the time dilation
factor. The motion is assumed to be along $x$-direction and the
uniform acceleration $\alpha$ is also along the same direction. Here
$\alpha_m$ is the upper limit of acceleration, just like the velocity
of light is the maximum possible value for velocity in the case of
Lorentz transformation in special theory of relativity.

To get an estimate for Doppler shift of an electromagnetic wave, we
follow Friedman and assume that the wave-vector $k$ in the proper
velocity-time representation is also along $x$-direction. Then from
\cite{R7}, the electromagnetic radiation may be represented by the function
\begin{eqnarray}
(\omega t-k u)&=&f\left [ \omega\gamma \left ( t^\prime
+\frac{\alpha u^\prime}{\alpha_m^2}\right ) -k\gamma (\alpha t^\prime
+u^\prime)\right ] \nonumber \\ &=& f\left [ \gamma \left (\omega
-k\alpha\right )t^\prime -\gamma \left ( k-\frac{\alpha}{\alpha_m^2}
\right )u^\prime \right ] \nonumber \\ &=& f(\omega^\prime t^\prime
-k^\prime u^\prime) ~~ ({\rm{say}})
\end{eqnarray}
Hence
\begin{eqnarray}
\omega^\prime&=&\gamma(\omega -k \alpha)\nonumber \\ &=& \omega
\frac{\left (1- \frac{\alpha}{\alpha_m}\right )}{ \left
(1-\frac{\alpha^2}{\alpha_m^2}\right )^{1/2}}
\end{eqnarray}
For $\alpha/\alpha_m\ll 1$ and writing $\omega=2\pi \nu$, with $\nu$
the actual frequency, we have
\begin{equation}
\nu^\prime =\nu \left ( 1-\frac{\alpha}{\alpha_m}\right )
\end{equation}
Following the discussion of section-2, here also we consider the outward
expansion of the wall of the enclosure, containing photon gas, with a
uniform acceleration $\alpha$. In this prescription,
when a photon of frequency $\nu$
incident on the surface of the enclosure,
it will be red-shifted to $\nu^\prime$ as given
in eqn.(24). Further, if the surface is perfect reflector, the wave
will again be red-shifted without any loss of energy by absorption
and the final frequency will be
\begin{equation}
\nu^{\prime\prime}=\nu \frac{\left (1-\frac{\alpha}{\alpha_m}\right
)}{\left ( 1+\frac{\alpha}{\alpha_m} \right )}
\end{equation}
Now writing $\nu^{\prime\prime}=\nu+d\nu$, where $d\nu$ is the
effective change in frequency due to Doppler shift, we have
\begin{equation}
\frac{d\nu}{\nu}=-\frac{2\alpha}{\alpha_m}
\end{equation}
Hence
\begin{equation}
\frac{d\lambda}{\lambda}=\frac{2\alpha}{\alpha_m}
\end{equation}
Here we have considered only normal incidence. Now eqn.(27) may be
approximated with  $z$, the gravitational redshift factor. Here the
quantity $z$ depends only on the uniform acceleration $\alpha$.
Further the redshift arises because of the accelerated motion of the
reflecting surface.
In accordance with the principle of equivalence, we may replace the
uniformly accelerated frame by a stationary frame in presence of
a constant gravitational field $\alpha$. Therefore one may assume that
$\alpha$ is the constant gravitational field produced by a self
gravitating object, e.g., a neutron star (not a black hole, because
nothing is known about the gravitational field of the black hole).
Then $\alpha_m$ is the maximum possible surface value of
gravitational field for a neutron star.
For $\alpha=\alpha_m$, the gravitational redshift factor $z$ becomes $2$.
Since $\alpha$ is always less that $\alpha_m$, therefore
$z$ is always less than $2$, the bound for gravitational redshift
factor at the neutron star surface for $M/R < 4/9$ \cite{R13}
in geometrical unit, where $M$
and $R$ are respectively the mass and radius of a neutron star.
Therefore according to our
analysis, the quantity $\alpha_m$ has physical significance. It is related to
the maximum gravitational redshift for the compact stellar object concerned.
\section{Wien's Displacement Law for de Broglie Waves in Rindler Space}
To develop a formalism for Wien's displacement law of de Broglie waves in Rindler space
we replace $\hbar \omega$ by the single particle energy $\varepsilon$ of the fermion or boson and further we write
in the non-relativistic approximation the single particle energy $\varepsilon=p^2/2m$, where $m$ is the particle
mass. In this model calculation we assume that the enclosure whose wall is expanding adiabatically with constant
acceleration is filled up with either a Fermi gas or a Bose gas. At
first we develop the formalism
in a very general manner, applicable for both the fermions and bosons. At the end of this section only we
shall differentiate between fermions from bosons. Further, the
collisions of the particles are assumed to be elastic in nature.

Now following eqns.(1) and (3), we have
\begin{equation}
p_1=p_0\left ( 1+\frac{\alpha \Delta H}{c^2}\right )^{1/2}\approx p_0\left (1+\frac{\alpha \Delta H}{2c^2} \right )
\end{equation}
and
\begin{equation}
p_1\approx p_2\left ( 1-\frac{\alpha \Delta H}{2c^2}\right )
\end{equation}
Combining these two equations, we have
\begin{equation}
P_2=p_0\frac{1+\frac{\alpha \Delta H}{2c^2}} {1- \frac{\alpha \Delta
H}{2c^2}}
\end{equation}
Now writing $\lambda=h/p$, the de Broglie wave length of the
particle, we have
\begin{equation}
\lambda_2=\lambda_0\frac{1-\frac{\alpha \Delta H} {2c^2}} {1+ \frac{\alpha \Delta
H}{2c^2}}
\end{equation}
This is the relation between the initial (before incidence) and final (after
reflection) de Broglie wavelengths of the particle.
Now as before, assuming an infinitesimal change in de Broglie
wavelength during reflection from the wall, we can write
$\lambda_2=\lambda+\delta \lambda$, where we have
put $\lambda$ for $\lambda_0$, the initial de Broglie wavelength and
$\delta \lambda$ is the infinitesimal change in de Broglie wavelength.
Then following the same procedure as has been used for photon gas, we
have in the limiting case
\begin{equation}
\frac{d\lambda}{\lambda}=-\omega_c \frac{dH}{H}
\end{equation}
On integrating, we have
\begin{equation}
\lambda H^{\omega_c}={\rm{constant}}
\end{equation}
Now for a non-relativistic gas
\begin{equation}
P=\frac{2}{3}\epsilon
\end{equation}
where $\epsilon$ is the energy density and $P$ is the kinetic
pressure of the gas. Now for the adiabatic expansion of
non-relativistic gas, we have
\begin{equation}
PV^{5/3}=\rm{constant}
\end{equation}
Combining these two equations, we can write
\begin{equation}
\epsilon V^{5/3}={\rm{constant}}
\end{equation}
Now for a non-relativistic gas obeying Boltzman statistics, we can
write
\begin{equation}
\epsilon = C T^{5/2}\exp\left (\frac{\mu}{kT}\right )
\end{equation}
where $C$ is a constant and $\mu$ is the chemical potential of the
gas. Combining eqns.(36) and (37) and using $V=44\pi H^3/3$ as the volume
of the enclosure, with $H$ its radius, we have
\begin{equation}
TH^2\exp\left (\frac{2\mu}{5kT}\right ) ={\rm{constant}}
\end{equation}
Again using eqn.(33), we have for a Fermi gas with non-zero chemical
potential
\begin{equation}
\lambda ={\rm{constant}} T^{0.5{\omega_c}}\exp \left (\frac{\mu
\omega_c}{5kT} \right )
\end{equation}
This is the modified form of Wien's displacement law for fermionic de
Broglie wavelength in Rindler space. Obviously the wavelength
increases in a much faster rate with the strength of gravitational
field $\alpha$ in comparison with photon gas for fixed $T$. Further,
the wavelength exponentially diverges for large $\alpha$. Similar to
the photon gas the de Broglie wavelength saturates to a constant
value for very low $\alpha$ ($\alpha \rightarrow 0$). On the other
hand if one considers an anti-fermion with chemical potential $-\mu$,
then the de Broglie wavelength after reflection becomes
\begin{equation}
\lambda ={\rm{constant}} T^{0.5{\omega_c}}\exp \left (\frac{-\mu
\omega_c}{5kT} \right )
\end{equation}
Therefore as the gravitational field becomes strong enough the de
Broglie wavelength of the anti-fermion decreases and in the extreme
case for $\alpha\rightarrow \infty$, $\lambda \rightarrow 0$.
Therefore  in extremely strong gravitational field anti-fermions
behave like classical objects. Since anti-particles do not exist in
classical mechanics, even in the non-relativistic quantum mechanics
they do not exist. In Schr\"{o}dinger equation particle and the
corresponding anti-particle are treated in equal footing. Therefore
we can conclude that Strong gravitational field will never allow the
emission of anti-particles. When the pairs are produced at the surface of a
strongly gravitating object, then we expect only the particle will be
emitted, whereas the anti-particle counter part will go inside the
object. Which may be the another version of Penrose mechanism, but the reason is quite different.

Next we consider a Bose gas with chemical potential $\mu=0$ (say a
mixture of $\pi^+$ and $\pi^-$.) Then it is obvious that
the modified form of Wien's displacement law is given by
\begin{equation}
\lambda={\rm{constant}} T^{0.5{\omega_c}}
\end{equation}
The variation is therefore little slower compared to photon gas.
\section{Conclusion}
In this article we have developed a formalism to study Wien's
displacement law for photon gas and a gas of de Broglie waves
in a frame undergoing a uniform accelerated motion.

It is well known that the conventional form of Wien's displacement
law for photon gas
is $\lambda \propto T^{-1}$, whereas in the present scenario
it is $\lambda \propto T^{\omega_c}$, with $\omega_c=\alpha/c
\geq 0$. Hence one can infer that for $\alpha \longrightarrow
\infty$, $\lambda \longrightarrow \infty$. This is consistent with the
results of gravitational redshift in presence of strong gravitational
field produced by some compact massive stellar objects.
In this case
the redshift is because of uniform acceleration of the frame or
because of constant gravitational field in the sense of principle of
equivalence. Therefore not the temperature, but the strength of
gravitational field plays the major role in producing Doppler shift
of the wave if the field is extremely strong.
It is also obvious that for low gravitational field
(acceleration), i.e., for $\alpha\longrightarrow 0$, the wavelength
$\lambda$ saturates to some constant value. This is true for the
formalism either based on the prescription of Feynman lecture or using
Rindler coordinates.

In the second part we have studied the
gravitational redshift for electromagnetic waves in the context of
extended relativistic dynamics with an upper limit of acceleration
$\alpha_m$ of the frame. In this scenario we have noticed that for
$\alpha=\alpha_m$, the gravitational redshift factor $z=2$. Since
$\alpha$ is always $ < \alpha_m$, we have $z < 2$, the bound of
gravitational redshift factor. This can also be obtained from general theory
of relativity with $M/R < 4/9$ \cite{R14}.

In the third part we have studied the gravitational redshift of de
Broglie waves in Rindler space. In the case of fermionic de Broglie
waves the effect is more prominent because of the exponential term.
The wavelength increases much faster with the gravitational field
compared to photon gas. For extremely high gravitational field the
wavelength diverges exponentially. Whereas for a Bose gas with zero
chemical potential the increase of wavelength with gravitational
filed is little bit slower compared to photon gas. For extremely high
field it again diverges, but not exponentially.

The physical reason for the gravitational redshift of photons is the
curvature of the space produced by gravity, whereas in the case of de
Broglie waves it is because of the gain or loss of energy of the
particle, when it goes in favor or against gravity respectively.

redpajama_set_name: RedPajamaArXiv


text:
Q: Squash all UIDs automatically, without "all_squash" I have a pair of Debian stable boxes sharing /home over NFS. The server used to serve LTSP workstations and has had a long running NFS configuration that never gave me any trouble.
The LTSP project ended, I got a new laptop, connected to the same NFS server, and saw no problems until the laptop died. I then got an old laptop out of mothballs, set it up with identical UIDs, mounted /home and discovered all the files in /home are owned by nobody.
Apparently, since I last was active in setting up NFS (not just using my stable setup) nfs4 and all_squash have become options. I checked my exports file, and everything looks fine: all_squash is not specified anywhere and it is not the default.
What did I miss?

redpajama_set_name: RedPajamaStackExchange


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text:
Gian Luigi Ferri – The 101 California Street Shootings – Mass Murder
Rhonda Dean
Gian Luigi Ferri
The 101 California Street Shootings
Gian Luigi Ferri appeared to be a portly middle-aged professional carrying an attache case and wheeling a lawyer's case on a dolly. But when he stepped into the law offices on the 34th floor of a downtown office building here, he shed his jacket, donned a pair of orange ear protectors and went to battle with three semi-automatic pistols.
The question today in San Francisco was what drove the gunman, identified as Gian Luigi Ferri of Los Angeles, into a murderous spree on a Thursday afternoon in which he killed eight people, wounded six others and then ended his own life with a bullet from a .45-caliber Colt placed under his chin.
A murky picture began to emerge today of Mr. Gian Luigi Ferri as a real estate speculator who once won a million-dollar judgment and more recently sought to file for bankruptcy. Members of the firm he assaulted, Pettit & Martin, were at first unable to recognize Mr. Ferri, but later discovered that he had been a client in 1981. They had given Mr. Ferri advice in several real estate transactions, mainly to buy several trailer parks in Indiana and Kentucky. No Contact since '1982.
Shortly after that, said Vickie Spang, marketing director for the firm, he ( Gian Luigi Ferri) had complained that the seller had made misrepresentations. She said the firm had helped him find local counsel in Indiana that helped him win a $1 million judgment there. Pettit & Martin had no records of any complaints about its own work from Mr. Ferri.
Whether Gian Luigi Ferri ever collected the judgment could not be learned, but it appeared that when he began shooting, Mr. Ferri was a man down on his luck. He recently approached a law office in Hollywood seeking to file for personal bankruptcy.
Gian Luigi Ferri told the lawyers in Hollywood that he had lost $300,000 in a land deal in Leadville, Colo., near Aspen. "Somebody did a real number on him," Elias Francisco, a paralegal at E. Francisco & Associates, a law firm run by his brother Emilio, had said.
Described as Quite Man
The county coroner, Boyd Stephens, identified the gunman as Mr. Gian Luigi Ferri, 55, of the Woodland Hills section of Los Angeles, owner of ADF Mortgage, which was incorporated in Nevada in 1987. The police found his 1986 or 1987 Cadillac in a parking garage in the Embarcadero Center, a block from the 48-story glass and granite tower where Mr. Ferri spread carnage.
"His name didn't mean anything to me," said Richard E. Climan, a partner in the Pettit firm, which has 160 lawyers in six offices and practices mostly business law.
In Woodland Hills, neighbors of ADF, which occupied a second-story office in a shopping strip, described Mr. Ferri as a quiet man who spoke with a foreign accent, when he spoke at all. He appeared to be in financial trouble, they said, and would sometimes sit in his car for two hours at time.
"He always stayed by himself and seemed lonely and sad," said Marilyn J. Petlack. "I never saw any clients going in there. I knew he was not doing well financially, but he didn't seem like a criminal type." At the nearby Oakwood apartment complex, where he rented a furnished one-bedroom apartment, the manager said Gian Luigi Ferri had not paid his June rent.
Wrong Place, Wrong Time
The police said they found a list of names on Mr. Ferri's body, but no one on the list appeared to be among the victims. And at least two of the dead appeared to have been entirely unrelated to any issue he had with the firm: Jack Berman, a 36-year-old partner in another San Francisco law firm, Bronson, Bronson & McKinnon, and a client of his, Jody Sposato, 30, who were there to give a deposition in a lawsuit she had brought against a former employer over her dismissal.
The San Francisco County coroner said the others killed were Deborah Fogel, a secretary for the law firm Davis Wright & Tremaine; Donald Michael Merrill, 48, of Oakland, whose employment and reason for being in the building were unclear; and four employees of Pettit & Martin, John C. Scully, 28, an associate lawyer in the firm; a law partner, Allen J. Berk, 52; a summer legal assistant, David Sutcliffe, 30, of San Francisco, and a secretary, Shirley Mooser, 64.
Gian Luigi Ferri Was Down On His Luck
Last October, Gian Luigi Ferri walked into the Hollywood offices of E. Francisco & Associates, bankruptcy lawyers based in Irvine, Calif., to ask about filing for bankruptcy. "He was very gentle, very friendly, a chubby little guy," recalled Elias Francisco. "But he was hard up. He was hurting."
He said Mr. Ferri described losing $300,000 when he was not allowed to build on land in Leadville. "I got the feeling he had a lot of money at one time," Mr. Francisco said. He said Gian Luigi Ferri could not even afford the $1,100 fee to file for bankruptcy. And this fact did not help the already fragile situation.
Gian Luigi Ferri Entered Prepared for Battle
San Francisco authorities gave this account of Thursday's events:
Mr. Ferri, dressed in a dark business suit and carrying his cases, entered the elevators at 101 California Street shortly before 3 P.M. At the 34th floor, "He shed his coat and prepared for battle," said Inspector Napoleon Hendrix.
His battle armaments were two 9-millimeter Intratec DC9 semi-automatic machine pistols, carried in shoulder straps and each loaded with 50-round magazines, a smaller .45-caliber semi-automatic handgun and hundreds of rounds of ammunition loaded into dozens of magazines carried in his innocent-looking lawyer cases.
Without speaking a word, Gian Luigi Ferri opened fire on a glassed-in conference room where a deposition was in progress, killing Mr. Berman, the lawyer, and his client, Ms. Sposato. He killed another person on the 34th floor, then moved to lower floors, leaving five more dead and six wounded.
Two minutes after the first emergency call, 110 police officers arrived and shut down the elevators. Terrified office workers tripped the fire alarms, but the police turned the alarm off, which locked the doors in the stairwell, trapping the gunman who was trying to escape down the stairs. Somewhere below the 29th floor, Mr. Ferri saw officers coming up the stairs, and fled back up the stairs and then shot himself to death with a single bullet.
And the unexplained battle just as quickly ended.
credit murderpedia – The Broker Who Killed 8 – By Robert Reinhold – The New York Times
The Insane Ramblings Of A Mad Man
By Robert Reinhold – The New York Times
The deadly rampage in the law firm appears to have been the irrational and desperate act of a deranged man.
That is the almost inescapable conclusion from a rambling semiliterate screed found on the man's body after he killed eight people, wounded six others and finally killed himself at the law offices of Pettit & Martin here. The 55-year-old gunman — variously identified by the authorities as Gian Luigi Ferri — carried a hit list of more than 30 names, apparently targets of his wrath, but no one on his list was among the victims.
In his four-page typed letter, Mr. Ferri ranted about a flavor enhancer in food, monosodium glutamate, the Food and Drug Administration, and the legal profession. Excerpts of the letter were published today in The San Francisco Chronicle.
In his letter, Mr. Ferri said he had been "raped" by Pettit & Martin. Contrary to rumors of a recent connection between Mr. Ferri and the law firm, Pettit & Martin reported Friday that it had advised him a dozen years ago on some real estate deals in the Midwest but had no contact with him since then.
The letter, filled with misspellings and grammatical errors, said, "The last thing that made all of this come to a head is that I am one of those people of the 5% of the population (12.5 million people), where the poison monosodium glutamate (MGS) has reached such high levels in our cells, that a minimum amount more can kill us."
The letter ended with a blast at lawyers. "When you hire a consultant or an attorney you don't hire for the purpose of getting raped and than having all your efforts toward legal recourse totally thwarted by a corrupt legal system of 'esquires'. Esquires in the dark ages romed the countryside to steel from the working people and give tothe prince. Do attorney want us to call them esquires because their allegiance is to the monarchy?"
None of the dead or wounded appeared to have any connection with Gian Luigi Ferri or were on his "list of criminals, rapists, racketeeres, lobbyists."
Martin Bryant – The Port Arthur Massacre – Tasmania, Australia
Jeffrey Lundgren – The Kirtland Massacre-Mass Murder of Mormans
Christian Longo – He Said He Killed Her For Killing His Kids! A Jury Said Otherwise

redpajama_set_name: RedPajamaCommonCrawl


text:
Saint-Léger-sous-Cholet è un comune francese di 2.579 abitanti situato nel dipartimento del Maine e Loira nella regione dei Paesi della Loira.

Società

Evoluzione demografica

Note

Altri progetti

Collegamenti esterni

Saint-Leger-sous-Cholet

redpajama_set_name: RedPajamaWikipedia


Jagadguru Ramanandacharya Rajasthan Sanskrit University, Jaipur formerly Rajasthan Sanskrit University was established in 2001 by Swami Narayan Dasji Maharaj. The university is recognized by the University Grant Commission (UGC). The university affiliates more than 50 colleges/institutions of Acharya, Shashtri and Shikshashatri level. Objective of the university is to develop and preserve the Sanskrit language and also to promote Sanskrit learning in the state. Not declared fit to receive Central/UGC assistance under Section 12 (B) of the UGC Act-1956.
This page was last modified on 28 March 2016 at 16:03.


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text:
Home > Human Resources > Compliance Corner >
Annual Security and Fire Safety Reportplus or minus
The University of Scranton's Annual Security and Fire Safety Report is published each year to provide crime and fire statistics, and information on safety and security related services offered by the University in compliance with the Jeanne Clery Disclosure of Campus Security Policy and Campus Crime Statistics. The report contains information and crime statistics for the three previous calendar years regarding crimes that occurred on campus; in certain off-campus buildings or property owned or controlled by The University of Scranton; and on public property within, or immediately adjacent to and accessible to the campus. The report also contains information regarding campus security and personal safety topics such as crime prevention, fire safety, university police law enforcement authority, crime reporting policies, disciplinary procedures and other information related to safety and security on campus.
The newest edition of the Annual Security and Fire Safety Report has been posted on The University of Scranton Police Department web site, and can be found by clicking on the link below. Printed copies may also be obtained by visiting University Police located at 820 Mulberry St., Scranton, PA 18510. The Annual Security and Fire Safety Report and may also obtain a copy by visiting either the Admissions Office or the Office of Human Resources.
Benefit Notifications: Summary Annual Reports plus or minus
The University of Scranton is legally required to annually provide you with important information about your benefits plans.
Summary Annual Reports
Employees who would prefer to receive the required Benefit Notices in hardcopy should notify the Office of Human Resources at hr@scranton.edu Questions regarding these notices may be directed to the Office of Human Resources.
Benefit Notifications: Summary Plan Descriptionsplus or minus
Summary Plan Descriptions
Form 1095-C plus or minus
Beginning with 2015, the Affordable Care Act (ACA) regulations require large employers, like the University of Scranton, to report certain health care coverage information to full-time employees and to the Internal Revenue Service (IRS).
Each year, the University will mail a Form 1095-C, which contains information about whether or not the University of Scranton offered health care coverage to you and your dependents the previous year. In addition, the form indicates months that you were enrolled in coverage and names the dependents listed on your coverage in Part III. For those staff and faculty who opt-out of the University's health care coverage, the 1095-C will indicate that coverage was offered but not selected.
Please review the information you will receive each year from the University and report any discrepancies to Human Resources.
You should keep this information with your tax records. If you would like general information questions about the IRS 1095 form and how it will be useful for some individuals, we have included the link from the IRS page for your reference.
https://www.irs.gov/Affordable-Care-Act/Individuals-and-Families/Heres-What-You-Need-to-Do-with-Your-Form-1095C
Thank you for your attention and cooperation as we work to maintain compliance with these federal reporting requirements.
Minors on Campus Policy - PA Act 153plus or minus
CHILD ABUSE REPORTING REQUIREMENTS
The University of Scranton maintains its facilities in a manner consistent with its mission of higher education. Although a university is primarily an adult environment, children under the age of eighteen (18) enter campus to visit faculty, staff or students. Children may enter the campus as part of a program, to attend an event, or to use a campus resource.
The conditions in this policy are in addition to any requirements that may apply to other visitors to campus. This policy applies to activities and programs taking place on the campus of the University of Scranton where minors will be present and under the care and control of a University representative, as well as off campus activities that fall under the authority and direction of the University. This policy applies to both programs in which adults have sustained and regular contact with children and programs where the contact with children is less regular. This policy is not intended to apply to:
Programs in which enrolled undergraduate students of the University, or of another university participating in the program, are the only minors participating.
Research programs subject to the review and approval of the Institutional Review Board where minors are the subjects of the research.
Admissions programs designed to attract high school juniors and seniors to the University, family weekend, and such other programs as may be designated by the appropriate divisional vice president in consultation with the General Counsel.
Programs where minors are on campus under the supervision of a parent, guardian, or other authorized adult.
Despite the tailored application of the restrictions set forth herein, the reporting requirement in this policy applies to all University employees and is not limited in any way by the exemption language above.
Minors on Campus Event Registration Form
Minors on Campus Policy
Self-Disclosure Form
Institutional Reporting Policy
Instructions for completing the FBI Fingerprint Background Check
Instructions for completing the Pennsylvania Child Abuse History Clearance
PA State Police Background Check Request Form
Minors on Campus Training
Minors on Campus registration forms should be submitted to hr@scranton.edu, Attn: Elisa S. Tuffy
University Drug and Alcohol Prevention Program Informationplus or minus
Dear Members of the University Community:
Below please find a compilation of information on The University of Scranton's Drug and Alcohol Abuse Prevention Programs. Notice of this information is required by federal regulation and provides a useful resource regarding University efforts in this important area. A copy of this disclosure is available in the Offices of Human Resources (St. Thomas Hall - 100) and Student Life (DeNaples Campus Center – Suite 201) upon request.
Please note, recent changes in Pennsylvania law regarding use of marijuana do not impact this policy. Marijuana remains a controlled substance under Federal law to which the University is subject.
Robert W. Davis, Jr., Ed.D.
Vice President for Student Life
Patricia L. Tetreault, SPHR, SHRM-SCP
Vice President for Human Resources
University Drug and Alcohol Abuse Prevention Program Information
The University of Scranton Drug-Free Workplace Policy
Staff and Administrators Handbook
Alternative Work Schedule
Mission and Community Service Leave
Time Away from Work
Tuition Remission
Adoption Assistance Program
Employee Meal Plan
Employer Assisted Housing Program
Mother's Room
Penn East Federal Credit Union
PNC Workplace Banking
Royal Card Merchant Program Discount
Elective Benefits
Voluntary 403(b) Plan
Employment and Employee Relations
Appearance/Dress Policy
Staff and Administrator Handbook
Holiday Pay Policy and Staff Holiday Calendar
Resources for Harassment and Discrimination
HR News and Updates
United Way Campaign 2020
St. Thomas Hall, Suite 100
To Report Suspected Child Abuse:
Call CHILDLINE: (800)-932-0313
Call Campus Police: (570) 941-7777


text:
Q: No podspec found for `React` in `../node_modules/react-native` No podspec found for React in ../node_modules/react-native
I am getting above error when i do pod install after successful npm install
NPM Version : 5.6.0
Below is the pod file text
# Your 'node_modules' directory is probably in the root of your project,
# but if not, adjust the `:path` accordingly
react_native_path = '../node_modules/react-native'
pod 'Yoga', :path => "#{react_native_path}/ReactCommon/yoga"
pod 'React', :path => react_native_path, :subspecs => [
'Core',
'RCTText',
'RCTImage',
'DevSupport',
'BatchedBridge',
'RCTLinkingIOS',
'RCTAnimation',
'RCTActionSheet',
'RCTWebSocket', # needed for debugging
# Add any other subspecs you want to use in your project
]

end

A: Check that file ../node_modules/react-native/React.podspec is really exists relative to Podfile. If not, check that you package.json really contain react-native as dependency.
For standard RN project directory structure, Podfile should be placed in <projectRoot>/ios/Podfile, and looks like:
platform :ios, '9.0'

target 'CGUI' do
  pod 'React', :path => '../node_modules/react-native', :subspecs => [
    'Core',
    'CxxBridge',
    'RCTAnimation',
    'RCTBlob',
    'RCTText',
    'RCTNetwork',
    'RCTWebSocket',
    'RCTImage',
    'RCTLinkingIOS',
    'DevSupport',
  ]
  pod 'yoga', :path => '../node_modules/react-native/ReactCommon/yoga'
  pod 'DoubleConversion', :podspec => '../node_modules/react-native/third-party-podspecs/DoubleConversion.podspec'
  pod 'GLog', :podspec => '../node_modules/react-native/third-party-podspecs/GLog.podspec'
  pod 'Folly', :podspec => '../node_modules/react-native/third-party-podspecs/Folly.podspec'

  pod 'RNDeviceInfo', :path => '../node_modules/react-native-device-info'
  pod 'RNFS', :path => '../node_modules/react-native-fs'
  pod 'RNVectorIcons', :path => '../node_modules/react-native-vector-icons'
end

This is for RN 0.51.0

A: *

*after successful npm install,

*delete the file podfile.lock in your project root dir,

*then pod install in your project root dir.

this works for me.

A: Go to your project directory
in IOS write command in terminal to open Xcode
open ios/[projectname].xcworkspace

and open Pods folder from the left navigation bar and open Profile file
after that remove the line,
pod 'RNVectorIcons', :path => '../node_modules/react-native-vector-icons'

and rebuild project.


I like them because they are all based on standards that are readily found in real books, they are motivic in their organization, and they come with a pro player performing them on CD. Guitar Guitar Tabs Piano, Vocal, Guitar Acoustic Guitar Bass Guitar Classical Guitar Easy Guitar Electric Guitar Fingerpicking Guitar Guitar Picks Guitar Strings Folk Instruments Accordion Banjo Fiddle Ukulele Strings Violin Viola Cello Double Bass Harp String Quartet Brass Trumpet Horn Trombone Tuba Brass Quintet Chamber Music Woodwinds Flute Clarinet Oboe Saxophone Bassoon English Horn Wind Quintet Percussion Instrument Choir Handbell Choir. Want it delivered by Saturday, 8 July? Most Helpful Customer Reviews on Amazon. Amazon Payment Methods Amazon Platinum Mastercard Amazon Money Store Gift Cards Amazon Currency Converter Payment Methods Help Shop with Points Top Up Your Account. Is the transcription accurate?


text:
Q: Is it possible to get tensrflowp-gpu working on macbook pro with High Sierra I am trying to install tensorflow-gpu  on my macbook pro and have tried pretty much everything which I will briefly mention. But first here is my setup
Macbook pro retina 15"
High Sierra 10.13.4
NVIDIA GT650M card
Over the past two weeks I have  tried all sorts of combinations and fed up with drivers/versions especially with High Sierra 10.13.4 and variables and so on.
If anybody has had success with this please could they tell me or point me to the versions and method for
CUDA
CUDNN
Tensorflow-gpu (understand 1.1 is the highest for mac)
XCode (I have 9.2)
and anything else.
I have my anaconda environment working well for all of the machine learning stuff on CPU and consider using the GPU to be the next challenge.

A: Here's a link that may help.
I have installed using the same guidelines and it's working for me on macbook pro with same configuration.

A: I was able to compile tensorflow 1.4.0 with GPU support for my MacBook Pro (Retina, 15-inch, Late 2013) with GT 750M card under MacOS 10.12.6 with instructions from the following link:
http://paolino.me/tutorial/tensorflow/machine-learning/deep-learning/gpu/2017/11/18/installing-tensorflow-1.4.0-macos-cuda/


You can try to match this piece of gear to Magnificent Mail (Recolor) or Blackforge Mail (Recolor) transmog sets. It's not perfect but looks quite good.
I think it must be a part of .
I think it must be a part of Sparkleshell Mail (Recolor).


Our company promises all users of the first-class products and the most satisfying post-sale service. We warmly welcome our regular and new customers to join us for Stainless Steel Door Accessories , stainless steel door accessories , Stainless Steel Door Retainer , We are assured to generate excellent achievements in the upcoming. We are hunting forward to becoming one of the most reliable suppliers.
"We are committed to delivering easy,time-saving and money-saving one-stop purchasing assistance of consumer for Stainless Steel Door Accessories , stainless steel door accessories , Stainless Steel Door Retainer , Taking the core concept of "to be the Responsible". We will redound up on society for high quality products and good service. We will initiative to participate in international competition to be a first- class manufacturer of this product in the world.


Item has been viewed 3,113 times.
Directions: Heading east on I-40 take exit 290 for US-70N toward Cookeville. Turn right onto US-70N E/E Spring St.for 0.3 miles. Turn left onto Poplar Grove Rd. for 85 ft.. Continue straight onto Bridgeway Dr. for 0.7 miles. Turn right onto Eastlake Dr. for 0.3 miles. Turn left onto Bartlett Dr. for 0.1 miles and the home will be on your right.
Buyers Premium: A 10% Buyer's Premium will be charged on this auction.
County Tax ID: Putnam County Tax Map 082E, Group A, Control Map 082C, Parcel 037.00.
Lot Size: 0.46 Acres±. See Survey in 'Auction Documents' section.
Restrictions: Subject to the Restrictions for Eastlake Estates Subdivision, Phase IV. See Restrictions in 'Auctions Documents' section.
Easements: Any of record see Survey & Plat in 'Auction Documents' section.
Mineral Rights: Unknown. An oil, gas, and mineral title search has not been performed on this property.
Electricity: Service is installed with UCEMC. Call customer service at 931-823-1213 for more information on applicable set-up & deposit fees.
Water: Service is installed the city of Cookeville. Call customer service at 931-526-9591 for more information on applicable set-up & deposit fees.
Natural Gas: Service is available with Middle Tennessee Natural Gas. Call customer service at 931-836-2825 for more information on applicable set-up & deposit fees.
Sewer: Sewer service unavailable; Home is equipped with a 1000 gallon subsurface septic tank located at the front left of the home. See Septic Map in 'Auction Documents' section.
2018 taxes will be prorated to date of deed.
Back taxes (if any) will be paid by the Seller.
Thursday December 06, 2018 from 2:00PM to 4:00PM C.T.
Extended Bidding: Each item in this auction is subject to a Soft Close, meaning any bid arriving within the last 10 minutes of the item's closing time, extends the time that item is open by 10 minutes.
Auction Ending – Real Estate: Beginning at the stated closing time, the auction software will conclude bidding for the auction lots with the following exception: if a bid is placed in the last ten (10) minutes remaining for any of the auction lots, bidding for that lot will remain open for an additional ten (10) minutes. Example: Auction ending time is 10:00 AM. A bid is made at 9:57 AM. The bidding is then extended to 10:07 AM.
Auction Ending with Timed Ending - Real Estate: 'Timed Ending' is a feature where the Auction Ending time for multiple lots is linked together. Should a bid be placed on any lot in the last ten (10) minutes remaining, bidding for ALL lots within that 'Timed Ending' will remain open for an additional ten (10) minutes. The lots that are contained within any 'Timed Ending' will be indicated in the Description field by a 'TIMEDENDING' in the bottom right of the field. Example: Auction ending time is 10:00 AM. A bid is made at 9:57 AM on at least one of the 'Timed Ending' lots. The bidding is then extended to 10:07 AM for ALL lots within that 'Timed Ending'.
Buyer's Premium: A 10% Buyer's Premium will be charged on this auction.
Closing: A Cash Closing will be handled by the BUYERS closing agent, and at the BUYERS expense. A Closing involving Financing will be handled as required by the BUYERS Lending Institution and at the BUYERS expense. If the property is sold in multiple tracts and each tract is sold to the same buyer the 2018 Property Taxes to be prorated to date of closing. If tracts sell to multiple buyers, 2018 taxes will be paid by Seller. Back taxes and Greenbelt Rollback Taxes, if any, will be paid by the Seller. If the property sells as one tract the 2018 Property Taxes to be prorated to date of closing. Back taxes, if any, will be paid by the Seller. The balance of the purchase price shall be paid at or before closing. Closing shall take place on or before 30 days after end of auction, unless otherwise stated in the Sales Contract (see Auction Documents section). The Escrow Agent will schedule and conduct the closing.
Page last refreshed Fri, Apr 19, 9:43am CT.


text:
Saturday 28th June - The Roses at Harlow Carr
It seems like a long time ago now (summer's flown!) but let's look back to the end of June and our meeting at Harlow Carr Gardens in Harrogate. Our June workshop was a repeat of last year's hanging baskets, and this year we were lucky enough to make them in the stunning surroundings of the RHS gardens at Harlow Carr. It was actually a great opportunity to see the gardens in early Summer, when everything was beautiful, fresh and blooming.
Before we got down to business with our baskets we held our usual meeting first, in a very nice room set aside for us in the swish Learning Centre. We ran through a bit of a pared down agenda (this was mostly a day out for us, after all!) and then settled down for a talk from our guest speaker, Dr Eleanor, a GP who'd kindly joined us to talk about women's health issues. There was a fair bit of giggling and groaning as we lamented what lies in store for us girls as we age - one or two uttered comments like "well that's me done for then" or "I'll book myself into Dignitas now" (we all deal with these things in different ways don't we?!) - but hopefully Dr Eleanor knew that we really appreciated her visit, and we do know that information is always a good thing!! A big thank you to the doctor, and we hope that she enjoyed her visit - we did let her make a hanging basket with us after, we're that generous.
Once the making of the baskets got under way, it was the usual mad free-for-all that these events always seem to be. Frantic bagging of plants... more mess than we could have imagined... not helped by the fact that many of the plants were entombed in polystyrene that literally had to be smashed up to get the goods out. Yes, we trashed the place, but you wouldn't have known it after the clean-up, honest. We all produced a pretty basket in double-quick time, and then enjoyed a walk around the gardens together. We even managed a sit down with a Betty's ice cream.
Special mention has to be made of Val Codling, who revealed herself as 'The Mad Bird Lady of Moortown' after showing up to the meeting with a tiny, scrawny, unidentified nestling, which she carried around with her all day in a woollen beanie hat lined with a piece of feather boa! She devotedly fed the little tweeter worms and offered drops of water from a tiny paint brush every half hour, prompted by her phone alarm. Crazy, but very nice, lady!
Since June we've had a bit of a Summer hiatus, but we'll be back at our church hall on Saturday 30th August with a packed programme - two speakers, plus cheese-tasting with Hayley & Clifford and (the one that everyone's been waiting for) wine-tasting courtesy of Majestic Wines. Can't wait!


text:
Q: How To make scope of variable Global(Without making it actually Global) How can I make scope of a String variable(In Java) global.So that it is accessed from another function
Eg
//String b="null"; I don't want to do this... because if i do this, fun2 will print Null

    public int func1(String s)
    {

    String b=s;

    }

    public int func2(String q)
    {

    System.out.println(b);//b should be accessed here and should print value of s

    }

Any Help... Thanks

A: One of the fundamental concepts in OOP is the concept of scope: in almost all cases it is wise to reduce the scope of a variable (i.e. where it is visible from) to its minimum viable range.
I'm going to assume you absolutely require the use of that variable in both functions. Therefore, the minimum viable scope in this case would cover both functions.
public class YourClass
{
   private String yourStringVar;

   public int pleaseGiveYourFunctionProperNames(String s){
      this.yourStringVar = s;
   }
   public void thisFunctionPrintsValueOfMyStringVar(){
      System.out.println(yourStringVar);
   }
}

Depending on the situation, you must assess the required scope of a variable, and you must understand the implications of increasing the scope (more access = potentially more dependencies = harder to keep track).
As an example, let's say you absolutely needed it to be a GLOBAL variable (as you call it in your question). A variable with Global scope can be accessed by anything within the application. This is exceptionally dangerous, which I will demonstrate.
To make a variable with global scope (there are no such things as global variables, exactly, in Java), you create a class with a static variable.
public class GlobalVariablesExample
{
   public static string GlobalVariable;
}

If I were to alter the original code, it would now look like this.
public class YourClass
{
   public int pleaseGiveYourFunctionProperNames(String s){
      GlobalVariablesExample.GlobalVariable = s;
   }
   public void thisFunctionPrintsValueOfMyStringVar(){
      System.out.println(GlobalVariablesExample.GlobalVariable);
   }
}

This can be exceptionally powerful, and exceptionally dangerous as it can lead to weird behaviour that you do not expect, and you lose many of the abilities that object oriented programming gives you, so use it carefully.
public class YourApplication{
    public static void main(String args[]){
        YourClass instance1 = new YourClass();
        YourClass instance2 = new YourClass();

        instance1.pleaseGiveYourFunctionProperNames("Hello");
        instance1.thisFunctionPrintsValueOfMyStringVar(); // This prints "Hello"

        instance2.pleaseGiveYourFunctionProperNames("World");
        instance2.thisFunctionPrintsValueOfMyStringVar(); // This prints "World"
        instance1.thisFunctionPrintsValueOfMyStringVar(); // This prints "World, NOT Hello, as you'd expect"
    }
}

Always assess the minimum viable scope for your variables. Do not make it more accessible than it needs to be.
Also, please don't name your variables a,b,c. And don't name your variables func1,func2. It doesn't make your application any slower, and it won't kill you to type in a few extra letters.

A: Hmm. You clearly need some lessons in object-oriented programming. In OO there is no "global" variable. But any variable defined as a member in a class (outside a method) is global within that class.
public class MyClass {

    private String myVar; // this can be accessed everywhere in MyClass

    public void func1(String s) {
        myVar = s;
    }

    public void func2(String q) { // why is q needed here? It's not used
        System.out.println(myVar);
    }

}

So func2 will output the value of s ONLY IF you call func1 first.
final Myclass myClass = new MyClass();
myClass.func1("value");
myClass.func2("whatever"); // will output "value"

Also, why are the methods returning int in your example? They should be void.


Whether you are coming to bootcamp to join us for a day or a week you will work hard and have lots of fun at the same time. There a lots of varied fitness sessions and workshops. You will leave us you with lots of new knowledge and the motivation to maintain your fabulous and healthy lifestyle.
When you arrive at BMR we will get you settled into your room. You will be given a tour of the facilities and we will introduce you to the team and your fellow Re-Booter's.
You will have a 1-2-1 session with your Personal Trainer and the option of a full body composition analysis.
You will then get straight into the programme with your first training session.
At the end of the day you will enjoy a delicious and nutritious dinner. In the evenings you will have time to to chill out in your room, go for a walk or relax in the hot tub.
Here is a list of the kit you will need to bring with you.
During your down time you can take the opportunity to go out for a walk, read a book, watch a movie or relax in the hot tub. You can also book the following treatments during your stay with us.
Bookings can be made before you arrive, simply contact us with your requirements. If you want specific treatments that are not listed please let us know and we will do our best to accommodate you.


This image is collection of reference materials and resources to assist our study and expression of the Subtle Realm.
It is not complete and is only meant to help facilitate learning, discussion and exploration. Please note that after a long history of multiple models of the chakras from a variety of schools, this is the map that won.
Chakra means "wheel" or "circle". The chakras are dynamic vortices of prana where the nadis converge. Attention to these centers is believed to assist in awakening our consciousness to deeper and more subtle dimensions within ourselves and the cosmos. Specifically, the chakras are believed to assist in moving the prana between the physical, astral and causal realms.
Just as our collective hip joints differ slightly in their shape, flexibility and strength, so do our chakras. And just as our hip joints perform basically the same function, so do our chakras. And just as we have a choice to allow our hips to tighten and close or open and move, so we also have the choice to ignore or connect and develop a relationship with our chakras.
Allow the information about the chakras to be there when you need it. Filling our minds with facts about the chakras does not draw us any closer. In fact, knowing the data can create an illusion of intimacy. Like reading books about swimming, nothing compares to diving in.


text:
'use strict';

Object.defineProperty(exports, "__esModule", {
  value: true
});
exports.default = differenceInCalendarISOWeeks;

var _index = require('../startOfISOWeek/index.js');

var _index2 = _interopRequireDefault(_index);

function _interopRequireDefault(obj) { return obj && obj.__esModule ? obj : { default: obj }; }

var MILLISECONDS_IN_MINUTE = 60000;
var MILLISECONDS_IN_WEEK = 604800000;

/**
 * @name differenceInCalendarISOWeeks
 * @category ISO Week Helpers
 * @summary Get the number of calendar ISO weeks between the given dates.
 *
 * @description
 * Get the number of calendar ISO weeks between the given dates.
 *
 * ISO week-numbering year: http://en.wikipedia.org/wiki/ISO_week_date
 *
 * @param {Date|String|Number} dateLeft - the later date
 * @param {Date|String|Number} dateRight - the earlier date
 * @param {Options} [options] - the object with options. See [Options]{@link https://date-fns.org/docs/Options}
 * @param {0|1|2} [options.additionalDigits=2] - passed to `toDate`. See [toDate]{@link https://date-fns.org/docs/toDate}
 * @returns {Number} the number of calendar ISO weeks
 * @throws {TypeError} 2 arguments required
 * @throws {RangeError} `options.additionalDigits` must be 0, 1 or 2
 *
 * @example
 * // How many calendar ISO weeks are between 6 July 2014 and 21 July 2014?
 * var result = differenceInCalendarISOWeeks(
 *   new Date(2014, 6, 21),
 *   new Date(2014, 6, 6)
 * )
 * //=> 3
 */
function differenceInCalendarISOWeeks(dirtyDateLeft, dirtyDateRight, dirtyOptions) {
  if (arguments.length < 2) {
    throw new TypeError('2 arguments required, but only ' + arguments.length + ' present');
  }

  var startOfISOWeekLeft = (0, _index2.default)(dirtyDateLeft, dirtyOptions);
  var startOfISOWeekRight = (0, _index2.default)(dirtyDateRight, dirtyOptions);

  var timestampLeft = startOfISOWeekLeft.getTime() - startOfISOWeekLeft.getTimezoneOffset() * MILLISECONDS_IN_MINUTE;
  var timestampRight = startOfISOWeekRight.getTime() - startOfISOWeekRight.getTimezoneOffset() * MILLISECONDS_IN_MINUTE;

  // Round the number of days to the nearest integer
  // because the number of milliseconds in a week is not constant
  // (e.g. it's different in the week of the daylight saving time clock shift)
  return Math.round((timestampLeft - timestampRight) / MILLISECONDS_IN_WEEK);
}
module.exports = exports['default'];

redpajama_set_name: RedPajamaGithub


text:
Paul Johann Ludwig Heyse
The German author Paul Johann Ludwig Heyse (1830-1914) is best known for his novellas. Marked by careful construction, nobility and dignity of content, and economy of form, these works reveal his relation to the classical tradition.
Paul Heyse was born in Berlin on March 15, 1830. The son of a professor, he pursued studies leading to a doctorate in philology. During an extended visit to Italy in 1852, he determined to abandon formal scholarship for a career in literature. In 1854 he was summoned to Munich by Maximilian II, king of Bavaria, who granted him a lifetime stipend. His subsequent career as a leader of the Munich Poets' Circle was marked by professional and popular success.
Heyse's half dozen novels avoid the political and sociological and tend to emphasize ethical views and goals. Kinder der Welt (1873) attests to his advocacy of "nature" and individual "freedom" as criteria in opposition to religious dogmatism. Im Paradiese (1875) is anti-Philistine in its ethical orientation. The element of classical balance and restraint and his opposition to the tenets and tactics of naturalism emerge in the novel Merlin (1892).
In his 120 novellas Heyse's imaginative and formalistic gifts are most fully realized. Here, too, his emphasis upon freedom, individuality, and instinct comes to the fore, although instinct is not presented as incompatible with spirituality or a sense of duty. Even the humblest or most unfortunate characters are endowed with dignity and nobility, which can provide a redemptive force if the individual remains "true to himself." L'Arrabbiata (1852) is perhaps his most famous novella.
As coeditor, Heyse published two extensive collections of 19th-century novellas: Deutscher Novellenschatz (24 vols., from 1871) and Neuer deutscher Novellenschatz (24 vols., 1884-1888). In his introduction to the former work he describes his "falcon theory" of the novella, advocating the utmost simplicity and clarity of content and form and urging the necessity for an inward conflict culminating in an abrupt turning point or change, which should be represented by a concrete symbol (as the falcon in a Boccaccio story).
Heyse's 60 carefully constructed dramas and many lyrics lack force, but his translations from the Italian poets are admired. In 1910 Paul Heyse received the Nobel Prize for literature. He died in Munich on April 2, 1914.
Further Reading on Paul Johann Ludwig Heyse
Georg Brandes's essay "Paul Heyse, " reprinted in his Creative Spirits of the Nineteenth Century, translated by Rasmus B. Anderson (1923), is an enthusiastic appreciation. A balanced view of Heyse as author and theoretician is in E. K. Bennett, A History of the German Novelle (1934; 2d ed. rev. 1961).


text:
Bow Bridge, Central Park, New York City in Winter
winter Monday, December 24, 2018 0
The Bow Bridge, which finished construction in 1862, is a bridge with a Classical Greek design and is named for its shaped.
Other quick facts about the bridge:
The bridge is made of cast iron.
It was constructed instead of a suspension bridge that was originally planned.
The eight cast iron urns are replicas of the originals and were installed in 2008.
The original urns disappeared in the early 1920s.
The street view panorama was taken during the January 2016 blizzard
Learn more about Bow Bridge at:
http://www.centralparknyc.org/things-to-see-and-do/attractions/bow-bridge.html
https://www.centralpark.com/things-to-do/attractions/bow-bridge/
Other interesting views of Bow Bridge and nearby points.
From Bow Bridge at Sunrise
Bow Bridge at the Gazebo
Bow Bridge - Central Park
Labels: New York City, winter
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text:
1 Albert Pease Petition recommending the appointment of George A. Smith to the office of register of deeds within Franklin County. 1868
2 Albert Pease Requesting the appointment of J. M. Pease to solmenize marriages along with accompanying papers. 1872
3 Burleigh Pease Recommending the appointment of David Worcester to the office of Superintendent of Common Schools. 1859
4 E. Pease Petitions recommending the appointment of Cyril Pearl to the office of Superintendent of Common Schools. 1864
5 G. L. Pease Petition recommending the appointment of Jotham S. Gould to the office of register of deeds for Franklin County. 1868
6 J. M. Pease Petition to recommending the appointment of Joseph W. Holden to the office of Trial Justice. 1872
7 Joel C. Pease Recommending the appointment of Joel C. Pease to the office of Justices of the Peace and of the Quorum for Penobscot County. 1872
8 L. C. Pease Petition recommending the appointment of T. R. Siminton to the office of County Attorney for Knox County. 1860
9 L. C. Pease Petition of the City Council of Rockland request all citizens of Rockland who have applied or who may apply for appointment to any one of the several offices in Knox County to withdraw their name for the betterment of the Republican Party. 1860
10 Moses Pease Petition recommending the appointment of Oscar D. Turner to the office of Trial Justice for Androscoggin County. 1872
11 Nathaniel Pease Petiton recommending the appointment of Nathaniel Pease to the office of Trial Justice. 1860
12 Nathaniel Pease Certificate to Senators elect. 1860
13 Priam Pease Petition recommending the appointment of Davis Tillson to the office of Clerk of the Courts. 1860


In this limited edition range, the classic design aesthetic of Lyle & Scott has been combined with Attaquer's technical cycling knowledge. Inspired by Lyle & Scott's heritage in knitwear, this cycling jumper is crafted from a breathable cotton knit. A bold stripe design will turn heads wherever and whenever you ride.


Pastor Chris Oyakhilome- the founding president of Believers' Loveworld Incorporated, also known as Christ Embassy, is one of Nigeria's most notable religious figures. As such, he published influential books, has participated in an initiated local and global philanthropy events, concerts, seminars, and TV projects. Some of them include the Healing School, International Easter Youth Camp and Worship and Communication Services.
As a PR company, Muller&Green was in charge of the promotional activities, surrounding the launch of Pastor Chris Oyakhilome's new television channel – LoveWorld USA that took place in 2017. Part of the campaign, designed by Muller & Green featured journalists and media representatives reach-out, influencer relations, initiating online press conferences, interviews and securing the international media coverage.


Here is just a short quip to help lighten the load for Alex Jones listeners.
Perhaps it would be helpful if people thought of Alex "the Drama Queen" Jones in a different way as they are listening to his daily diatribes. Instead of getting sucked into his vortex of gloom and doom and non-stop drama, think of him as the pesky TV commercial spokesperson with an ATTITUDE. Here, let's imagine a commercial about dogs with fleas.
ALRIGHT!!!! LISTEN UP ALL OF YOU TRENDY, LIBERAL, sandal wearing, Cappuccino slurping, dog owners. Your four-legged poop factory named "Fluffy" has fleas and it's high time that you "TAKE ACTION" and I mean NOW!!!! I've studied fleas for decades and I TOLD YOU 5 years ago that this would happen. I told you 1 year ago! I told you 6 months ago!!! I TOLD YOU that the Globalists and the Bankers are responsible and NOW LOOK.... "Fluffy" has the fleas that I warned you about!!! I want you to "TAKE ACTION". Tell your neighbors, tell your friends, get this message OUT THERE to EVERYBODY. Make this message go VIRAL!!!
The moron police K-9 units are going to SWAT team your home if you don't "TAKE ACTION NOW"!!! If there is one thing that they hate more than the Constitution, the Declaration of Independence, and the Bill of Rights, it's sandal wearing Yuppies with flea bitten dogs. This is a RED ALERT!!!
We have a video about Fleas at our website. Get it now. Make copies. Give them to everybody. "TAKE ACTION".


Around 1500 people attended the funeral of Father Leo Donnelly, Emeritus Parish Priest of St Agnes' Parish of Port Macquarie, who died aged 91 at St Vincent's Hospital in Sydney on 23 January.
His Requiem Mass on 1 February at St Agnes' was celebrated by parish priest Father Paul Gooley and assistant priest Father Peter Wood with Bishop of Lismore Gregory Homeming OCD and 23 other clergy.
The service was broadcast live on the St Agnes' Parish website and streamed via Facebook, allowing residents in the parish's aged care facilities and thousands of people further afield, including parishioners on Lord Howe Island (which is part of the St Agnes' Parish) and others overseas, to join in honouring Father Donnelly's life.
Two of Father Donnelly's nephews, Matthew and Anthony Donnelly, delivered the eulogy while other family members led the prayers of intercession and offertory procession.
Matthew remembered the special place Father Donnelly held in the hearts of his family.
Father Leo Donnelly pictured with his beloved dog Shannon.
"Uncle Leo had an authority about him but it wasn't just because he was a priest; it wasn't his intelligence; or his physical presence; it was his unending kindness and compassion; and, his ability to always see the good in every person," he said.
Anthony told anecdotes about Father Donnelly's humour and of other treasured times spent with his uncle.
"I loved it when I got to drive Uncle Leo home after sharing a Sunday evening meal with our family – it was 25 minutes of one-on-one time spent in conversation with him about faith and the things that mattered," he said.
In his homily, Father Gooley spoke of Fr Donnelly as a priest, mentor and friend.
"Leo was a man of prayer," Fr Gooley said.
"Cardinal Newman, to whom Leo had a devotion, wrote 'God has created me to do Him some definite service. He has committed some work to me, which He has not committed to another. I have my mission. I may never know it in this life, but I shall be told it in the next. I am a link in a chain, a bond of connection between persons'.
"This is true of Leo and his life, as it is true of all of us as we continue the mission of Jesus Christ.
Bishop Homeming said Father Donnelly's impact on the community was evident in the diversity of mourners.
"Father Donnelly was a driving force behind improvements to education, training, aged care, welfare and sport in the community," he said.
Adam Spencer, chief executive of St Agnes' Parish and close friend, said Fr Donnelly would be a great loss to the community and was "without peer" in terms of what he achieved in the areas of aged care, early education, vocational education and training, community services and more.
Following the funeral hundreds of people including St Agnes' Parish parishioners, staff, teachers, students, and community members formed an honour guard that extended along nearby streets.
Father Donnelly was parish priest of St Agnes' Parish for 48 years, from 1970 until his retirement in March 2018.


The Hospital Quirónsalud Torrevieja launches a new edition of the free campaign for early diagnosis of prostate cancer on the occasion of the world day of this pathology, which is celebrated on September 15. The initiative consists of carrying out free PSA tests and consultation with the urologist with prior appointment requests to males from the general population and patients from the hospital center aged 45 and over, and from 40 years if they have a family history.
Thanks to the PSA, which is measured in a simple blood test, the specialist can establish the value of this protein synthesized by the prostate, whose value increases in the presence of a tumor. As explained by Dr. Sven Petry, head of the Urology Unit at Hospital Quirónsalud Torrevieja. "The fact that the tumor cells produce it in greater quantity can determine in which people it is more probable to find this type of cells and decide to investigate or not the presence of these cells, by means of a prostate biopsy, depending on the potential benefits and risks that may derive from their diagnosis and treatment. " PSA levels increase with age, so that men without prostate cancer will have higher PSA values as they get older: "If at forty-five years old we consider a normal index a value of less than 1.5, until sixty-five years old this index of normality moves to 2.5 and so on," explains the specialist.
The objective of the campaign is to raise awareness among the population about the importance of prevention and early detection for a good prognosis of this disease. The intention is "to inform and raise awareness in society about prostate cancer, since there is a low perception of the risk of suffering from it. Curing prostate cancer is possible if it is detected early, "explains Dr. Petry.
Prostate cancer is the second most common cancer in the world in men and the first in incidence in Europe. Each year about 25,000 new cases are diagnosed in Spain, of which between 20% and 30% are patients who have relapsed in the disease. "However, when detected early, this tumor can be cured in 90% of cases," cautions Dr. Petry. Prostate cancer, except for advanced stages, rarely produces any symptoms; hence the importance of PSA, which allows the early detection of this disease in asymptomatic patients.
It is not necessary to go on an empty stomach and it will be performed at Hospital Quirónsalud Torrevieja. The analytical period will be from September 10 to 14 and interested persons may request information from Friday, September 7 from Monday to Friday from 10 am to 2 pm. Calls will be made through telephone 966 90 95 06, in the email prevencion.trv@quironsalud.es or through the web http://www.quironsalud.es/torrevieja/es.
Quirónsalud is the most important hospital group in Spain, and the third largest in Europe. It can be found in 13 autonomous communities in Spain, has state-of-the-art technology and offers over 6,500 beds in more than 100 healthcare centres, such as Fundación Jiménez Díaz, Hospital Universitario Quirónsalud Madrid, Hospital Universitario Dexeus, Ruber, Centro Médico Teknon, Hospital La Luz, Policlínica de Guipúzcoa, Hospital Quirónsalud Valencia, etc., as well as a huge team of highly qualified professionals of international prestige.
We promote teaching (seven of our centres are university hospitals) and medical and scientific research (we run the FJD [Spanish acronym, Jiménez Díaz Foundation] Instituto de Investigación Sanitaria [Healthcare Research Institute], the only private research centre licensed by the Secretaría de Estado de Investigación, Desarrollo e Innovación [Ministry for Research, Development and Innovation]).
Likewise, our healthcare service is organised in units and crosscutting networks that allow for the optimisation of accumulated experience at difference centres, and the clinical application of our research. Currently, Quirónsalud is developing many research projects across Spain, and many of its healthcare centres carry out cutting edge work in this field, as pioneers in different specialisations such as radiology, cardiology, endocrinology, gynaecology, neurology, oncology and sports medicine, among others.
How Should You Choose a British School for Your Children?


Beerhouse: The pioneers in the biggest, best variety of beer in South Africa have a new menu. Developed by Beerhouse and the Ultimate Braai Master; Pieter Marais. They have managed to combine the Latin American style of smoke and spice with the rich goodness of beer to create something exceptional. This is something you don't find in South Africa: Latin American style inspired smoke and spice flavours with a South African twist.
This is evident throughout the new menu with beer infused cheese, seasonings of beer through an array of beer brine and fermentation in the form of beer fermented bread and their new signature Beeracha sauce made with beer fermented chili fruit.
With instant favourites like nachos, ribs and pulled pork, let's get down and dirty and delve deeper into the highlights of the new menu.
Pulled pork made with their amazing "beer dust" smoked spice rub. Brisket that melts in your mouth and yet, firm enough to hold. The beautiful proudly South African Beerhouse Boerie made with craft stout beers and notes of coriander.
Pap chips, which is literally chips made from "stywe pap" coupled with chakalaka (This is a must try! Fluffy on the inside and just crispy enough on the outside). The Nachos is paired with beer infused cheese and beeracha crema.
Then the two absolute must try dishes in my personal opinion are the amazing smoked meat and beer cheese BBQ Bitterballen and the Spare Ribs Brew-BQ sauce. There's something beautiful about spice rubbed spare ribs that hit the sweet-spot of tenderness right between dense and falling off the bone.
The new menu unfortunately only lists one dessert: the Beerhouse Beer Float. This is a very pleasant Milk stout with salted caramel and whiskey ice cream, topped with honey comb, grilled marshmallows, and whipped cream.
It's still the same Beerhouse that we have all come to love over the years. There is still a lot of "Gees" with the best options in local and international beers. We might miss a couple of the old favourites like the "oepsies", "flammkuchen" and "malva pudding" but, you will soon find new favourites inside the Brew Food menu with rich beer tastes and vast amounts of smokey goodness.
I will gladly recommend Beerhouse to anyone, this is not just a great place to experience and explore 99 bottles of beer on the wall and 25 on tap, it is truly a great place to go for lunch or dinner to experience smokey culinary creations that stands out from your everyday pub or restaurant.
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BettingBias was formed in 2010 and consists of a group of professional punters, journalists and gambling industry veterans.
The founder is Simon Miller who previously spent six years at Oddschecker.com as Commercial Manager and seven years as a pro punter.
During my six years in the industry I must have come across hundreds of websites run by chancers full of empty promises to make you rich. As a fellow punter I want a betting content website to educate, challenge and entertain me on this fascinating subject. That is what BettingBias strives to deliver. I strongly believe that to get the most enjoyment out of betting you should give yourself the best chance of winning. My passion - horse racing -remains a mystery to millions because very few have taken the time to explain the nuances and complications. It is complexity that makes the Sport of Kings a joy and the more you learn the more satisfying it is to pick a winner. We all want to be successful but the joy is in understanding how and why we got there. This is what we want to share with you, for all sports, all of the time. Enjoy the site.


Do you ever have one of those weeks where you celebrate the fact that you've all managed to survive the week? Well last week was one of those weeks!
I know I have been moaning a little recently due to a long Winter and endless germs, I'm sorry to say this week I can't avoid discussing that subject again! We haven't had a season like this in years, whether it's just one of those years or the fact that we have moved areas and are now susceptible to new germs, who knows! I was unlucky enough to get a chest infection whilst flying solo at home with the kids and felt pretty rotten. Teddy had suspected Chicken pox and so was off nursery, and lastly little Flo was down with a temperature and full of cold. We still don't know if it was chicken pox- myself and nursery think yes, but the doctor wouldn't confirm. Maybe it was just a mild dose and the spots, although very red and lasted a while, weren't itchy. At least little man was cheerful and didn't suffer with them. Once my antibiotics kicked in I convinced the family to get outside into the cold sunny garden, and start clearing all the dead branches away and start making more of our new garden. The two eldest loved helping and enjoyed having a little bonfire with all the wood, and Finlay threw himself into chopping wood like a mini Bear Grylls.
My photo taking was kept to a minimum last week and so these are pretty much all I have of the week. As I'm writing this the snow is falling and I'm spoilt for choice with my many snowy pics of the children!


text:
hijack is a film production company, based in London, specialising in art/science films and installation. The Co-Director's, Gilly Booth and Chris Horrocks, fine art background means they emphasise exploration and experimentation to create inspiring films and multi-media environments which often use technological innovation.
hijack love to collaborate with: Paul Plowman (www.paulplowman.tv) Anthony Burrill (www.anthonyburrill.com) Harmonic Kinetic (www.harmonickinetic.co.uk) Mike Silver (http://www.residentadvisor.net/dj/mickeymoonlight) Jonny Trunk (www.trunkrecords.com) Dacapo (www.dacapo.co) Touchpress (www.touchpress.com) Malcolm Goldie (www.malcolmgoldie.com), Images&Co (53k.co.uk), Ab Rogers (www.abrogers.com) KCA (www.kcalondon.com).
Films and muliti-media installations have been Commissioned and Exhibited by: ICA London, Pompidou Centre Paris, Museum of Modern Art Tokyo, MOMA New York, Serpentine Gallery, Science Museum, Geffrye Museum, Design Council, Design Museum, Dorich House Museum, Rogers Stirk Harbour + Partners, Book Works, Watts Gallery, Paolozzi Foundation, Venice Architecture Biennale, and International Film Festivals .
Awards received from: Lottery Arts Council of Wales, Heritage Lottery Arts Council, Arts Humanities Research Council, Arts Council England and Nesta.
Gilly Booth is an artist working with moving image and sound and co-director of hijack film production. She graduated with an MA in Fine Art from the Royal College of Art. She makes films for theatrical release and site-specific digital installation. She has lectured on her work in Fine Art at Kingston University, Chelsea College of Art & Design, Ruskin School of Drawing and Fine Art and Royal College of Art & Design.
"Setting, place or a particular building is often a starting point. Past films have invested in a political language of architecture, especially in relation to 1960s French and Italian film. I use voice over, text/graphics, archive, interview footage and location to create a filmic investigation that destabilizes reality and fiction. The subject is translation, whether immediate or through memory, in order to re-visit lost places, images, a particular film history or an archive, which are then re-mediated for the viewer within a cinematic or installation context."
Chris Horrocks is a writer, filmmaker and lecturer, and co-director of hijack film production. He is Associate Professor and Course Director of the MA in Art & Design History at Kingston University. He graduated in Fine Art at Bath Academy of Art, was awarded an MA in Cultural History at the Royal College of Art. He gained a PhD for his theoretical research at Kingston University. He has published widely in the field of cultural theory. His work has appeared in academic and popular books, radio and press. His publications include Introducing Foucault, Baudrillard and the Millennium, TokyoGlamRock, Marshall McLuhan and Virtuality, Cultures of Colour and The Joy of Sets.
© hijack 2019


text:
Q: Django : How to access a localhost database hosted by a user? I want to develop a website (with it's own database) where all the users will host a tiny database on their computer (SQlite or mySQl). I need to find a way for the users to access their local database and work with it on the website.
I read the docs concerning the multi-database (https://docs.djangoproject.com/en/dev/topics/db/multi-db/) we can in the settings tell to django which database it needs to  connect to.
For example :
DATABASES = {
    'default': {
        'ENGINE': 'django.db.backends.postgresql',
        'NAME': 'mydatabase',
        'USER': 'mydatabaseuser',
        'PASSWORD': 'mypassword',
        'HOST': '127.0.0.1',
        'PORT': '5432',
    }
}

How to tell django to connect to the database hosted by the user ? I assume that 127.0.0.1 will refer to localhost of the django server. Am i right ?

A: I think you misunderstood the concepts behing Django, or backend at all.
Django runs on a host, it could be a server, cloud hosting, on your local machine, etc.. When you use 127.0.0.1 as the database server host address, you are targeting localhost of the host where Django is running. You cannot simply start a MySQL server on the client side from django or python, you cannot do anything. You cannot even start a SQLite database as the django simply has no ability to see to user's filesystem.
What exactly are you trying to achieve? If you want to build something on top of a local database, it has to run locally, or you will have to somehow mount the database files to the django, which will be a snapshot instead of realtime change relfection.


We Need to Help Them!
Thank You Donors From Bakersfield!
Massive Amounts of Relief Supplies May Still Sit In Warehouses!
Typhoon Relief Delivered by Dennis Saco and His Team!
Interview: Politics Hampering Relief Effort!


FC Comets away in Ickleford was the venue for the U8 Blacks this morning, and management were hoping that a weeks rest from school would see the boys refreshed and ready to go. A poorly Louis meant we were down to six but the boys were determined to make the most of it. Stanley scored in the opening minutes, shortly followed by a left footed goal from Liam. Harry scored again in the first quarter and the boys were doing well. Second quarter and a great shot from Charlie followed by another from Liam meant the boys were looking comfortable at half time. At this point Hares decided to move the players around allowing William to come out of goal, replaced by our ever dependable Reggie, who demonstrated yet again how to play well in goal! William was soon involved in the action and scored a great goal. 3/4 time and Hares looked good, but then watch out boys as FC Comets were not giving up. Overall a great morning of football enjoyed by all, well done boys, see you all at home to Letchworth next week. POTM Harry with Liam voted POTM by FC Comets.
Hares U12 Yellows travelled to Walkern today and started the brighter of the 2 teams and were rewarded when Francis scored early on. Hares continued to dominate only for the home side to equalise. Hares retook the lead straight away when Harry stabbed in the rebound from a Francis freekick. With the game turning scrappy on what was a very poor pitch, Hares added to their tally with a great finish from Zane, only for the opposition to quickly respond. The boys stayed strong under pressure, working hard when needed. The final 10 minutes was all Hares with late goals from Beeshman and Francis. MOTM today went to Toby for excellent work at the back.
The Under 14's travelled to Hitchin Town this weekend looking to extend their unbeaten run in the League. The game started well for The Hares and they found themselves 1 up after 3 minutes when Joey Wedge netted his 14th League goal of the season. With the Hares enjoying the majority of possession it was surprising that it took another 15 minutes to add their second of the game when George Clark slotted home. A minute later 0-2 became 0-3 when George Clark was involved again, this time by running on to a through ball from Jake Craddock-DeBois and despite the keeper making a save from his shot, Jamie Lynch was in the right space at the right time to score. Despite The Hares being 3-0 up and coasting it was Hitchin who began to look the better side, and deservedly pulled a goal back to make it 1-3 at the break. The second half began as the first had finished, and The Hares were doing their best to allow Hitching to get themselves back into the game, however Joey Wedge added his second of the game to make the final score 1-4 to the visitors. The result keeps the Hares at the top of their league having won 5 and drawn 1 from their 6 games played so far. MOTM this week went to Joey Wedge.