Pattern - Gardens aren't only for lawns and household play fields, but can certainly be perfect locations for storage sheds wherein anybody can just basically stock unused household stuffs while in the shed. As part of the entire house exterior, it is merely but proper that garden sheds will also look presentable and in-relative towards house's design.
So as not being a total complete eyesore, garden shed designs needs to be well-planned. Shed plans needs to be harmoniously with possible space in the garden as well as the design befitting the house's style. Furthermore, garden shed designs should serve its purpose to the owners in general.
* Space. Just before a single cause his/her very own storage area putting together designs, one particular has now any approximate involving originates from in which the garden lose will undoubtedly be placed. In addition to the area available, establish also which unfortunately section of the garden plants it's going to be located. Guarantee that it will not be found some time close main road to be able to eliminate block of the process within the future.
* Layout. On the sheet of paper, contain a theme in your garden shed designs. One needs not really that they are a powerful architect and / or electrical engineer for this purpose question; an style and design connected with the backyard storage shed - including what seems as if - will do considering the fact that the following will simply serve as strategies for this carpenter and / or stylish inside constructing any shed. If one is extremely very involved over it, he/she can easily employ the service of a fabulous trendy or architect to create these outdoor garden shed plan.
* Materials. Inside storage space making designs, add be familiar with components which usually that appeals to you intended for your garden storage devices shed. Most of which really are produced fire wood as timbers are generally looked at simply because most suitable equipment for one flowerbed safe-keeping shed. Aside from the proven fact that woodlands seem to be lower priced, it will also fit properly with the habitat from a backyard garden where tones connected with natural plus soil hues occupy typically the area. A good idea is, on the other hand, helping put wood treatment plans using some areas of a garden safe-keeping shed. This is exactly to stop pest infestations as well as residence pests in getting into your woods.
If you fail to achieve it without any help, find someone who may be acquired together with competent inside woodwork and then making storage containers sheds. Seek seriously trained those that could certainly construct a garden storage shed. This does not exclusively encompass the tough back garden outdoor garden shed end product, but also a fabulous preserving as a result of time after materials used.
Popular yard drop layouts nowadays add some A-frame variety as well as barn-style sheds. You can also get various other looks for example family pet barns, saltbox greenhouse, playhouses, cottage, pool cabanas, or maybe a small option of yours house. Garden storage devices can be tailored with a porch along with other accessories. When viewing backyard storage shed types, investigate the things every different developer is required to offer.
For just a garage storage shed when you would like to school yard gadget cars, bicycles, motorcycles, and in some cases passenger cars, there are shed kits which come in various sizes available. In opting for, you would probably needless to say be required to numeration the number of cars or trucks from the household. Often, shed outdoor garden sheds also are intended to accommodate crash restoration programs, elements, materials, as well as cleansing equipment. Considering the fact that car port outdoor sheds are generally appreciated for their inside excellent, exterior types are generally very little and then simplistic.


At Dumpster Blog, we strive to bring you the best service at the best price available. We have a wide selection of dumpster sizes in stock in Newfields, NH, with flexible & timley pickup and delivery. Give us a call today for all your dumpster rental and roll off needs.
Dumpster is a wonderful handy application in discarding the trash simple at very affordable cost. Dumpster rental organizations make dumpsters easily obtainable in different sizes geared to the designed needs of the customers. Dumpsters are prepared for any type of trash however large it is, however they have limits on the tonnage of the trash treated by these. You have to be certain to choose the right type of dumpster that fits within your requirements.
That especially comes about when the tonnage of trash thrown away is very large like design project particles. Roll down dumpsters are usually meets for these types of projects, they may be enclosed using two entries on at the bottom to get rid of heavy trash and one on the top to remove light weight. Breaking the trash into small servings will leave room for the further trash to the dumpster. If your trash includes something such as plywood, be sure that you place the trash at the bottom of the roll down so that they stop working into tiny pieces creating an extra room for your trash.
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Remember to verify which what you prepare to put in the Cost of a Roll Off Dumpster in Newfields, NHs, garbage container rentals or perhaps disposal bins are allowed. You additionally want to confirm the pricing beforehand and allow the actual sales person describe your options pertaining to sizes and exactly how much. Most companies that concentrate on Cost of a Roll Off Dumpster in Newfields, NHs or perhaps garbage bin accommodations in various urban centers and suggests have unique bases for his or her charges. A number of charge per week, others only for each weight taken away. A number of charge from the ton or perhaps material broke up with. Obviously, you would like to ask about you can actually charging design when you are scheduling and figure out which package goes to suit your needs the very best. You would detest to find out your day you are taking your party, or perhaps tearing along your garage area that you are powerless to use the dumpster or perhaps garbage bins for your reason you actually intended.
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Lease Duration: How long do you need the actual dumpster for? Dumpsters is usually rented from the month or perhaps on a long lasting basis (typically with a 12-month contract). Keep in mind that when you keep a short-term roll-off longer than the actual previously approved lease timeframe, there can be extra charges of the average $15-$50 every day.
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Home	General	Raquel Vendome and The Concept behind the Habitable Structure – Raquel Vendome's Desire to Continue Her Father's Legacy
Raquel Vendome and The Concept behind the Habitable Structure – Raquel Vendome's Desire to Continue Her Father's Legacy
by Olufisayo June 4, 2018
written by Olufisayo June 4, 2018
Combining architecture with modern day art, the Habitable Structure is one of Philip Johnson's last works before he passed away. The concept of the building was achieved based on the idealism proposal of Raquel's father, real estate developer Antonio 'Nino' Vendome.
Working closely with Alan Ritchie, Johnson created an elaborate design that mixes the aesthetics of cubism. The inspiration behind the design was taken from the works of pioneering artists Georges Braque and Pablo Picasso who greatly influenced modern art.
Following the death of Johnson in 2005, successful entrepreneur and real estate developer Antonio Vendome wants to see one of his last works erected in the New Manhattan area. He also envisions establishing the same structure across countries to herald the new dawn of architectural genius the late designer will be known for.
Johnson's creative and distinctive ideas are seen as a pioneering push in the concepts of modern building construction. His Glass House in New Canaan, Connecticut has been widely acclaimed in the architectural industry for its perfect proportion and simplicity. Completed in 1949, the Glass House and the nearby structures created by the creative genius have been declared as National Historic Landmarks.
Through the artistic designs and pioneering works of Philip Johnson, real estate developer Antonio Vendome wants to have five of these buildings erected in the US. He proposes to have them constructed in New York, Washington, Los Angeles, and two other unnamed locations. He also plans to have the buildings built up in five other countries which he still debates on.
In the recent years, Antonio Vendome has been actively involved in putting up a team who would construct the Habitable Structure, and give a new life to the downtown Manhattan area again. His dreams of combining quality and beauty through the works of the late architect and Ritchie would also be a great source of inspiration for the generation to come and give the architectural design a new path in combining arts in the postmodern world of architecture.
Raquel Vendome, as she was growing up, watched her father work tirelessly to turn his vision into reality and achieve what he has accomplished today. Raquel took up Early Childhood Education in college, as she had worked with children for most of her life. However, she eventually chose to pursue a career in real estate.
Antonio's passion was what inspired her to get started in the business. Raquel is currently employed by her father and plans to further her career in this area. She has the will and the desire to expand what Antonio has already established and to keep the family legacy alive, helping foster a business that can transcend generations.
Read more information about Raquel Here.
he Concept behind the Habitable Structure
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Elena Full Movie In Italian Free Download Mp4
Posted by Troy Johnson on October 11, 2018 at 8:18am
Elena Full Movie In Italian Free Download Mp4 ->>> DOWNLOAD
Original Title: Elena
Genge: Action,Adventure,Crime,Drama,Thriller
Rollin Hand is sent to investigate the case of a beautiful Latin American spy who has suddenly started to act suspiciously. Is she still on the right side - and is she losing her sanity?
The IMF are sent to Latin America to investigate the awkward behavior of a female scientist in "Elena". Rollin Hand is up to the task of investigating Dr.Elena Del Barra.He tries to find out what her objective is;her action that she is taking; and to observe clearly as she acts away from her front.
It was a fun episode especially the scenes between Martin Landau and BarBara Luna,who portrays Dr. Elena.The dynamism and chemistry between the two was great and it made the episode entertaining. Dr. Carlos Enero (Barry Atwater) and Rollin Hand (Martin Landau) are the only two members of the team on this mission when it begins at Brigg's apartment. Sure, you see Briggs (Steven Hill) at the beginning and the psychiatrist, but otherwise it's mostly just Rollin behind enemy lines (though the psychiatrist meets him later to examine the suspect). It seems that Elena Maria Del Barra (BarBara Luna) has been working for the US--sending important data for some time from her South American country*. However, lately she's been behaving irrationally--so much so that Rollin's mission is to infiltrate and meet Elena to see if she's lost her mind. Not surprisingly, once he meets her, it's obvious something more is going on in this one. Under the influence of a so-called truth serum, they see that some sort of mind control has been exerted on her. However, they have to sort it out quickly, as another agent has been sent to assassinate Elena if they don't get answers fast!
This episode is different than most because there isn't a lot to the mission. Rollin enters the country and looks to see if Elena is bonkers. There are no gadgets, not a lot of trickery and it's all very straight forward. It's all about determining her competence as well as determining if someone has brainwashed her--all before the assassin does his job. Despite the simplicity of the show, it works well. Not a great episode but a very good one--even with some rather crazy acting!
*While the names of the countries in this series are rarely real nations, this one seems to indicate they are in Peru, as their national drink is called 'Chicha'--a popular beer-like drink that's made in a most unusual fashion (people chew and spit corn into a vessel and then let it ferment--yuck!). I've had Chicha but a more modern version made (thankfully) without spit!
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EVENTING: Rebecca Howard crowned Canadian Equestrian of the Year
Rebecca Howard and Riddle Master. Picture: Libby Law
MARLBOROUGH-BASED Rebecca Howard and her horse Riddle Master have been crowned Canadian Equestrian of the Year and Canadian Bred Horse of the Year respectively at the Equine Canada Annual Awards Gala, held in Winnipeg, Manitoba.
Rebecca and Riddle Master had their best finish when third in the hotly-contested CIC*** at her local Barbury International Horse Trials in July.
Additionally, they finished 12th at both Badminton and Burghley. Riddle Master ended the season at 13th place in the 2013 FEI World Horse Rankings.
After the 2012 London Olympics, where Rebecca and Riddle Master represented Team Canada, they relocated to Tim and Jonelle Price's yard, near Marlborough.
On receiving the Dr George Jacobsen Trophy for the Canadian Equestrian of the Year award, Rebecca said: "I am honoured to receive this award and would like to thank Equine Canada for this fabulous evening and for the recognition. I am also delighted for Caroline Blazely, who owns Rupert (Riddle Master) and has collected his Canadian Horse of the Year Award tonight.
"Caroline has been such an incredible support to me and believed in us from the outset. Furthermore, she is providing a further exciting opportunity for me, Rupert and Canada in 2014.
"In the Chinese Year of the horse, deemed to be' fortunate and magical', what better time to deliver something really exceptional, which I hope will be at the World Equestrian Games in Normandy this August."


DevOps is desired; Security is required. DevSecOps brings them together.
The demand for speed and innovation is everywhere. However, that enthusiasm sometimes creates conflict when it butts up against security, which tends to value the status quo. In some cases, the dogged hunt to increase velocity can introduce new challenges and risks (e.g., skipped process gates, insufficient testing).
The goals of development teams can seem at odds with what security teams need to do. Traditional models of security have certain characteristics (e.g., manual, sequential, segregation of groups, narrow guardrails) that don't always jibe with a development team's thirst for speed, flexibility, and innovation. The result is an all-too-common mindset that "security is blocking the world" ("It doesn't matter how fast we develop, delivery will be halted by onerous security checks and change control").
But it doesn't have to be that way. Especially considering that development, security, and operations teams all strive for the same end state: Fewer vulnerabilities in production.
This scenario applies universally to government agencies and the vast surrounding ecosystem of private industry that advises and performs services related to DevOps, IT modernization, and information security. With a government-wide push for IT modernization, citizen-facing digital services, website modernization, and the fact that many programs rely on producing functional and secure software, agencies want greater DevOps maturity, but they're often unsure how to turn that goal into reality in a world where compliance matters a lot.
Enter DevSecOps, which unites groups around a shared objective: software that is both functional and secure. Agencies increasingly recognize that security plays a key role in software delivery, and therefore it makes perfect sense to "push security to the left" by weaving security steps into developer workflows. The result: faster releases, more secure releases, and the freedom to focus on the mission.
A tidy definition of DevSecOps comes from my colleague Nic Chaillan, who is doing some incredibly pioneering work to build a DevSecOps platform of best-of-breed tools that can be leveraged as a turnkey solution across the Department of Defense enterprise.
The General Services Administration is pursuing a DevSecOps model "that will not only engage Security throughout the development and operations processes, but more specifically, ensure their involvement as we align the Authority to Operate (ATO) process" with its increasing adoption of cloud.
The Department of Homeland Security is working technical and policy angles simultaneously. While its cloud steering group tackles aspects of policy, its Cloud Factory is helping to establish a highly automated, secure, reliable set of managed services that allow for the dev/ops flow, feedback, and innovation of various applications.
A prime example of a thorny issue wrapped up in both technology and policy is everyone's favorite whipping boy: the ATO process. One sticking point is that an ATO is usually good for three years, although it assumes no major changes to a system's cybersecurity posture will be made during that time. When changes do occur, the Authorizing Official might require a reassessment and reauthorization, which impacts project cost and schedule and runs counter to being Agile.
Fortunately, the National Institute of Standards and Technology's Risk Management Framework (RMF), the government's foundation for system assessment and accreditation, encourages an alternative approach to the traditional 3-year ATO process through continuous reauthorization. The daunting and labor-intensive application of RMF controls presents a prime DevSecOps opportunity: automation and orchestration can minimize the release of crappy code (happy Dev!), make the results of security gates a foregone conclusion (happy Sec!), and provide continuous visibility into system changes and security posture (happy Ops!).
People have been using CloudBees or open source Jenkins for a long time, primarily for traditional software development, which makes the DevSecOps use case a novel – and logical – extension of a tool that's familiar the world over. Because of that, pivoting from traditional use cases to the DevSecOps use case feels simultaneously natural and revelatory.
Weave security functions and controls throughout the development lifecycle by plugging security actions into Jenkins pipelines (example below).
Insert automatic and manual gates to ensure insecure or non-compliant software doesn't move downstream.
Integrate approvals, warnings, rejections, and remediation into developers' own tools and workflows.
Visualize software pipeline through the CloudBees Core UI in order to monitor pipeline progress and correlate it back to security checks.
Apply governance protocols like RBAC to provision smartly – and make security staff and sys admins happy.
What's more, CloudBees Core leverages the massive ecosystem of ~1,500 Jenkins plugins to integrate with the most commonly used security tools (see sample below). That means that, no matter the tools in an environment, CloudBees Core can orchestrate them right out of the box.
CloudBees solutions help meet common needs of enterprises embarking on their DevSecOps journeys, as seen below.
Leverages 1,500+ plugins to orchestrate security tools – and can easily extend to integrate with additional solutions – enabling automation of compliance checks and enforcement.
Standardized, templated workflows enable compliance across the application portfolio.
Full end-to-end orchestration and automation of the software development life cycle with Jenkins Pipeline-as-Code and integration into security scanning and testing tools and processes.
Implement Infrastructure as Code for your environments and CD pipelines with integrations to CM solutions like Chef and Puppet, and deep support for containers and Kubernetes to support scalable immutable infrastructure.
Automatic and manual gates ensure that insecure or non-compliant software does not move downstream.
Integrate approvals, warnings, rejections, and remediation into the developers' own tools and workflows.
Empower developers to own the security experience – continuously test code and fix defects – without having to be security experts.
Continuous assurance that software has passed security screening.
Consistent audit trail showing how an application was built over time.
Visualization of the software pipeline through CloudBees Core teams' UI, thereby enabling quick and continuous monitoring.
All builds (job runs) are recorded and logged, including who/what originated an action. Additional log monitoring and analysis provided by CloudBees Jenkins Metrics.
Allow security teams to continuously monitor ATO posture by providing visibility into pipelines that can be correlated back to security checks.
DevSecOps isn'teasy to implement, it requires a commitment to new ways of carrying out a mission. Fortunately, DevSecOps can yield profound benefits to agencies.
DevSecOps might seem out of reach, but don't be fooled! With just a basic CI/CD foundation, security can be pushed to the left and the benefits of "speed to capability" can be had. By automating security/compliance tools and processes, defects due to human error are reduced. Developers can be confident the right security checks have been completed (and acted upon), build a consistent and transparent audit trail showing how applications were built over time, and ensure a system is always worthy of release.
The result? A quicker path from concept to creation, with fewer vulnerabilities released into production, thereby strengthening security posture and decreasing the performance problems that cause outages and bog down security teams and developers alike. Imagine being able to identify and correct flaws early in the delivery process, before they're exposed to the public.
With the astonishing rise of DevSecOps, it's an exciting time to be with CloudBees, teaming with government agencies and service providers to give customers an extraordinary experience.


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Our full length practice test questions are drawn from our pool of 900+ questions and you can take about 6 full-length tests before running out of new questions; however we recommend only taking 2-3 and saving the other questions for more targeted practice. You can also reset your questions and retake tests over and over again. You can learn more about our tests here!
To access practice tests, you can click on the link on the dashboard that says "Take a practice test"-- it's in the Quick Practice section, right above the green Practice Verbal buttons.
We also recommend Powerprep from ETS, which you can find here.


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\section{INTRODUCTION}

An understanding of magnetic structures on the solar surface is important because they function not only as a method of energy storage for various solar surface activities but also as a practical example of a magneto-convection system on the stellar surface.
Although some researches have been conducted from the perspectives of both observation and numerical simulation, many questions still remain.

One such question is the frequency distribution of the flux in the patches \citep{wan1995,sch1997,hag1999,hag2001,par2009,zha2010,iid2012,shio2012}, which is used in this series of the papers as a word corresponding to the magnetic elements, magnetic features, or flux concentrations in the literatures.
In an important discovery, \cite{par2009} reported a power-law distribution with an index of $1.85\pm0.14$ in a flux range of $2 \times 10^{17}$ Mx - $10^{23}$ Mx, namely from the observational limit to the active region.
Several subsequent papers also report similar results within a margin of error \citep{zha2010, iid2012, shio2012, zho2013}.

Despite the accumulation of observational results, the formation and maintenance mechanism of this distribution are still unclear.
\cite{par2009} suggested two possible interpretations.
One is the production of such a power-law distribution in the deeper layer of the convection zone.
This means that the flux supply from the deeper layer to the surface directly forms in the observed power-law distribution.
The other is the production by the surface processes of patches, meaning that the flux supplied from the deeper layer is deformed to the power-law distribution by merging, splitting, and cancellation on the surface.
These interpretations can be discriminated by comparing the timescales of the magnetic flux supply and surface processes.
However, despite the importance of delving further into these findings, such an investigation by counting the processes manually is difficult because such occur at a very high frequency on the solar surface.

Therefore, we developed an auto-tracking algorithm of patch structures and surface processes in the previous paper (Iida et al., 2012; hereafter Paper I).
Note that not only the algorithm but also the stable high-resolution data acquired by the ${\it Hinode}$ allows us to perform a statistical investigation.
The occurrence frequencies of merging and splitting are found to be considerably higher than those of emergence and cancellation.
This result is equivalent with that the reprocessing time scales of merging and splitting are considerably shorter than those of flux supply from a deeper layer, i.e., the observed distribution of flux is nontrivially affected by the surface processes.

Paper I focused only on merging and splitting because the temporal duration of the data was not enough for a statistical investigation of the other processes, i.e. emergence and cancellation.
These dynamic processes are related to various types of energetic events.
They are also considered important for the understanding of flux transport, in that they represent flux supply and removal from the solar surface \citep{liv1985, mar1985}.

Flux emergence, defined as the appearance and separation of opposite polarities, is thought to be the origin of magnetic flux on the solar surface.
It is a highly visible phenomenon with its distinct features in magnetogram images.
The separating velocity of opposite polarities reaches up to $4$km s$^{-1}$, which is significantly larger than the typical patch motion at $\thicksim 1$km s$^{-1}$ \citep{ots2007}.
There are many studies investigating the frequency distribution of the flux of emergence \citep{har1975, har1993,tit2000,hag2001,ots2011,tho2011}.
One of the most interesting questions is which scale is dominant in flux supply.
\cite{tho2011} obtained a steep power-law form with an index of $\thicksim -2.7$ by combining their results in quiet regions based on their feature-tracking and those from previous studies.
This power-law index, which is steeper than $-2$, suggests that smaller-scale flux emergence dominates the flux supply from below the photosphere.

A cancellation event is defined as a converging motion and subsequent disappearance of opposite polarities and is a relatively less distinct phenomenon in magnetogram images, with a typical velocity of less than $1$km s$^{-1}$ \citep{cha2002,par2009}.
It is considered a major process of flux removal process from the solar surface and is also related to various solar features, e.g., filament formation, flares, and EUV bright point \citep{mar1998,mart2001}.
Two scenarios describing this process, U-loop emergence and $\Omega$-loop submergence, are suggested \citep{zwa1985}.
Investigations of Doppler velocity, upflow or downflow, and the horizontal field direction, connecting positive to negative or negative to positive, are critical to discriminate between these scenarios.
Some recent papers report downflow structures and a normal connection in the horizontal field \citep{cha2004b,iid2010,cha2010} but are still inconclusive \citep{kub2010,wel2013}.
From the view of flux maintenance, the flux dependence of cancellation still remains uninvestigated despite its importance \citep{iid2012}.

Besides emergence and cancellation, apparent unipolar appearances and disappearances occur without any interactions with surrounding patches.
\cite{lam2008} first investigated such unipolar appearance events statistically with the magnetograms obtained by Michelson Doppler Imager on board {\it Solar and Heliospheric Observatory}.
\cite{lam2010} extended the research and also used magnetograms by Solar Optical Telescope on board the {\it Hinode} satellite.
They investigated an ensemble of averages of magnetic flux profiles around such unipolar appearance events and found a surrounding plateau that has the same polarity as the detected features.
This means that there are magnetic fields undetected by the auto-tracking technique, which supports the idea that these appearances are actually a coalescence of undetected patches.
Further, \cite{lam2013} investigated the birth and death of magnetic patches.
They determined that unipolar events are frequent dominant processes during the partial lifetime of patch structures, i.e., the expected lifetime of patches by a particular process, calculated from its occurrence frequency.
This dominance means that they are also dominant in apparent flux removal, which is consistent with our results in Paper I.

Accordingly, to understand flux maintenance on the solar surface, the second paper in the series investigates the patch interactions accompanying changes in flux in patches, namely the apparent unipolar process, cancellation, and emergence, with a focus on the flux dependence of their occurrence.
In Sections 2 and 3, observational data and definitions of flux change events, emergence, and cancellation in our analysis are described.
Results are shown in Section 4.
Finally, these results are discussed and one plausible picture of flux maintenance in quiet regions is presented in Section 5.

\section{OBSERVATION}
Two data sets of magnetograms taken by a Solar Optical Telescope (SOT) / Narrowband Filter Imager (NFI) onboard the {\it Hinode} satellite \citep{kos2007, ich2008, tsu2008, sue2008}, are used.
One is the data set also used in Paper I (hereafter Data1).
To increase number of detected cancellations and emergences there, another data set of magnetograms is used, with the longest duration hitherto obtained by the {\it Hinode} satellite (hereafter Data2).
For a detailed description of Data1, refer to Section 2 in Paper I.

The observational period of Data2 is from 10:24UT on December 30, 2008 to 5:37UT on January 5, 2009, a total duration of 115h 13min.
The {\it Hinode} satellite is usually pointed to the disk center for the synoptic observation.
During this period, all the synoptic observaton are cancelled and the data is uninterrupted for the long duration.
The SOT tracks a quiet region near the solar equator.
The center of the SOT view moves from $(-520.9'',-9.3'')$ to $(695.9'',-6.9'')$ in the solar coordinate.
SOT/NFI obtains circular polarization images, namely Stokes-V/I, at one wavelength shifted by +140m$\AA$ from the Na$_{\rm I}$ D$_1$ resonance line at 5896$\AA$.
The temporal cadence is $5$ min.
The original pixel scale of the CCD camera is $0.08''$ for this band.
The data are summed by 2 pixels in both the x- and y-directions onboard and are recorded with a spatial binsize of $0.16''$.
The total view is $704$ pixels $\times$ $704$ pixels, which is equivalent to $112.6'' \times 112.6''$.
Note that, because the center of the view is gradually shifted because of the long duration of the observation, we extract the field of view contained through throughout the entire observational period, which is explained in detail later.
The final analyzed view measures $94.9'' \times 91.4''$ after this extraction.
An example of a magnetogram from Data2 is shown in Figure 1.
We can observe some network cells in the field of view, as with Data1.
The total number of retrieved images is 1642 after removing the frame with missing data because of a readout error of CCD camera.
The cadence of analyzed data is $\thicksim$5 min though it occasionally 10 min due to this removal.
Table 1 shows a summary of the observational parameters in Data1 and Data2.

Before detection and tracking of patch structures, the cleaned-up magnetogram images must be prepared.
Such preparations are performed in the same manner as for Data1 in Paper I: dark current subtraction and flat fielding by the ${\rm fg\_prep}$ procedure in the SolarSoftWare package; removal of the columnwise offset of SOT/Filtergram (FG) data by subtracting the average in each column \citep{lam2010}; conversion of each pixel from a circular polarization signal to magnetic flux by fitting a scatter plot of the circular polarization signal, obtained by the SOT/FG, and magnetic flux, obtained by Solar and Heliospheric Observatory ({\it SOHO})/ Michelson Doppler Imager (MDI); spatial and temporal averaging to smooth the observed signal; and de-rotation to a certain time, for which we use 20:35UT on January 1 for Data2 when the observed region is near the disk center.

In addition to these processes, two more corrections are needed due to the long observational period of Data2.
First, the observed line-of-sight magnetic field is projected onto the field perpendicular to the solar surface, simply assuming that the magnetic field is always perpendicular to the solar surface.
The vertical magnetic flux density in each pixel is calculated as
\begin{equation}
B_{\rm ver} = \frac{B_{\rm LOS}}{\cos \theta}
\end{equation}
where $\theta$ is the heliocentric angle of each pixel.

Next, the gradual shift in the field of view that occurs due to the small difference between the tracking curve of the satellite and the rotation of the Sun is removed by making correlations between consecutive magnetograms
There is one other change of the observational field of view in the long period observation by {\it Hinode}/SOT.
The difference between the tracking curve and rotation accumulates, and when the position of the tip-tilt mirror hits the stroke limit, it returns to its original position.
Thus, there is one sudden change of field of view in Data2.
We limit our analysis only to the field of view contained throughout the entire observational period.
The final analyzed field of view measures $94.9'' \times 91.4''$, which is slightly smaller than the original field of view of $112.6'' \times 112.6''$.

Figure 2 shows the time series of the total flux contained in the analyzed field of view.
Though we cannot observe any active regions during this observational period, there are some periods during which both polarities simultaneously increase; these are periods of relatively large flux emergence.
Quantitatively, the total flux averaged over the observational period are $1.70 \times 10^{20}$ Mx, $1.54 \times 10^{20}$ Mx, and $3.24 \times 10^{20}$ Mx for positive, negative, and both polarities, respectively.
These correspond to $3.76$ Mx cm$^{-2}$, $3.42$ Mx cm$^{-2}$, and $7.16$ Mx cm$^{-2}$.
Because these averaged flux densities are not considerably larger than those in Data1, $2.53$ Mx cm$^{-2}$ and $3.60$ Mx cm$^{-2}$, this region is thought to be quiet region.
In case of flux balance, the difference in the flux of positive and negative polarities is, on average, less than 9$\%$.

\section{DETECTION OF UNIPOLAR FLUX CHANGE, CANCELLATION, AND EMERGENCE}
We use the same methods to track the patch structures and detect merging and splitting events as in Paper I.
Clumping method is used in the recognition of patches.
The signal and size threshold are set as two sigma of the histogram of magnetic flux density in each image and 81 pixels respectively.
We employ relatively large value for the size threshold with an aim to pick up only patches on the network boundary.
Checking spatial overlaps does the tracking between the consecutive images.
Merging and splitting are also determined by spatial overlaps.
Refer to Section 3 in Paper I for more detailed explanation of these methods.
Note that we need a margin of five extra pixels for tracking.
This is because the time interval of the consecutive magnetogram is 5 minutes and the expected travel distance is larger than the scale of 1 pixel in the {\it Hinode}/SOT magnetogram.
Our method of detecting unipolar flux change events, cancellation, and emergence are described below.

First, significant flux change events, excluding merging and splitting, are detected in each tracked patch.
A significant flux change event is defined as a flux increase or decrease that has a duration and flux change rate exceeding certain threshold values.
Because this step occurs after the detection of merging and splitting, i.e., we already know which patches experience merging and splitting, and when, flux changes caused by merging and splitting can be excluded.
We subtract the flux of other merged parent patches after the occurrence of merging and repeat the same step for splitting.
Based on this concept, a corrected time series of flux in a certain patch, $\phi_{\rm COR}$, is calculated as
\begin{equation}
\phi_{\rm COR}(t) = \phi(t)
- \sum_{j=1}^{N_{\rm mrg}} \sum_{k=1}^{N_{\rm mrg}^j} \phi_{\rm DAU, k}^j(t_{\rm mrg, j}) H(t-t_{\rm mrg, j})
+ \sum_{j=1}^{N_{\rm splt}} \sum_{k=1}^{N_{\rm splt}^j} \phi_{\rm PAR, k}^j(t_{\rm splt, j}) H(t-t_{\rm splt, j})
\end{equation}
where $\phi(t)$ is the time series of the flux of the considered patch; $\phi^i_{\rm DAU, j}$ and $\phi^i_{\rm PAR, j}$ are the time series of the flux of the $j$-th daughter patches for the $i$-th merging and the $j$-th parent patches for $i$-th splitting, respectively; $N_{\rm mrg}$ and $N_{\rm splt}$ are the number of merging and splitting events, respectively; $N_{\rm mrg}^i$ and $N_{\rm splt}^i$ are the number of daughter and parent patches, respectively, excluding the considered patch in the $i$-th merging and splitting; $t_{\rm mrg, i}$ and $t_{\rm splt, i}$ are the time intervals of the considered merging and splitting occurrences, respectively; and $H(t)$ is the Heaviside step function.
The second term in corresponds to the total flux of daughter patches in the merging events and the third term does that of parent patches in the splitting events.

To pick up flux change events, we set duration and flux change rate thresholds based on the typical values for cancellation and emergence events.
Cancellations in a network field have a time scale of a few tens of minutes \citep{cha2004b,iid2010}, whereas flux emergence has a shorter time scale of less than $10$ min \citep{ots2007}.
Because we set as short a threshold for temporal duration as possible to detect emergences, the threshold for temporal duration is set as 5 min in Data1 and 10 min in Data2.
Note that the time interval in Data2 is 5 min.
The threshold for the flux change rate is derived from the typical flux change rate for cancellation.
This is because cancellation is thought to be a more moderate event in terms of flux change rate than flux emergence.
There are some reports of flux change rates of cancellation events in network fields \citep{cha2002, park2009}.
\cite{cha2002} reported a cancellation flux change rate of $3.5 \times 10^{18}$ Mx hr$^{-1}$ from their analysis of magnetograms obtained by ${\it SOHO}$/MDI.
We use a slightly smaller value, $10^{18}$ Mx hr$^{-1}$, as the threshold for flux change rates to detect as many cancellations as possible.
Applying these thresholds and averaging flux over three data points in the temporal direction to obtain a smoothed data, we detect significant flux change events, excluding merging and splitting.

Figure 3 shows an example of the time evolution of flux in one tracked patch in Data1.
The dotted line represents the flux before the removal of flux changes from merging and splitting, $\phi(t)$.
The solid line represents the flux after the removal of flux changes, namely $\phi_{\rm COR}(t)$.
After the removal, three large flux change events, indicated by shaded area, can be seen in the solid line in Figure 3.
These flux changes are detected as significant flux change events.

Next, we make pairs of the flux change events among positive and negative polarities within the certain spatial and temporal overlaps.
We set the same spatial threshold for cancellation as that for tracking patches, 1 pixel in Data1 and 5 pixels in Data2, because the typical proper velocity of canceling patches is less than 1 km s$^{-1}$ \citep{cha2002, park2009}.
Remind that the temporal cadence of Data2 is 5 minutes and one fifth of that of Data1.
On the other hand, an emerging bipole is known to have a larger velocity than that of typical patch motion \citep{ots2007}.
We set the threshold for emergence at 4km s$^{-1}$, which corresponds to 4 pixels in Data1 and 20 pixels in Data2.
In the case of temporal overlapping, three data points in the temporal direction in both Data1 and Data2 are measured and averaged.
The pairing is done from the events with larger flux changes, which guarantees the uniqueness of the pairing.
After forming pairs between opposite polarities, unpaired flux change events are categorized as unipolar flux change events.

Our method can detect partial cancellations, i.e., those in which one or both the involved patches do not disappear.
It can also detect partial emergences by the same logic.
However, this method categorizes a hybrid event of flux increase and decrease, i.e., the simultaneous occurrence of cancellation and emergence,
as a single cancellation, a single emergence, or a mix of uni-polar processes.
Thus, the detected numbers for emergence and cancellation events may underestimate the actual numbers.
Another item to note is why a pair of flux increases in patch structures are defined as a flux emergence.
It may seem that a pair of flux appearances should be defined as an emerging flux; however, as will be pointed out in Figure 4, because emerging bipoles coalesce with pre-existing patch structures soon after their appearance, tracking an emerging bipole from its birth is difficult.
A final note addresses our definition of the change in flux during emergence and cancellation events.
Larger change in flux of positive or negative polarities in each event is employed because the first part of appearance and last part of disappearance cannot be followed because of size thresholds of detection.
This is also shown in Figure 4.

Based on the method described above, flux change events in each patch are detected and categorized into unipolar flux change, cancellation, and emergence events.
Unipolar flux change events will be shown and investigated in Section 4.2.
The present section concentrates on cancellation and emergence in this section.

Figure 4 shows examples of paired flux change events, namely emergence and cancellation.
The upper panels in Figure 4 show time evolutions of magnetograms in an emergence event.
There is a pre-existing positive patch in the north of the emerging region in the first panel.
The emerged negative polarity is small and unrecognizable under our detection conditions around its birth at 1:09UT.
It continues to grow larger, and when it becomes large enough at 1:13 UT, the appearance of the patch structure is detectable with our threshold.
On the other hand, an isolated patch structure of positive polarity cannot be detected because it merged with the large positive patch.
However, we can observe a continuous increase in the flux of the positive polarity from 1:11 to 1:18 UT.
After the appearance of both polarities, the distance between them continues to grow from 1:19 to 1:23 UT.
It can be observed that the quiet region is filled with a magnetic field, making it very difficult to detect isolated patch structures from their birth.
Many coalesce with pre-existing patches very soon after their birth.

The lower panels in Figure 4 show a typical example of a cancellation event.
One negative patch shown by the yellow arrow, is converging with a larger positive patch in the north.
They contact at 0:49 UT and begin to cancel each other.
The negative patch continues to shrink, and it becomes smaller than our size threshold at 1:05 UT.
Subsequently, it cannot be tracked with our threshold and totally disappears below the detection limit at 1:17 UT.
On the other hand, the positive patch remains even after the cancellation because the flux of the positive patch is larger than that of the negative patch, which results in a partial cancellation.

These events show that tracking patches from their exact time of birth to their exact time of death within certain size threshold limits is impossible.
This suggests that estimated values of the change in flux during these events are smaller than the actual values.

\section{RESULTS}

\subsection{Frequencies of each event and frequency distribution of flux in Data2}
Table 2 summarizes the incidence of detection for both Data1 and Data2.
The number of detected processes in Data2 increases from Data1 by approximately one order of magnitude because of the long duration.
The number of detected cancellations becomes particularly large, sufficient for a statistical analysis of Data2, as we expected.
On the other hand, the number of detected emergence events is still small and not sufficient for an investigation of scale dependence.
The occurrence of splitting and merging is roughly $7 \-- 8$ times that of cancellation, which is consistent with Paper I.
There are many unipolar events.
Furthermore, the incidence of all four unipolar processes has the same order of magnitude for each data set.
Despite the fact that the requirement for the detection of an emergence event is simply an occurrence of flux increase of opposite polarities within a certain distance, the number of emergence events is still considerably lesser than other processes.
This definition is less strict than those used in  previous papers on emergences \citep{hag2001,tho2011}, but we employ a larger size threshold to detect network structures.

Figure 5 is the frequency distribution of the flux in Data2.
We fit the range increasing monotonically from $10^{17.7}$ Mx indicated by the green dashed line in the figure.
A slightly smaller value, $10^{17.5}$ Mx, was obtained in Data1.
By fitting the data with a power-law function of the form $n(\phi)=n_0 \, (\phi/\phi_0)^{-\gamma}$ in the range from $10^{17.7}$ Mx to $10^{19}$ Mx, we obtain $n_0 = 1.63 \times 10^{-36}$ Mx$^{-1}$ cm$^{-2}$ and $\gamma = 1.93 \pm 0.03$ with $\phi_0 = 10^{18}$ Mx.
The errors show a 1$\sigma$-error in the fitting.
Alterations in the power-law index arising from different fitting ranges are also checked.
By considering these errors, the power-law index is $\gamma=1.93\pm0.07$, which is consistent with the previous studies \citep{par2009, iid2012, zho2013}.

\subsection{Unipolar Flux Changes}

As described in the previous section, many flux change events were detected in apparently isolated patches.
We call these flux change events unipolar processes in this study and categorize them into increase, appearance, decrease, and disappearance.
A unipolar increase is a significant increase in flux without recognizable paired flux increase events of opposite polarity.
A unipolar appearance is a significant increase in flux by a newly appeared patch but without a paiered flux increase of opposite polarity patch.
The other unipolar events are defined in a similar manner.

Figure 6 shows typical examples of unipolar flux change events in Data1.
We use Data1 here because of its better temporal cadence of the magnetogram than Data2.
Figure 6(a) is a unipolar increase event.
There is a negative patch at 1:46 UT, indicated by the blue contour around the center of the field of view (patch A).
In addition, there are two small patches without contours located to the east of patch A (patches B and C shown by the yellow arrow), which are below our detection threshold.
Patch A absorbed B and C to become larger at 2:01 UT.
Because patches B and C are below our detection limit, this event is recognized simply as an increase of flux in patch A, i.e., a unipolar increase event.

Figure 6(b) shows a unipolar appearance event.
In this case, at 2:29-2:31 UT, there are three small patches below the detection limit, which are shown by the yellow arrow.
They converge and coalesce to one large patch structure at 2:33 UT and retain the shape of the individual patches until 2:47 UT.
This event is explained in a similar manner in \cite{lam2010}, as a coalescence among undetected patches.

Figure 6(c) shows a unipolar flux decrease event.
One detected positive patch shown by the yellow arrow, is located near the center of view at 1:41 UT.
A hump appears in the eastern part of the patch at 1:42 UT and separates later at 1:46 UT.
The patch structure gradually grows until 1:45 UT and is finally separates at 1:46 UT.
The separated patch is below our detection limit.

Figure 6(d) shows a unipolar disappearance event.
One detected negative patch is indicated by the yellow arrow at 2:19 UT.
A dipped shape suddenly forms in the outline of the patch at 2:27 UT.
At 2:29 UT, the patch is divided into two small negative patches below our detection limit, and they separate from each other.

All the unipolar processes depicted in Figure 6 are explained as interactions with and among patches below the detection limit, which supports the conclusion reached by \cite{lam2010} that unipolar appearance is actually the coalescence of undetected patches.

Based on the interpretation that these apparent unipolar processes are interactions among patches below the detection limit, the change in the flux during these processes should be close to the detection limit because of the higher frequency of interactions between two patches than that among more than two patches.
Figure 7 shows histograms of changes in the flux during unipolar processes.
All four histograms concentrate around the detection limit, $10^{17.5}$ Mx, which is shown by the green dotted line in the figure.
This result supports the above interpretation.

\subsection{Frequency Dependence of Change in Flux During Cancellation}
We investigate the frequency distribution of changes in the flux during the cancellations by using Data2.
The distribution is derived from the observational results in the same manner as that of merging and splitting in Paper I, namely
\begin{equation}
\frac{\partial n_{\rm cnc}(\phi)}{\partial t} = \frac{N_{\rm cnc}^{\rm tot}(\phi)}{t^{\rm tot} \, S \, \Delta \phi},
\end{equation}
where $N_{\rm cnc}^{\rm tot}$ is the total number of cancellation events for patches with the flux  from $\phi$ to $\phi+\Delta \phi$, $t^{\rm tot}$ is the duration of the data, and $S$ is the area of the total field of view.
Figure 8 shows the resultant plot.
We can observe power-law-like dependence above the detection limit, $10^{17.7}$ Mx.
To quantify the dependence, a least-squares fitting is applied as the power-law distribution.
The fitting form employed is
\begin{equation}
\frac{\partial n_{\rm cnc}}{\partial t}= \left( \frac{\partial n}{\partial t} \right)_{0,{\rm cnc}} \left( \frac{\phi}{\phi_0} \right)^{-\gamma_{\rm cnc}},
\end{equation}
where $\left( \partial n/ \partial t \right) _{0,{\rm cnc}}$ is the reference frequency of cancellation, $\phi_0$ is the reference flux, and $\gamma_{\rm cnc}$ is the power-law index of cancellation occurrence.
We obtained $\left( \partial n / \partial t \right) _{0,{\rm cnc}}=(1.29\pm0.12) \times 10^{-41}$ Mx$^{-1}$ cm$^{-2}$ s$^{-1}$ and $\gamma_{\rm cnc}=2.48\pm0.26$ with $\phi_0 = 10^{18}$ Mx and a fitting range of $10^{17.7}$ Mx$\-- 10^{18.4}$ Mx.
The errors indicate 1$\sigma$-errors of least-squares fitting.
We also check the obtained power-law index with different bin sizes from 0.1 to 0.24.
Figure 9 shows the result of this investigation.
The range of the power-law index from $2.3$ to $2.6$ stays within the 1$\sigma$-error range in all cases; thus, we conclude that the proper power-law index obtained here is from $2.3$ to $2.6$.

Further, we apply the Kolmogorov-Smirnoff goodness-to-fit test on power-law fit of the cancellation frequency distribution.
The Kolmogorov-Smirnoff statistic, $D$, is introduced as a maximum difference of the cumulative distributions of the reference, power-law here, and the actual data.
The critical value $D_{\rm crit}$, with which we compare $D$, is calculated from number of data point and confidence level we set.
See \cite{par2009} for more detailed explanation of the Kolmogrov-Smirnoff test.
With number of analyzed cancellations in Data2, $362$ events, and the most permissive value of the confidence level of 99$\%$, we obtain the $D_{\rm crit}=0.0857$ from the Kolmogorov-Smirnov Table.
On the other hand, $D=0.186$ is obtained from our result.
This result, $D > D_{\rm crit}$, implies that the power-law fit is not good with the confidence level of 99$\%$.

\section{DISCUSSION}

\subsection{What are Unipolar Processes?}
\cite{lam2010} first investigated the unipolar appearances and found a same polarity plateau with the same polarity as the detected features, which supports the concept that these events are actually coalescences of undetected patches.
This paper has also offered four results supporting that all detected apparent unipolar processes, disappearances as well as appearances, are interactions with and among patches below the detection limit (Figure 7).
We want to emphasize that our result shows this result in the different way from that of \cite{lam2010}.
They compared the simultaneous magnetograms with different resolutions, {\it SOHO}/MDI and {\it Hinode}/SOT.
Only the magnetogram by {\it Hindoe}/SOT is used in this paper but we can compare detected-scale and undetected-scale by the large size threshold for the patch detection.

Several statistical findings are also important.
First, the frequency of incidence of such unipolar processes is much considerably higher than that of cancellation and emergence events and is of the same order as the frequencies of merging and splitting.
Second, all the four types of unipolar processes have occurrence frequencies of the same order.
As shown in Figure 10, there are actual physical possibilities that these unipolar processes occur through merging and splitting, but not through cancellation.
From the finding that merging and splitting are dominant processes on the solar surface, which is investigated in Paper I, these four processes occur in frequencies of the same order.
Third, the frequency distributions of changes in flux during the apparent unipolar processes is concentrated around the detection limit.
This result also supports the aforementioned interpretation because the interactions in Figure 10 result in apparent unipolar flux change events that change the flux by an amount that is at most twice the detection limit.
All these characteristics support the interpretation that apparent unipolar processes are in fact interactions involving small patches.

\subsection{Comparison with the Cancellation Model Suggested in Paper I}

The frequency distribution of canceling flux is evaluated by Eq.(18) of Paper I as
\begin{equation}
\frac{\partial n^{\rm APP}_{\rm cnc}}{\partial t}=\frac{v_0 n_0^2 \phi_0}{2(\gamma -1)\sqrt{\rho}}\left(\frac{\phi}{\phi_0}\right)^{-2\gamma+1},
\end{equation}
where $v_0$ is the typical velocity of patches, $n_0$ is the reference frequency of the flux of patches, $\gamma$ is the power-law index of flux distribution of patches, and $\rho$ is the number density of network cells.
Comparing this and Eq.(4), we obtain two relationships:
\begin{equation}
\gamma_{\rm cnc}=2\gamma-1
\end{equation}
for the dependence on flux, and that
\begin{equation}
\left( \frac{\partial n}{\partial t} \right)_{0,{\rm cnc}}=\frac{v_0 n_0^2 \phi_0}{2(\gamma -1)\sqrt{\rho}}
\end{equation}
for the magnitude.

In Data2, comparing the observational results and this model is possible.
From the model presented here, $\gamma=1.93\pm0.07$ was calculated and $\gamma_{\rm cnc}$ was evaluated as $2.86\pm0.14$ by Eq.(6). Observational measurement yielded a similar value of $\gamma_{\rm cnc}$ as $2.48\pm0.38$. This consistency in dependence index supports our model.
In Eq.(7), we adopt $v_0=0.5 \, {\rm km \, s}^{-1}$ and $\rho=1.0 \times 10^{-19} \, {\rm cm}^{-2}$ as typical values \citep{hag1997}, yielding an amplitude of $3.6 \times 10^{-41} {\rm Mx^{-1} cm^{-2} s^{-1}}$, which is larger than our observation, $\partial n_{0,{\rm cnc}} / \partial t=(1.29\pm0.12) \times 10^{-41}$ Mx$^{-1}$ cm$^{-2}$ s$^{-1}$.
This difference is possibly because the transport of patches cannot be treated as a ballistic motion with a constant velocity. Future work will improve upon this model.

Furthermore, Paper I discussed the possibility of the recycling of flux through submergence by cancellation and re-emergence in small scales.
\cite{tho2011} reported the frequency distribution of emerging flux as $3.14 \, \times \, 10^{-14} \times \left( \phi  \, [{\rm Mx}] / 10^{16} \right)^{-2.69} \, {\rm Mx^{-1} \, cm^{-2} \, day^{-1}} = 1.52 \times 10^{-40} \times \left( \phi \, [{\rm Mx}] / 10^{18} \right)^{-2.69} \, {\rm Mx^{-1} \, cm^{-2} \, s^{-1}} $.
The power-law index is consistent with the recycling model; however, the magnitude of occurrence is different by one order of magnitude.

This contradiction is significant and flux recycling probably does not happen in the flux scale investigate in this paper.
However, there are several possibilities of flux recycling.
One possibility is that the submerged flux is fragmented after the submergence and hence the frequency distribution of re-emerged flux is different from that of cancellation.
The second possibility is that flux recycling does not happen in the network field but does in the other convective structure.
Note that our analysis is mainly limited to the network field due to the relatively large size threshold, 81 pixels.
There is a strong downflow on the network boundary.
It is possible that such downflow forces the canceled magnetic field to penetrate deeper, which results in total submergence into the convective zone.
Future investigation at smaller scales is important.
The last possibility is that our detection method is not as good for emergence as for cancellation.
As we mentioned, the detection of emergence is more difficult than that of cancellation due to the shorter time scale and higher velocity of emerging patches.
Actually there are several undetected emergences in Figure 7, which are pointed out.
It will be helpful to compare the results from different detection methods.

\subsection{Flux Maintenance in Quiet Regions}

Based on the analysis performed in Paper I and this paper, we suggest a scenario of flux maintenance in quiet regions.
Figure 11 shows a schematic describing this proposed scenario.

First, after the flux is supplied from below the photosphere and active regions, magnetic patches are advected, predominantly by convection on the solar surface.
During advection, a power-law frequency distribution of the flux is formed and maintained at an index of $\thicksim 1.8$ by merging and splitting on the solar surface.
This occurs when the time scales of merging and splitting are considerably shorter than those of emergence and cancellation, which is shown in Paper I, and means that the flux distribution is formed as a power-law distribution before the encounter of opposite polarities.

Quantitative investigations of this scenario are still an open question for future works. The work of \cite{mey2011} is notable. They conducted a mathematical simulation of a magnetic carpet with the observed flux distribution of emergence and frequent splitting. As a result, they obtained a flux distribution of patches similar to observational results, e.g., a power-law distribution with an index of $1.8\--1.9$.

During and after the maintenance by merging and splitting, patches are advected by convective motion. If one assumes that cancellation is caused only by advection and is nearly independent of patches' flux, it results in a steep dependence of cancellation occurrence rate on flux, i.e., a power-law index of $\thicksim 2.6$.
This is shown in the discussion of Paper I, and the present paper confirms this speculated steep power-law index observationally, though we caution that the power-law fit to the observations is not a statistically good fit.
Note that the magnitude is not precisely consistent with this model, and it needs improvement.

Then, through the cancellation, the flux submerges below the photosphere and later rises to the solar surface again.
This re-appearance may result in a steep power-law distribution of emergence on flux because the distribution of cancellation, i.e., submergence of flux, also has a steep power-law distribution.
Although the steep power-law distribution of cancellation is found, there is a contradiction in the magnitude between the frequency distribution of cancellation in this study and that of emergence in \cite{tho2011}.
There are several possibilities explaining this result, the fragmentation to smaller scale in the convection zone, the convective flow effect, or such recycling does not occur on the actual solar surface.
Further investigation is needed to understand the flux maintenance in quiet region.

\section{SUMMARY OF RESULTS}
Extending the investigation of surface magnetic processes based on the auto-tracking technique employed in Paper I, this paper has investigated apparent unipolar processes, cancellations, and emergences.
It was found that all four apparent unipolar events are considerably more frequent than cancellation and emergence events, which is consistent with \cite{lam2010} and \cite{lam2013}, and that all four types occur in frequencies of the same order of magnitude, which supports that these processes are related to the same actual processes, i.e., merging and splitting.
This paper further investigated the frequency distribution of flux changes during apparent unipolar processes.
It was found that all distributions were concentrated around the detection limit set for the experiment, which also supports the interpretation that these processes are in fact merging and splitting with and among undetected patches.
This interpretation also implies s physical picture of many interactions within the flux range in this analysis and below the detection limit.

As for cancellation and emergence events, the occurrence frequency distribution of decrease in flux during cancellations was investigated, but not for emergences owing to the lack of event numbers.
As expected from the discussion in Paper I, a steep power-law frequency dependence, $2.48 \pm 0.26$ as a power-law index, was found for cancellation.

From these results, we proposed one plausible picture of local flux maintenance in quiet regions, shown in Figure 11.
The important assumption of this model is that merging and splitting, not cancellation and emergence, are dominant process that is confirmed by this paper and previous studies \citep{lam2010, iid2012, lam2013}. Notably, cancellation occurs by the advection in a random direction and includes local recycling rather than actual flux supply.
However, the quantification of this plausible modeling is an open question for future works.
For a deeper understanding of flux maintenance on the solar surface, a mathematical simulation of the proposed model will allow insight into whether our picture can exist in the quantitative sense.
From the viewpoint of dynamics, we believe that analyses of spectropolarimetric observation and RMHD numerical simulation are plausible candidates to understand what dynamic process causes this picture, e.g., frequent splitting of patches on the solar surface.

\section*{Acknowledgement}
First of all, we appreciate the referee for a lot of helpful comments and advices.
The paper is much improved with the advices.
Hinode is a Japanese mission developed and launched by ISAS/JAXA, in collaboration with the domestic partner NAOJ and international partners NASA and STFC (UK). Scientific operation of the Hinode mission is conducted by the Hinode science team at ISAS/JAXA. This team mainly consists of scientists from institutes of partner countries. Support for the post-launch operation is provided by JAXA and NAOJ, STFC, NASA, ESA, and NSC (Norway). Also the authors would like to thank Enago (www.enago.jp) for the English language review.

\bibliographystyle{apj}

redpajama_set_name: RedPajamaArXiv


text:
Q: How do you prevent Textbox from erasing current value entered by user on error? $sql = "select * from tbl_pi where patientNumber='" . $pn . "'";
$res = mysql_query($sql);
if (mysql_num_rows($res) == 1) {
    echo '

PATIENT NUMBER ALREADY IN USE!!
';
}

after the error detection, the user have no choice but to start over since the previous data entered were all gone or reset.
How can I prevent that from happening?

redpajama_set_name: RedPajamaStackExchange


The best ways to promote your extension. That's what I call interesting article.
Awesome, you just created your very own extension! Congrats!
Be social, spread the message on Facebook, Twitter, Google+, Tumblr, your personal blog etc.
See ChimneySwift11 promoting his extension in this awesome video!
Hope you and especially your fans enjoy your new extension!


The Cycle-to-work scheme offers a tax-free benefit to employees in the form of cycles loaned to them by employers in exchange for a salary sacrifice (s244 of the Income Tax (Earnings & Pensions) Act 2003). However, with new HMRC guidelines in the Autumn of 2010 on valuations on cycles at the end of the salary sacrifice period, complexities arose that temporarily halted schemes and our customer needed advice and a structure that would assist in dealing with the additional employee cost.
Our customer, a global car manufacturer, had concerns as to how to handle the new "end of life" regulations for cycles. The funding by AFM enabled a cash-neutral situation with AFM paying suppliers for certificates and recovering costs in line with salary sacrifice dates and and amounts, however, the new rules threatened some of the benefits.


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Apple has a tendency to create iconic products that transform the way we do things. The iPhone took the smartphone market to the next level, the iPod revolutionized the way people listened to music, and the iPad's versatility made it an adequate replacement for computers in some situations. While other companies have attempted to follow Apple's footsteps, they haven't yet managed to reach the heights Apple has. The iPad Pro might not be as successful as the iPhone but is a hit product in its own right. iPads are well-loved among professional designers, artists, graphic designers, and individuals from similar fields.
Introduction to iPad Pro
The first iPad Pro was launched back in 2015 and it was well-received by almost everyone. The larger screen, better processor, larger battery life and memory, etc., make it an appealing device for professionals. iPad was ideal for people who wanted an on-the-go device to supplement their computing needs. Experts noted that while iPads performed some tasks as well as a computer, it wasn't a full replacement so people would still need a computer for more intensive tasks.
Every generation of iPad that followed the first release is reaching for that goal of being a laptop replacement. The first generation of this device was released in 2015 and the second was released in 2017. Since the last release, people have been waiting impatiently for the latest iteration of the iPad Pro. While Apple didn't release the Pro tablet with its new iPhones, most speculate it will drop by the end of October.
Features and Benefits of iPad Pro
The iPad Pro is designed for professionals and has professional-grade features. Apple has a good track record of keeping bloatware low and making sure only the best and most useful features find their way into the new devices. Here's a look at some of the key features of the previous generation iPad Pro and the speculation around upgrades in the upcoming version:
Display – The previous generation iPad Pro had a 10.5-inch display, which was bigger than the first gen model. Apple increased the screen size without increasing the weight and dimensions of the new model. They will follow the same pattern with the new iPad Pro models. The 2018 devices will have an edge-to-edge display like the one found in iPhone X and its successors. Smaller bezels mean Apple can fit in a bigger screen without increasing overall device size. In fact, many experts speculate that the company will reduce the overall size of iPad Pro 2018.
Design – The previous iPad has a very clean design with a home button at the bottom, narrow bezels on all sides, and a camera on top. The newer iPad design is likely to be inspired by iPhone X design. Experts speculate the new iPad Pros won't have a home button and it won't include the dreaded camera notch, which was so prevalent in most 2018 phones.
Pro Motion Display – The ProMotion display was big news in 2017. No other tablet had a display with a 120Hz refresh rate. This display is crisp and very smooth. There's no lag when you play games, watch videos, or just browse through the internet. The previous iPads had a regular LCD display that only operated in 60Hz. It is possible that Apple will retain this feature or improve it with the new iPad Pro.
Performance – The second generation iPad Pro had higher CPU speed, graphics speed, and better battery life. Everything was 30% to 40% faster. Users can expect a similar boost in performance with the new iPad Pros. It is likely that Apple will use its latest chip in the iPad.
There are many other features of note in the previous and current generation of Ipads. You can expect all the features to improve. The new iPad Pro might also include FaceID and remove the headphone jack.
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Customer Response
Customer response to iPad Pro has always been either mixed or good. These iPads suit specific types of users best, which is why many Apple fans choose regular iPads instead of iPad Pros. Apple's iOS 12 has already garnered much praise in the tech community. Some tech reviewers have even called this Apple's best-operating systems yet. It is possible that the new iPad Pros will ship with this OS.
Advantages and Disadvantages
The most common complaint the price because iPad Pros are expensive. Aside from this factor, the customer reviews are good. Most Apple users love the improvements on the previous generation and they will be eager to see an iPad Pro with the latest Apple design. People who are moving some Android tabs will find the iPad Pro ecosystem a little too restrictive. However, you get excellent software efficiency with great hardware.
1. Will the pen stylus come with the iPad?
You will have to get the Apple Pencil separately as it doesn't come in a pack. It works well with the latest screen developments and advances.
2. Will it have a camera?
The iPhone will most likely have two cameras; one primary camera and one for HD Facetime.
iPad devices rarely disappoint and work efficiently for several years. That makes iPad Pro a worthwhile purchase. The 2018 version will be even better.
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Criticizing President Barack Obama's health care reform law on Wednesday, Rep. Mike Kelly (R-Pa.) likened the requirement that private insurance plans provide contraception coverage to two of the most devastating attacks on American soil.
"I know in your mind, you can think of the times America was attacked," he said at a press conference on Capitol Hill. "One is Dec. 7, that's Pearl Harbor Day. The other is Sept. 11, and that's the day the terrorists attacked. I want you to remember Aug. 1, 2012, the attack on our religious freedom. That is a day that will live in infamy, along with those other dates."
Wednesday marked the first day private insurers must include birth control coverage in their plans without charging a co-pay, per requirements in the Affordable Care Act. The change will affect most women on private health plans, with some exceptions. More than a dozen Republican members of the House of Representatives, mostly freshmen, held a press conference to blast the law for what they said were violations of religious freedom.
"As this mandate goes into effect, Americans are going to be forced to act against the principles of their faith," said Rep. Ben Quayle (R-Ariz.). "This coercion by taxation that this president seems to like must stop and it must come to end now."
The conservative lawmakers' objections focus on the fact that employees and students with religiously affiliated groups will be able to have access to contraception coverage through their health care plans. A compromise offered by the Obama administration requires insurance companies to offer the coverage directly, so that the employers are removed from the transaction.
Still, the members threw one vitriolic jab after another at the mandate, calling it an attack on freedom and an assault on first amendment rights. Rep. Tim Huelskamp (R-Kansas), a Roman Catholic, characterized the law as "thinly veiled religious bigotry."
"Today is the day religious freedom died in America," Kelly added. His colleague Rep. Billy Long (R-Mo.) expressed a similar sentiment, saying, "We're not the land of the free anymore, and we need to get that straight."
Rep. Ann Marie Buerkle (R-N.Y.) called the mandate "the largest assault we've seen on first amendment rights in the history of our country," and her colleague Rep. Jeff Fortenberry (R-Neb.) called it "unprecedented government coercion in health care."
"This is not an issue of birth control, it's an issue of government control," Rep. Steve Pearce (R-N.M.) said.
"It's outrageous that this administration believes it's within their power to force people to violate their right of religion if it interferes with this administration's agenda," Rep. Alan Nunnelee (R-Miss.) said. "It should disturb people of all faiths, or for that matter people of no faith at all, that President Obama has such a low opinion of the first amendment that he would trample on these rights."
In addition to the contraception mandate, health insurance plans must now cover additional screenings and services for women without passing on any of the cost to the patient.
"These include services that are essential to helping women stay healthy -- such as domestic violence screening, FDA-approved contraception, breastfeeding support and supplies, gestational diabetes screening, HPV testing, sexually transmitted infection counseling, and HIV screening," Health and Human Services Secretary Kathleen Sebelius and House Minority Leader Nancy Pelosi (D-Calif.) wrote in a USA Today op-ed published Tuesday.
"That's on top of other potentially life-saving services such as cholesterol screenings and flu shots that many private plans and Medicare have already begun covering with no co-pay thanks to the law."
UPDATE: 3:00 p.m. -- Democrats hammered Kelly for his remarks.
"Equating women's health care and contraception with two of the darkest days in American history is not just wrong -- it's shameful," said Rep. Carolyn Maloney, (D-N.Y.), who has spent the last decade dealing with the aftermath of 9/11. "Hopefully Rep. Kelly will realize his rhetoric doesn't match the situation. Safe, accessible contraception is a fundamental part of virtually every woman's health care at some point in their lives."
Rep. Jerry Nadler (D-N.Y.), whose district incudes Ground Zero, said Kelly should apologize.
And Sen. Daniel Inouye (D-Hawaii) responded in a similar manner.
"I witnessed the attack on Pearl Harbor and had the privilege of serving in the United States Army during World War II and I find the comments made by the Congressman from Pennsylvania to be misguided and insulting," he said. "It is complete nonsense to suggest that a matter discussed, debated, and approved by the Congress and the President is akin to a surprise attack that killed nearly 2,500 people and launched our nation into the second World War or a terrorist attack that left nearly 3,000 dead and led to fighting and dying in Afghanistan and Iraq. Having fought for this nation in Europe, I find that I have a special kinship with those who served in Afghanistan and Iraq and I routinely visit with the most severely wounded veterans of those conflicts. Just yesterday I met with a brave young man who lost all four of his limbs in Afghanistan. I hope the Congressman from Pennsylvania has the courage to share his comparison with them."
Amanda Terkel and Mike McAuliff contributed reporting.


Big or small our villages are nestled among forests with springs, or simply line the shores of the Myrtoan Sea, making their guests feel the that all amazing beauty and serenity generously offered by nature.
The last village of Arcadia nestled in Mount Parnon, 1,150m above sea. It features stone-built houses surrounded by walnut and chestnut trees. The main square is the beating heart of the village. Here, you' ll find the stone-built church of Agioi Anargiroi, the huge shady trees, as well as cafe serving syrupy sweets. There are also tavernas with local cuisine and traditional shops selling honey, herbs and handmade ceramics.
Seaside village with stone-built mansions, flower gardens and beautiful beaches full of fishing boats and tavernas.
The scenic lush villages of Mount Parnon create a beautiful natural environment filled with springs running from fountains, stone-built houses and cobbled streets. There is also a forest with plane trees and cedars. Just before Agios Vasileios, visitors will meet the monastery of the Archangels of Moorea with their beautiful frescoes, whereas in Palaiochori you can visit the Mycenaean tombs and caves featuring beautiful formations of stalactites and stalagmites.
Charming villages with two-storey mansions and stone arches, beautiful squares and traditional tavernas where many festivals take place during summer. Peleta is famous for its aromatic red wine and a cave 490m deep. After passing by Pigadi, visitors will find the pebbled beach of Fokianos. The area is a wetland and in the migratory months you may also see flocks of rare birds.
Sampatiki is a picturesque fishing village with a beautiful harbor, Pera Melana is a typical Tsakonian village hosting a Folk Museum with exhibits from the cultural tradition of the area and Pragmatefti offers views to amaze every visitor.


As marketers, making people aware of our brand is a central tenet of our job description. But what that means today is radically different than what it meant even ten years ago.
In the most cutting edge companies marketers are no longer just the voice of the brand, but its face and ears as well. In this way, our role now is less about broadcasting messages and more about increasing awareness through constant Customer Relationship Management (CRM).
Here I'll break down just what CRM means today, why and how it continues to be essential for all businesses, and where it fits within the broader scope of your new sales funnel.
Social proof has always been essential to marketing. Consumers are much more likely to buy a product if they see it validated either by their social equals (e.g. friends, family, community members, etc.) or their social superiors (e.g. celebrities).
In the traditional sales funnel a marketer's main job existed in those early stages, where we tried to snag customers with promises of savings and other incentives before our competition could do the same. This is also when we tried to use social proof to convince customers of their need. If we were successful, we'd then usher customers down the line to the sales department and customer service.
Now, however, the "funnel" isn't nearly so linear. The deeper your business gets into content production and social media (and you should get deep into both), the more quickly and completely you'll be expected to respond to customer inquiries, comments and requests. The goal is no longer to simply advertise your brand or product, but to establish credibility and a unique, helpful, expert presence.
What's more, today's CRM is about creating social communities, one where users can find helpful information either directly from your brand or from fellow customers. It is the marketer's job to spark and guide those conversations, as well as to respond at the right moments in a well-honed, distinctive company voice. The more responsive and helpful you are, the better your company will stick out in a consumer's mind as a trusted industry leader — one from whom they should buy either now or somewhere down the line.
Developing your own CRM is a matter both of social and content strategy, as well as of embracing new technical tools.
Separate yourself from the pack by developing a unique online presence. For a good model, take a look at the Zappos Twitter feed, managed by the company CEO, Tony Hsieh. These Tweets are helpful, informative, relatable and distinctive, lending both the company and Hsieh an understanding, human face. You just can't establish that kind of humanity if you're only announcing your great deals.
Develop original content. This is the fastest way to establish your company as a cutting edge, industry leader, to establish your voice, and to show your customers how responsive you can be to their thoughts and comments. And, as more people are sharing quality content than ever before, it's a great, inexpensive way to get your brand discovered through social networks.
Buy or create a CRM management platform to manage and measure your extensive social and content campaigns. The more of a presence you establish, the more you'll have to monitor and measure to stay on top of requests for responses and for measuring the effectiveness of your efforts. That's why it's so important to have a centralized platform to help you manage all of your efforts.
Salesforce, for instance, provides a number of metrics right on its dashboard, as well as the ability to track customer interaction and click through rates across multiple channels. However, for companies with very diverse and unique CRM needs, it may be worth using an agile application development provider to create your own, rather than trying to adjust your needs to a standard system.
While going at it yourself will be a larger investment in the short term, you'll get a high ROI if the system can help you not just manage and track your campaigns, but if it also can give you the tools you need to create even more unique content, based on the data you've collected.
There has never been a time when CRM has been more crucial than in our hyper-social age. Do CRM correctly, and the world is yours for the taking.
Adria Saracino is a marketer and blogger. When not consulting on outreach and content strategy, you can find her writing about style on her personal fashion blog, The Emerald Closet.


Mac and Bumble brings you the hottest women in the world and Kristin Jackson is a prime example. We travel far and wide looking for the most attractive girls and when we met Kristin Jackson, we knew we had found something great. This pretty young beauty is sure to be a wide-spread sensation – and we're sure you will agree. One look at this fresh-faced lovely with her shapely curves and impressive style and we know that Kristin Jackson is going to go far.


Anguilla is the most envied island in the Caribbean for the caliber and quantity of it beaches. The most pristine of all, Shoal bay, is rated one of the world's best with its truly spectacular miles of long curving ribbon of white powdery sand held in the protective arms of crystal clear water. Snorkeling is realized in an abundance of sea life that thrives on the coral reef at beach's edge. Take a 20 minute speed boat leap to Anguilla where a mini island tour awaits you to discover its unique treasures.
See St. Maarten from the deck of a luxury catamaran-it's a party with beach, swim, and snorkel! The friendly crew has lots of activities planned for you!
As you sail along the palm-lined seashore framed by emerald hills, you'll see some of St. Maarten's famous sights-Fort Amsterdam, Little Bay, Cay Bay, and Pelican Key.
St Barth was once a popular pirate haunt, but today it is frequented by celebrities. They know the island's unique treasures are well worth discovering and we have the map to all of their secret locations not found in any tourist books! So grab your sense of adventure and hop on our State-of-the-Art powerboat for a quick 45 minute cruise and discover this gem on your own in a fun, interactive ATV Craze. You will follow our game plan map navigating through the four corners of this magical island.
You'll be hungry after all your adventuring, but this tour has that covered! Cheeseburger in paradise is among the menu items served in a bistro of Gustavia, the capital, where you will grab a bite. You will have plenty of time to visit the shops, take a seabath, or snorkel on a pristine beach.
This is the same as our daytrip to St. Barth with ATV, only with your own private Jeep instead!
St Barth was once a popular pirate haunt but today it is frequented by celebrities. They know the island's unique treasures are well worth discovering, and we have the map to all of their secret locations not found in any tourist books! So grab your sense of adventure and hop on our State-of-the-Art powerboat for a quick 45 minute cruise and discover this gem on your own in a fun, interactive Jeep Scavenger Hunt. You will follow our game plan map navigating through the four corners of this magical island!
Explore in Voguish Chic St Barth, the "Exclusive French Island" loved by the jet-setter with a luxurious day trip from St-Martin. Its rivera style boutiques, gorgeous beaches, gourmet restaurants and stunning snorkeling will give you a sample of that magical French flavor. Savor all the facets of this 14 square mile gem in style and discover why the Rich and Famous call it the "Pearl of the Caribbean".
Its riviera style boutiques and bistros, gingerbread houses, gorgeous beaches wrapped in a magical French flavor make this gem a not to be missed while in St Martin! Come, live the magic and discover why the rich and famous call it the "Pearl of the Caribbean".
Take a quick 45 minute cruise in a new state-of-the-art motorboat, take a walking tour of Gustavia, the capital, and hop into a taxi for an all around one hour narrated tour of this enchanting island.
Enjoy your day in St Maarten at the famed Orient Beach and enjoy a welcome drink and lunch along with beach chairs and umbrellas. A great way to relax or to enjoy the water.
Let us grant you the opportunity to sail a tall ship, hear tales from the high seas and be a pirate for a day. The Lord Sheffield departs Dock Maarten/Great Bay Marina.
Four-time winner of the prestigious "Tour of the Year Award", Rhino Safari Excursions is St-Martins original, one and only interactive tour. Experience on-the-water excitement piloting your very own RHINO RIDER. These zippy 10 ft. inflatable motorboats are yours to command for thrill of a lifetime ride that is safe, sturdy, reliable and tons of fun! Unlike some other tours, you're not just going to be driving around in circles. Following your friendly guide, you'll cruise safely alongside mega-yacht marinas and boat anchorages before exiting Simpson Bay Lagoon to the French side capital of Marigot.
This is the absolute best excursion to maximize your day in St. Maarten. A combination of a sightseeing tour of the island in the morning plus a fun filled day on the beach.
This is a unique journey that is designed to give the participant an opportunity to experience both sides and cultures of the island. Enjoy a drive through the countryside, pass by the Great Salt Pond, and the French side of the island with a stop at the picturesque Marigot.


Originally Published by Policy Network 6 November 2014. Original linked here.
In Hungary, national, European and municipal elections this year have further solidified a unipolar party landscape, in which conservative party Fidesz has dominated. With the state of opposition parties in prolonged disrepair, liberal and leftwing voters continue to replace their electoral disillusionment with participation in protests and social movements. The most recent demonstrations taking place on 26 October and again on 28 October have seen an estimated 100,000 protest against Fidesz government initiatives.