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O WEC 47: Bowles vs. Cruz foi um evento de MMA promovido pelo World Extreme Cagefighting ocorrido no Nationwide Arena em Columbus, Ohio.

Backgrond

Esse foi o único evento do WEC a acontecer em Ohio, anteriormente o UFC já realizou três cards em Columbus.

Diego Nunes foi obrigado a se retirar de sua luta contra Leonard Garcia devido a uma lesão e foi substituído por George Roop.

Bryan Caraway foi obrigado a se retirar de sua luta contra Fredson Paixão devido a uma lesão no joelho e foi substituído por Courtney Buck, a luta foi remarcada para o WEC 50.

O evento reve como comentaristas os lutadores Stephan Bonnar e Frank Mir ambos do UFC. Também foi o último evento do apresentador de ringue Joe Martinez, Martinez apresentou o WEC 52 quando seu substituto Bruce Buffer estava apresentando o UFC 122 na Alemnaha.

Card do Evento

Card Preliminar
Luta de Peso Leve:  Ricardo Lamas vs.  Bendy Casimir
Lamas venceu por Nocaute (joelhada) aos 3:43 do primeiro round.
Luta dePeso Pena:  Fredson Paixão vs.  Courtney Buck
Paixão venceu por Finalização (mata leão) aos 2:39 do primeiro round.
Luta de Peso Pena:  Leonard Garcia vs.  George Roop
Garcia e Roop obtiveram um empate dividido (29–27, 27–29 e 28–28). Foi retirado um ponto de Roop devido a um chute aplicado na virilha de Garcia.
Luta de Peso Leve:  Danny Castillo vs.  Anthony Pettis
Pettis venceu por Nocaute (chute na cabeça e socos) aos 2:17 do primeiro round. Essa luta foi ao ar na transmissão.
Luta de Peso Pena:  Chad Mendes vs.  Erik Koch
Mendes venceu por Decisão Unânime (30–27, 30–27 e 30–27).
Luta de Peso Galo:  Scott Jorgensen vs.  Chad George
Jorgensen venceu por Finalização (guilhotina) aos 0:31 do primeiro round. Essa luta foi ao ar na transmissão.

Card Principal
Luta de Peso Leve:  Bart Palaszewski vs.  Karen Darabedyan
Palaszewski venceu por Finalização (chave de braço) aos 4:40 do primeiro round.
Luta de Peso Pena:  Deividas Taurosevičius vs.  LC Davis
Davis venceu por Decisão Majoritária (29–28, 29–28 e 29–29).
Luta de Peso Pena:  Jens Pulver vs.  Javier Vazquez
Vazquez venceu por Finalização (chave de braço) aos 3:41 do primeiro round.
Luta de Peso Galo:  Miguel Torres vs.  Joseph Benavidez
Benavidez venceu por Finalização (guilhotina) aos 2:57 do segundo round.
Luta pelo Cinturão Peso Galo:  Brian Bowles (c) vs.  Dominick Cruz
Cruz venceu por Nocaute Técnico (lesão) aos 5:00 do segundo round e se tornou o novo Campeão Peso Galo do WEC.

Bônus da Noite
Luta da Noite (Fight of the Night):  Leonard Garcia vs.  George Roop
Nocaute da Noite (Knockout of the Night):  Anthony Pettis
Finalização da Noite (Submission of the Night):  Joseph Benavidez

Referências

2010 nas artes marciais mistas

redpajama_set_name: RedPajamaWikipedia


Whitnash is next to both Warwick and Leamington, and can trace its origins back to before the Romans. Having grown dramatically during the post-war period, Whitnash became a town in 1978. The Plough and Harrow dates from the 17th century, and is still a pub in the present day.
The Parish Church of St. Margaret which was originally built during the Medieval period but which was largely rebuilt during the Imperial period. It is located on Whitnash Road, Whitnash.
Leamington Spa Airfield was extended by combining three fields into one area during the 20th Century.
Find spot - an Iron Age coin was found south of Ashford Road, Whitnash.
Find spot - a stone axe of Neolithic or Bronze Age date was found in the Whitnash area.
Find spot - assorted Post Medieval finds were found in the area of Whitnash.
Find spot - a coin of Post Medieval date was found in Golf Lane, Whitnash.
Find spot - a Roman coin was found on Church Lane, Whitnash.
This map shows markers for every photo, article, historic site and catalogue record within the Whitnash category.


There are too many stories to tell and general examples seem to paint my picture best. One chronicle I can think of, that may have had some influence happened in third grade. All I can recall about the teacher was some sort of tie dye jacket. But getting away from those details, this was the first year I learned to draw in three dimensions. I think, at least from what I can remember, I learned to write vivid coherent stories because of my new found ability to draw. The first small book I wrote because of these changes mixed up a vacuum and a rabbit in a tale; where the rabbit lived with his rabbit parents in a very rabbit like world. He had his rabbit parents and rabbit sister and just about rabbit everything. The rabbit's days changed when he was sucked into a powerful innovative, yet secretly magical vacuum his mother had purchased. A whole new world opened up to the rabbit. There was a forest with hazelnut colored leaves and all kinds of new furry woodland creatures inside. The story introduced its plot when the daring rabbit learned of a dangerous force had taken control of the vacuum world. The book, only about ten hand written pages, also had a lot of illustrations to go along with the story. Most of my influence here probably had to do with my amazing adventures with my friends and family in the forest.


text:
To Critics of The Beautiful Tree, a Pearl of a Reply
Really Good Schools: Global Lessons for High-Caliber, Low-Cost Education
By James N. Tooley
Independent Institute, 2021, $29.95; 273 pages.
As reviewed by Paul E. Peterson
Nuggets of amber occasionally reward patient beachcombers who wade through miles of cold, gray clay on the southern shores of the Baltic Sea. Nuggets likewise await the patient reader who wades through this dense, repetitive private-school apology.
Sixteen years ago, James Tooley, a professor at the University of Buckingham and the former director of the E. G. West Centre at Newcastle, wrote an essay that in 2009 became a pathbreaking book, The Beautiful Tree, which awoke the world to the reality of low-cost but effective private schools thriving in some of the poorest slums of the developing world. Many such schools, Tooley revealed, were outperforming expensive but inefficient state-run schools. So original was the work that Education Next saw fit to use its most telling episodes as the cover story for its Fall 2005 issue. The essay even won a prize, as Tooley is wont to remind us.
Tooley's Tree has been sturdy enough to weather stern criticism from state school defenders, international organizations, and Nobel Prize winners. Now, Tooley offers an extended reply.
Tooley is not a trained econometrician, and his methods are vulnerable to attack. His landscapes are drawn from personal observations, firsthand accounts, and participant testimonials, not the systematic surveys, quasi-experimental studies, and randomized field trials that mark most contemporary education research. The current book builds on prior research by introducing new entrepreneurial leaders who teach the children of the poor at a very low cost. Tooley's tales are of interest at a time when affluent parents in
rich countries are forming their own "learning pods" to replace the suddenly closed public schools during the coronavirus pandemic.
It isn't clear who the intended audience is for this book. Is Tooley still appealing to parents? Or is he now addressing the academic community by taking on critics and broadening his claims? Unclear as to his objective, the author wanders into dense thickets of controversy. Still, he offers up nuggets of gem-like quality.
The largest pearl is a critique of the world's biggest and most convincing school voucher experiment in Andhra Pradesh, an Indian state with a population of 50 million. To appreciate Tooley's critique of this study by Karthik Muralidharan and Venkatesh Sundararaman, one must first consider the original accomplishment. With the cooperation of the state government, and supported by funds from the World Bank, the two scholars drew a sample of 360 rural villages. Half of the villages were randomly assigned to receive vouchers, while the other half did business as usual. In the voucher villages, a random half of the sampled children attending state-operated schools were offered vouchers to attend private schools. The study could thus estimate the effects of being offered a voucher or not receiving that opportunity. It could also estimate the effects on all children in a voucher village as compared to those not living in a voucher village. Tracking students two to four years later, the researchers found little difference between those receiving vouchers and those who did not—or between voucher villages and the others. Learning in math, language of instruction, science, and social studies remained the same. The only advantage of receiving a voucher was that a child learned more Hindi, because the subject was only taught in the private sector. As the Times of India put it: "The findings dispel a popular myth that private schools lead to better learning."
Tooley found the study "disheartening." His only "comfort" was that the "private schools were on average doing the same for less than one-third the cost."
One cannot dismiss the study on the grounds that the researchers were fervent supporters of state-run schools, for they themselves had identified extreme inefficiency, if not corruption, in India's state schools, and the non-ideological quality of their other work suggests they are the kind of scholars who call it as they see it. The study was published in the Quarterly Journal of Economics, one of the profession's most prestigious journals.
But Tooley noticed a detail overlooked by others: the tests were administered in the language officially declared to be the medium of instruction at the school. For the state schools, that language was Telugu, the native tongue of Andhra Pradesh. Among the private schools, about half advertised themselves as teaching in Telugu, while the other half said they taught in English. It might seem to make sense that the research team would administer tests in a school's language of instruction, but Tooley points out that many of the private schools that report English as the language of instruction are expressing an aspiration more than a practice. While they may teach in English to older students, they conduct much of their instruction in the native tongue. In other words, the students in private schools who took the tests in English were being examined in their second language while the state-school students were being tested in their native tongue. Tooley says the appropriate way of comparing student performance in the two sectors would have been to administer tests to all students in both languages simultaneously. And, in fact, the original study reports that students attending Telugu-language private schools do better than those at state schools, a finding interpreted in the initial investigation as showing that students do less well if they change to a school where the language of instruction is not the same. Perhaps, but the more likely explanation is Tooley's: Students perform better on tests administered in their native tongue.
Professor James Tooley with students at an Omega private school in Bawjiase, Ghana.
After this triumph, Tooley takes on a consensus document from the the Department for International Development, the British agency responsible for foreign aid. Prepared by a group of scholars, the document reported "evidence . . . of inequality of access for girls to private schools," citing specifically a Tanzanian study that found fewer girls than boys in mixed-gender schools. The consensus document fails to note that many girls attend single-gender schools instead. Overall, 77 percent of the students recruited into private schools are female. This is just one of multiple instances of the department going off in its own misguided direction.
Nor do the Nobel Prize–winning economists Abhijit Banerjee and Esther Duflo escape Tooley's sharp knives. Admittedly, Banerjee and Duflo, in their book Poor Economics, find that "children in private school learn more than children in public schools." But Tooley also quotes them as saying private schools are not "as efficient as they could be" or as effective as state schools might be if they were not inefficient, corrupt, and focused on inappropriate goals. In other words, Banerjee and Duflo are judging private schools against an ideal standard rather than currently available alternatives.
Tooley's warm stories of entrepreneurial accomplishments and cutting critiques of other research both appear in the early chapters that comprise Part I. He might well have ended the book there, for the rest of the volume loses focus. Part II offers a rambling critique of government-operated schools, with a focus on the wayward policies of Tooley's home country. In Part III he takes on education reform across the pond. Tooley does not like charter schools, nor does he think much of vouchers. Forgetting his critique of Banerjee and Duflo for criticizing the real from some ideal standpoint, Tooley says choice interventions in the United States fall short of the libertarian economist E. G. West's vision of totally privatized schooling. For Tooley, the pandemic cannot last too long if it drives everyone to pod learning—even if the teachers managing the pods are poorly paid.
No one can accuse Tooley of iterating conventional wisdom. The Beautiful Tree proves that. But as Really Good Schools goes on and on, the author strays farther and farther from his main turf into lands better left untraveled.
Paul E. Peterson is the Henry Lee Shattuck professor of government at Harvard University, director of Harvard's Program on Education Policy and Governance, and senior editor of Education Next.
The post To Critics of The Beautiful Tree, a Pearl of a Reply appeared first on Education Next.
By: Paul E. Peterson
Title: To Critics of The Beautiful Tree, a Pearl of a Reply
Sourced From: www.educationnext.org/to-critics-of-the-beautiful-tree-pearl-of-reply-review-really-good-schools-tooley/
Published Date: Wed, 03 Mar 2021 10:00:40 +0000
EdNext Podcast: Keep Cameras on in Classrooms, Even after the Pandemic Ends
Biden Is Right, We Need Kids to Go Back to School But Not Like Before

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text:
Grace Akers
Grave site information of Grace Akers (21 Sep 1886 - 23 Nov 1965) at Indiana Veterans Cemetery in West Lafayette, Tippecanoe, Indiana, United States from BillionGraves
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Nasceu: 21 Sep 1886
Indiana Veterans Cemetery
3861-3959 Soldiers Home Road
West Lafayette, Tippecanoe, Indiana
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Grace Akers is buried in the Indiana Veterans Cemetery at the location displayed on the map below. This GPS information is ONLY available at BillionGraves. Our technology can help you find the gravesite and other family members buried nearby.
West Lafayette,Tippecanoe,Indiana
Life timeline of Grace Akers
Grace Akers was born on 21 Sep 1886
Grace Akers was 6 years old when Electrical engineer Nikola Tesla gives the first public demonstration of radio in St. Louis, Missouri. Nikola Tesla was a Serbian American inventor, electrical engineer, mechanical engineer, physicist, and futurist who is best known for his contributions to the design of the modern alternating current (AC) electricity supply system.
Grace Akers was 22 years old when Ford puts the Model T car on the market at a price of US$825. Ford Motor Company is an American multinational automaker headquartered in Dearborn, Michigan, a suburb of Detroit. It was founded by Henry Ford and incorporated on June 16, 1903. The company sells automobiles and commercial vehicles under the Ford brand and most luxury cars under the Lincoln brand. Ford also owns Brazilian SUV manufacturer Troller, an 8% stake in Aston Martin of the United Kingdom, and a 49% stake in Jiangling Motors of China. It also has joint-ventures in China, Taiwan, Thailand, Turkey, and Russia. The company is listed on the New York Stock Exchange and is controlled by the Ford family; they have minority ownership but the majority of the voting power.
Grace Akers was 26 years old when The British passenger liner RMS Titanic sinks in the North Atlantic at 2:20 a.m., two hours and forty minutes after hitting an iceberg. Only 710 of 2,227 passengers and crew on board survive. RMS Titanic was a British passenger liner that sank in the North Atlantic Ocean in the early hours of 15 April 1912, after colliding with an iceberg during its maiden voyage from Southampton to New York City. There were an estimated 2,224 passengers and crew aboard, and more than 1,500 died, making it one of the deadliest commercial peacetime maritime disasters in modern history. RMS Titanic was the largest ship afloat at the time it entered service and was the second of three Olympic-class ocean liners operated by the White Star Line. It was built by the Harland and Wolff shipyard in Belfast. Thomas Andrews, her architect, died in the disaster.
Grace Akers was 43 years old when The New York Stock Exchange crashes in what will be called the Crash of '29 or "Black Tuesday", ending the Great Bull Market of the 1920s and beginning the Great Depression. The New York Stock Exchange, is an American stock exchange located at 11 Wall Street, Lower Manhattan, New York City, New York. It is by far the world's largest stock exchange by market capitalization of its listed companies at US$21.3 trillion as of June 2017. The average daily trading value was approximately US$169 billion in 2013. The NYSE trading floor is located at 11 Wall Street and is composed of 21 rooms used for the facilitation of trading. A fifth trading room, located at 30 Broad Street, was closed in February 2007. The main building and the 11 Wall Street building were designated National Historic Landmarks in 1978.
Grace Akers was 44 years old when Great Depression: In a State of the Union message, U.S. President Herbert Hoover proposes a $150 million (equivalent to $2,197,000,000 in 2017) public works program to help generate jobs and stimulate the economy. The Great Depression was a severe worldwide economic depression that took place mostly during the 1930s, beginning in the United States. The timing of the Great Depression varied across nations; in most countries it started in 1929 and lasted until the late-1930s. It was the longest, deepest, and most widespread depression of the 20th century. In the 21st century, the Great Depression is commonly used as an example of how far the world's economy can decline.
Grace Akers was 59 years old when World War II: Hiroshima, Japan is devastated when the atomic bomb "Little Boy" is dropped by the United States B-29 Enola Gay. Around 70,000 people are killed instantly, and some tens of thousands die in subsequent years from burns and radiation poisoning. World War II, also known as the Second World War, was a global war that lasted from 1939 to 1945, although conflicts reflecting the ideological clash between what would become the Allied and Axis blocs began earlier. The vast majority of the world's countries—including all of the great powers—eventually formed two opposing military alliances: the Allies and the Axis. It was the most global war in history; it directly involved more than 100 million people from over 30 countries. In a state of total war, the major participants threw their entire economic, industrial, and scientific capabilities behind the war effort, blurring the distinction between civilian and military resources. World War II was the deadliest conflict in human history, marked by 50 to 85 million fatalities, most of whom were civilians in the Soviet Union and China. It included massacres, the genocide of the Holocaust, strategic bombing, premeditated death from starvation and disease and the only use of nuclear weapons in war.
Grace Akers was 69 years old when Disneyland Hotel opens to the public in Anaheim, California. The Disneyland Hotel is a resort hotel located at the Disneyland Resort in Anaheim, California, owned by the Walt Disney Company and operated through its Parks, Experiences and Consumer Products division. Opened on October 5, 1955, as a motor inn owned and operated by Jack Wrather under an agreement with Walt Disney, the hotel was the first to officially bear the Disney name. Under Wrather's ownership, the hotel underwent several expansions and renovations over the years before being acquired by Disney in 1988. The hotel was downsized to its present capacity in 1999 as part of the Disneyland Resort expansion.
Grace Akers died on 23 Nov 1965 at the age of 79
Browse > United States > Indiana > Indiana Veterans Cemetery > Grace Akers
Grave record for Grace Akers (21 Sep 1886 - 23 Nov 1965), BillionGraves Record 3512119 West Lafayette, Tippecanoe, Indiana, United States


India's cricket captain Virat Kohli, who is an avid Audi fan, revealed the German manufacturer's latest car in India, the Audi RS5 Coupe in Bangalore.
In the hometown of his Indian Premier League Team, the Royal Challengers Bangalore, Virat Kohli was part of the new Audi RS5 Coupe launch.
The India cricket captain has taken time out of his cricket schedule to launch the German car manufacturer's latest luxury car on Wednesday 11th April 2018.
Alongside the Head of Audi India, Rahil Ansari, the 29-year-old immediately fell in love with the RS5 Coupe.
Virat, who owns a fleet of Audi vehicles that include the R8, A8, Q7 and S6 is the first person to own an Audi RS5 Coupe in India.
A lighter 2.9 litre V6 TFSI Quattro engine is capable of producing 450bhp with the car able to go from 0-62mph in 3.9 seconds.
All-wheel drive (AWD) comes as standard with the RS5 Coupe, which should make for a smooth driving experience for one of the best cricketers in the world.
When it comes to the interior, Virat will be greeted with an all-black cockpit with the RS sports seats being stitched in Fine Nappa leather.
With all those features in mind, Virat spoke about his love of luxury cars. He said: "I am a big fan of luxury cars, both sedans and SUVs – and it depends on where I am going and what occasion I am attending.
Virat also explained about his association with Audi, as well as being one of the main faces to launch their latest range of cars.
He added: "Audi has made me feel like I am involved in all the innovations that come through which I think is the most important thing.
"They have given me respect; they have given me the feeling of being involved with the brand thoroughly which I am thankful to them for.
Mr Ansari spoke about what the Indian cricketing superstar brings with his association with Audi.
He said: "The Audi brand attributes are sporty, progressive and sophisticated and Virat Kohli embodies all these attributes perfectly.
He is not the only one to have purchased a new Audi in 2018 as Bollywood actress Kriti Sanon is an owner of the Audi Q7.
Many Indian actors and actresses have purchased Audi vehicles, not at least including Salman Khan (Audi RS7) and Saif Ali Khan (Audi Spyder R8).
The sporty, aggressive looks of the RS5 Coupe will definitely bowl over Virat as he takes his RS5 Coupe on the road.
At Rs. 10,650,000 (approx. £114,263 GBP and $163,151 USD), the new Audi RS5 Coupe is now available in all dealerships across India.
Images Credited to Audi India.
"it's clear they were cutting drugs on an industrial scale."


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Q: UIScrollView + Autolayout + Interface Builder: No scrolling, extra space at top after bounce I'm attempting to embed several sets of buttons and labels in a scroll view using Interface Builder and autolayout. I've tried nearly every solution I can find but nothing gets the scroll view scrolling (i.e. scrolling enabled + no bounces enabled = no movement). In addition, when I do enable bouncing, attempting to scroll down, while revealing the extra content but bouncing back up, leaves what is likely 20px more space at the top of the scroll view, as the content inset seems to get stuck at -20px in the y.
What I've tried so far:

*

*Setting content size, content insets manually. Doesn't and shouldn't work with auto layout.

*Setting every constraint I can find to make sure the scroll view can tell how big it is. Content size at runtime is still zero. This includes sizing constraints on the scroll view and positioning constraints on the buttons and labels inside.

*Various combinations of IB settings and metrics.

*Embedding the buttons and labels inside another UIView, which is inside the scroll view. No change.

*Read the similar questions and answers here.

I'd like to avoid writing code to do this, as it seems like the tools should be able to do this, but I will if I have to. But I'm at a loss; I haven't seen anything that would fix this that I shouldn't be able to do in IB just as well as code.

A: Adding height and width constraints, as well as size 0 spacing constraints between a content view and the scroll view seems to have fixed the scrolling issue, finally. Now if only I could figure out why the contentOffset is being set to 20 by default and when scrolling back to the top.

redpajama_set_name: RedPajamaStackExchange


What are ISRC codes, and how do I get them on my release?
ISRC codes are digital signatures that are embedded onto CD's that allow for the tracking and management of songs in the digital domain. They are usually required by online music distributors such as iTunes. If you want them on your CD, you need to provide them to us before your master is finished -- only the artist or label can obtain these codes, you must acquire them and send them to us. Please use this spreadsheet to provide us with your ISRC codes.
What exactly are you going to do to my album?
How do unattended sessions work?
How do I make my titles appear in iTunes or other computer software?
How do I make vinyl records?
Will you make my CD louder than a hydrogen bomb if I ask nicely?
Who is Grey Market Mastering?


Quadruple jumps were limited, the practice of backloading programs to gain bonus points was severely curtailed, and neither a major conflict-of-interest issue nor raising the minimum age for senior competitions was even approved for discussion.
Those were the major takeaways from the biennial International Skating Union congress last week in Seville, Spain.
But the impact of what did -- and did not -- happen at the 57th ISU Ordinary Congress will likely be far less significant than the ramifications of ISU Communication No. 2168 (pdf), issued 10 days before the congress began.


text:
Q: Filezilla public_html set permission from 00 to 750 How do I set permission to public_html folder ?
Now it has permission 00 and when entering my site I get Forbidden error 403.
And when I'm trying to open public_html folder I get:

550 Can't change directory to public_html: Permission denied

Thank you.

A: Use these commands:
(For ownership) sudo chown -R user:group folder/
(For permisions) sudo chmod -R 664 folder/

Check out the this wikipedia entry to learn more about chmod http://en.wikipedia.org/wiki/Chmod


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HomeAlzheimerSymptoms Alzheimer's Early Onset
AlzheimerMust Read
Symptoms Alzheimer's Early Onset
Latest Advances In Alzheimers Disease Fluid Biomarkers
The past several years have witnessed dramatic advances in the analysis of p-tau species in the CSF and plasma as potential AD biomarkers . Measurements of plasma tau phosphorylated at residues 181 and 217 in particular have shown that these tau species have remarkable accuracy as candidate biomarkers of AD diagnosis and progression, both in CSF and plasma . However, much work remains to be done in determining the validity of these biomarkers in diverse populations that have thus far been underrepresented in these studies.
What Is Alzheimer's Disease
Alzheimers disease is the most common form of dementia, affecting up to 70% of all people with dementia. It was first recorded in 1907 by Dr Alois Alzheimer. Dr Alzheimer reported the case of Auguste Deter, a middle-aged woman with dementia and specific changes in her brain. For the next 60 years Alzheimers disease was considered a rare condition that affected people under the age of 65. It was not until the 1970s that Dr Robert Katzman declared that "senile dementia" and Alzheimers disease were the same condition and that neither were a normal part of aging.
Alzheimers disease can be either sporadic or familial.
Sporadic Alzheimer's disease can affect adults at any age, but usually occurs after age 65 and is the most common form of Alzheimer's disease.
Familial Alzheimers disease is a very rare genetic condition, caused by a mutation in one of several genes. The presence of mutated genes means that the person will eventually develop Alzheimer's disease, usually in their 40's or 50's.
The Healthy Human Brain
Behind the ears and temples are the temporal lobes of the brain. These regions process speech and working memory, and also higher emotions such as empathy, morality and regret. Beneath the forebrain are the more primitive brain regions such as the limbic system. The limbic system is a structure that is common to all mammals and processes our desires and many emotions. Also in the limbic system is the hippocampus a region that is vital for forming new memories.
Stage : Moderate Dementia
Patients in stage 5 need some assistance in order to carry out their daily lives. The main sign for stage 5 dementia is the inability to remember major details such as the name of a close family member or a home address. Patients may become disoriented about the time and place, have trouble making decisions, and forget basic information about themselves, such as a telephone number or address.
While moderate dementia can interfere with basic functioning, patients at this stage do not need assistance with basic functions such as using the bathroom or eating. Patients also still have the ability to remember their own names and generally the names of spouses and children.
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Changes In Mood Or Emotion
The person may be more anxious, frightened or sad, and so at risk of depression. It is also common to become more irritable perhaps in frustration at lost abilities or easily upset. A person can often be more withdrawn, lack self-confidence and lose interest in hobbies or people.
Changes in behaviour are not common in early-stage dementia, other than in FTD. A person with behavioural variant FTD may lose their inhibitions and behave in socially inappropriate ways. They may also act impulsively and lose empathy for others.
Significant physical changes at this stage tend to be limited to DLB, where problems with movement are similar to Parkinsons disease. If someone with vascular or mixed dementia has a stroke, this can lead to weak limbs on one side.
Need help finding dementia information?
Everybody forgets things from time to time. But if you or other people are noticing that memory problems are getting worse, or affecting everyday life, it could be a sign of dementia.
Mapt Variation In Clinical Early
A subset of variants in MAPTencoding the microtubule-associated protein tau and the causative gene for chromosome 17-linked familial FTD with parkinsonism have been found in cases of early-onset dementia resembling clinical AD. In particular, the p.R406W variant is often associated with a clinical phenotype resembling EOAD . This phenotype may be connected to the observations that p.R406W tau can form the paired helical filaments that make up NFTs in AD and that individuals harboring the p.R406W variant have abnormal levels of p-tau217a marker that is otherwise very specific for ADin the absence of amyloid pathology . Independent of causative alleles, the rare p.A152T variant of MAPT has been identified in several individuals with sporadic EOAD after having previously been found to increase risk for both AD and FTD .
Fig. 3: Alzheimers disease tau pathology can be induced by distinct amyloids and specific MAPT variants.
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If you think you notice the signs of Alzheimerâs in yourself or a loved one, the best thing to do is to talk to a doctor. They can let you know what the symptoms mean and what your options are for treating them. There are new advances available which can help with early detection and treatment. One is as simple as a blood test to determine the presence or absence of proteins that may indicate there are Alzheimer's associated plaques in the brain.
Wandering Or Getting Lost
Wandering also features prominently as one of the warning signs of early-onset Alzheimers. Studies show that 6 in 10 people who have the disease will wander.
Persons with the illness may become disoriented because they cannot remember where they are coming from or their destination. This can make them get lost or wander even on familiar grounds.
A couple of factors may contribute to wandering. These include fear, following past routines like going to their favorite store, boredom, or wanting to satisfy basic needs like eating or using the toilet.
Wandering can pose safety issues if a person is not doing it in a controlled, safe environment. Caregivers should, therefore, come up with adequate preventive measures to deal with wandering.
Don't Miss: Can Dementia Get Worse Suddenly
Putting Things In Strange Places
Early onset Alzheimer's disease – Hilary's story: The dementia guide
Everyone forgets where they put their keys every once in a while, and sometimes you're so tired that you might accidentally put the milk in the cupboard. That's totally normal! For those with Alzheimer's, though, misplacing possessions and putting them in places that don't make sense happens with startling frequency, according to the Mayo Clinic. And for more age-related health issues to be aware of, check out these 40 Things Doctors Say Affect Your Health After 40.
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Difficulty Completing Familiar Tasks
Some people may experience a greater problem with concentration. Routine day-to-day tasks requiring critical thought may take longer as the disease progresses.
The ability to drive safely may also be called into question. If you or a loved one gets lost while driving a commonly traveled route, this may be a symptom of AD.
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Conditions With Symptoms Similar To Dementia
Remember that many conditions have symptoms similar to dementia, so it is important not to assume that someone has dementia just because some of the above symptoms are present. Strokes, depression, excessive long-term alcohol consumption, infections, hormonal disorders, nutritional deficiencies and brain tumours can all cause dementia-like symptoms. Many of these conditions can be treated.
What Can You Do About It
Unfortunately, there is no cure for Alzheimer's or other forms of dementia. According to the Alzheimer's Association, 1 in 10 seniors over the age of 65 has dementia. Though the disease affects each patient differently, most people with Alzheimer's live only 4 to 8 years after diagnosis.
While you cannot reverse dementia or the damage it causes, there are ways to improve quality of life. Here are some simple tips for management that you can discuss with your doctor:
Take prescription medications to counteract cognitive and behavioral symptoms such as anxiety, depression, and mood swings.
Find support in the form of therapy, support groups, friends, or family to help develop coping mechanisms for cognitive and behavioral changes.
Address safety issues in the home by installing safety bars in the bathroom and shower, automatic shut-off switches on appliances, and reminders to lock the door.
Stay on top of co-existing conditions, working with your doctor to manage medical problems with the proper form of treatment.
Follow a healthy diet that supports brain health and function. Focus on antioxidant-rich fruits and vegetables, natural sources of omega fatty acids, and foods high in fiber and protein.
Talk to your doctor about taking supplements to support memory and cognitive function. Options you might consider include caprylic acid, coenzyme Q10, ginkgo biloba, phosphatidylserine, and omega-3 fatty acids.
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Early Warning Signs Of Alzheimers Disease Include:
Difficulty recalling newly learned information
Forgetting appointments
Trouble with word recall or language comprehension
For most of us, forgetting things is just a normal part of aging, Garrett said. You dont need to worry about Alzheimers disease just because you forgot where you parked your car unless it happens all the time. But if youre consistently forgetting things, Id recommend that you contact your doctor.
There are many potential causes of Alzheimers-like symptoms, including brain injuries, stroke, heart disease, severe infections, sleep apnea, vitamin B12 deficiencies, and diabetes. So while Alzheimers disease has no known cure, many of the other dementia-causing conditions can be treated. Plus there are some medications and treatments that have had some success in slowing the progression of Alzheimers if theyre administered early. Thats why its important to see a doctor soon if youve noticed signs of memory disorders.
Early Symptoms Of Dementia
Misplaced your keys again? Forgot the title of that movie you saw last night? How can you tell whether you're just having a âsenior moment," or if there's a more serious health problem to consider? Current treatments available for dementia are more effective when the condition is caught in its early stages, so it's important to know when a âsenior moment" might really be a sign that it's time to see your doctor.
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Identification Of The Major Mendelian Early
A crucial genetic discovery in EOADwhich has been massively influential for the course of research into all forms of ADoccurred 30 years ago with the mapping of a missense variant in APP that segregated with disease in an autosomal-dominant EOAD family . Subsequent studies identified pathogenic variants in PSEN1 and PSEN2 in additional autosomal-dominant AD families . Analysis of LOAD families has more recently resulted in the identification of rare, risk-conferring variants and established pathogenic variants in APP, PSEN1, and PSEN2, thus suggesting that these genes may also be relevant for the more common, late-onset variety of AD . Additional studies using data from the AD Sequencing Project also provide suggestive evidence that rare variation in PSEN1 increases risk for LOAD . Given the potent influence that the amyloid cascade hypothesis has had on the field and on AD drug development, the finding that variants in these genes may also confer risk for LOAD provides important support for the generalizability of this hypothesis to all forms of AD.
Frequently Asked Questions About Dementia
Into the Fog: Living with Early-Onset Alzheimer's | WebMD
What are the early signs and symptoms of dementia and Alzheimer's?Some of the most common early signs of dementia and Alzheimer's symptoms include trouble remembering recent events, difficulty concentrating, increased mental confusion, changes in behavior or personality, apathy or withdrawal, and depression or anxiety. While these first signs of dementia may seem somewhat unassuming it is important to notice when these symptoms are occurring on a regular basis.
Is short-term memory loss a sign of dementia?Changes in memory is a normal sign of aging, but significant memory loss may be a sign of dementia. Additionally, having trouble remembering recently learned information can be an early warning sign of dementia.
What is the life expectancy of someone with dementia?Life expectancy depends largely on the patient's age and health, and can range anywhere from 1 to 26 years, according to one study. Every case is different, and it depends on the type of dementia the patient has. The general life expectancy for an Alzheimer's patient is 8 to 12 years from the date of diagnosis. Patients diagnosed around the age of 60 tend to decline more slowly than those diagnosed over the age of 80.
Can dementia be cured?There is no curative treatment for dementia currently available and no vaccination to prevent it. Medication is available to help relieve symptoms, and certain lifestyle changes may slow the progression of the disease.
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Struggling To Adapt To Change
For someone in the early stages of dementia, the experience can cause fear. Suddenly, they cant remember people they know or follow what others are saying. They cant remember why they went to the store, and they get lost on the way home.
Because of this, they might crave routine and be afraid to try new experiences. Difficulty adapting to change is also a typical symptom of early dementia.
Limitations And Interpretation Of Genetic Studies Of Early
In the sections that follow, we highlight associations of several genes with clinical EOAD that are better known for their role in other neurodegenerative diseases. When interpreting the results of genetic studies of EOAD, it is important to ask several questions. First, is the phenotype in question clinically diagnosed EOAD or pathologically confirmed EOAD? If the former, is there good reason to believe the underlying neuropathology is AD? If such evidence is not presented, interpretation of the results should be shaped by the possibility that any identified variants may actually contribute to clinical EOAD via non-AD pathology. The importance of these questions is further highlighted by the broad spectrum of clinical EOADand particularly the atypical syndromeswhich may overlap with that of etiologically distinct neurodegenerative disorders. Finally, it is important to remain cognizant of the fact that many genetic studies have focused, for reasons of cost and practicality, on genes already known to be implicated in AD and other forms of dementia or neurodegeneration. The above factors and biases have cumulatively played an important role in shaping our current knowledge regarding the genetics of EOAD.
Recommended Reading: Can A Person Diagnosed With Dementia Change Their Will
Warning Signs Of Alzheimer's
Memory often changes as people grow older. Some people notice changes in themselves before anyone else does. For other people, friends and family are the first to see changes in memory, behavior, or abilities. Memory loss that disrupts daily life is not a typical part of aging. People with one or more of these 10 warning signs should see a doctor to find the cause. Early diagnosis gives them a chance to seek treatment and plan for the future.
1. Memory loss that disrupts daily life: forgetting events, repeating yourself or relying on more aids to help you remember .
2.Challenges in planning or solving problems: having trouble paying bills or cooking recipes you have used for years.
3.Difficulty completing familiar tasks at home, at work, or at leisure: having problems with cooking, driving places, using a cell phone, or shopping.
4.Confusion with time or place: having trouble understanding an event that is happening later, or losing track of dates.
5.Trouble understanding visual images and spatial relations: having more difficulty with balance or judging distance, tripping over things at home, or spilling or dropping things more often.
The Centers for Disease Control and Prevention and the Alzheimers Association have created the Healthy Brain Initiatives State and Local Public Health Partnerships to Address Dementia: The 2018-2023 Road Map.
8. being a victim of a scam, not managing money well, paying less attention to hygiene, or having trouble taking care of a pet.
Signs Of Dementia Where To Find Help
When your loved one is displaying troubling symptoms, a trip to a primary care physician is often the first step. But to get a definitive diagnosis, youll need to see a specialist such as a neurologist, geriatrician or geriatric psychiatrist.
If you cant find one, the National Institute on Aging recommends contacting the neurology department of a nearby medical school. Some hospitals also have clinics that focus on dementia.
Ailments can mimic dementia
Specialists will want to know about the patients personal and family medical history. A close relative or relatives having had Alzheimers is a major risk factor.
Recent research suggests that a prevalence among even members of your extended family can increase your dementia risk. Doctors also will conduct physical and neurological exams to rule out other treatable causes for dementia symptoms.
Some of the methods that doctors use to diagnose dementia:
Cognitive and neuropsychological tests assess language and math skills, memory, problem-solving and other types of mental functioning.
Lab tests of blood and other fluids, including checking levels of various chemicals, hormones and vitamins, can help rule out nondementia causes for the symptoms.
Brain scans such as CT, MRI or PET imaging can spot changes in brain structure and function. These tests also can identify strokes, tumors and other problems that can cause dementia.
More on Dementia
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Sounds European!: Germany | Alice Merton - "Funny business"
German star Alice Merton has just released another amazing song. It's entitled "Funny business", and it is another song with Alice's trademark sounds: it's classy, it's exciting and it's highly entertaining!


Ultimately, it's up to lawmakers to weigh the economic consequences of these laws, and industry lobbyists are working hard to ensure they're informed. Over the last two months alone, several proposals have been introduced in the Senate. There's senator Brian Schatz's (D-HI) Data Care Act, which would require companies to "reasonably secure" user data, and give the FTC new powers to fine companies that abuse that data. Senator Marco Rubio (R-FL), meanwhile, introduced a bill that would entrust the FTC with crafting new privacy guidelines to be approved by Congress. Following Cook's piece in TIME, senator Markey announced his intention to reintroduce the Data Broker Accountability and Transparency Act, which would enable people to request their data from data brokers, and either correct it or order brokers to stop using it. Of course, at a time when the government has been shut down for more than a month and bipartisan consensus seems harder than ever to come by, the fate of these bills is uncertain.


Hello folks! Sorry for leaving this blog unattended for a while. I'm Annie, the new Alumni Coordinator, and I thought I'd write a nice summary of the 2012 Football Season. At the start of the season we weren't expecting anything out of the ordinary from our team, but after a 3-game winning streak in the Ivies and two fountain gigs, the Tigers were in the middle of the best season they'd seen in years.
-Shirley Tilghman joining us in the stands at the Dartmouth game.
Shirley visits the band in the stands!
-Oh right, and a Bonfire for the first time since 2006!
What an incredible season for Princeton Football, who ended up 4-3 in the Ivy League.
A great big thanks to all our wonderful officers from this past year for all their hard work in engineering yet another undefeated season for the one and only Princeton University Band!


cheertechnique. Speeds are up by 90-95. Also, I can039;t tell if you039;re trying to put a song on a mp3 player, CD or what. Then drag them from the downloaded folder to the media player and burn them. music-buzz. comactress_1265. My husband just got an Ipod touch and Yule want him to know how to Yule free downloads. html Can anyone help me with Yule Z dubbing information?165Alright Yule I039;m hoping to start watching DBZ again after Yule 10 years and I found 3 different downloads for the series but I039;m kinda confused about which one to DLwatch One is Funimations DBZ Remastered (not Kai).br-Copy the HTML codetag from the MP3 player039;s website (click 039;Generate the Code.


Nice post! It's an interesting concept and I think it's great that people are talking about it more. I find it repulsive how big companies try to use IP as weapons, and the only people really laughing all the way to the bank are the lawyers!!!
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Home All issues Volume 529 (May 2011) A&A, 529 (2011) A123 Full HTML
Volume 529, May 2011
2. Observations
Period persistence of long period oscillations in sunspots
N. Chorley1, C. Foullon1, B. Hnat1, V. M. Nakariakov1,2 and K. Shibasaki3
1 Centre for Fusion, Space and Astrophysics, Physics DepartmentUniversity of Warwick, Coventry CV4 7AL, UK
e-mail: n.d.y.chorley@warwick.ac.uk
2 Central Astronomical Observatory of RAS at Pulkovo, 196140 St Petersburg, Russia
3 Nobeyama Solar Radio Observatory/NAOJ, 384-1305 Nagano, Japan
Long period oscillations in the microwave radiation intensity generated over the sunspot of NOAA AR 10330 are studied with the Nobeyama Radioheliograph as the sunspot passes over the solar disk, over the course of 9 days (06−15 April 2003). Periodogram, Fourier and global wavelet analyses reveal the presence of a significant oscillatory component in the range P ≈ 50−120 min over the course of the observations. The spectral amplitudes of five significant Fourier components in the range P = 50−150 min are also seen to be stable over the observations, when the data are not affected by changes in magnetic configuration in the region. The ground-based nature of the instrument naturally introduces long data gaps in such long duration observations and the presence of the gaps does not allow any conclusion as to the stability of the phases of the oscillations. As a model to explain the persistence of the dominant long periods, a simple oscillator with a nonlinear driving term is proposed. The spectral difference between distinct peaks within, e.g. the 3 min spectral band, is expected to be able to resonate with the long period one hour oscillations.
Key words: Sun: oscillations / Sun: activity / sunspots
Sunspots are the most visible manifestation of the solar magnetic field in lower regions of the solar atmosphere and are interesting features to study as they may provide clues about the nature of the mechanism for generating the magnetic field, the solar dynamo. Associated with them may be filaments – dark, cool structures which lie parallel to the magnetic polarity inversion line in the region.
Long period (P > 10 min) oscillations in sunspots could be connected with large scale reconfiguration of the Sun's magnetic field, or even the leakage of waves (g-modes) from the solar interior. The nature of such oscillations is not understood, though several studies have sought to answer this question. Berton & Rayrole (1985), using photospheric magnetic and velocity data in the neutral iron line λ = 630.2 nm, first observed torsional oscillations in the umbral magnetic field of a sunspot, with periods of approximately 45 min and suggested that these could be related to magnetohydrodynamic (MHD) oscillations generated at the top of the solar convection zone. Sunspot penumbrae were also found to oscillate, as reported by Druzhinin et al. (1993), in the Doppler velocity of two spectral lines of photospheric origin (with periods around 60 min). Moreover, optical observations by Nagovitsyna & Nagovitsyn (2002) indicated two kinds of oscillation mode, with periods ranging from 40 to 100 min – one associated with sunspots and the other with pores (sunspots without umbrae). Nagovitsyna & Nagovitsyn (2001) also used optical observations to detect quasi-hourly oscillations in magnetic fragments in sunspots, finding that the oscillation had its maximum amplitude in the penumbra and that there was an anisotropy of the oscillation in the azimuthal direction.
More recently, Efremov et al. (2009) detected periods of 60 − 80 min in the Doppler shift of six spectral lines formed at different heights in the sunspot atmosphere and found that the power of the long periods decreases with height; the oscillations were well pronounced at a height of 200 km and barely seen at a height of 500 km. Efremov et al. (2010) detected periods in the range 40 − 180 min in wavelengths formed between 190 km and 535 km (periods of 250 and 480 min were found in the line-of-sight magnetograms from space-borne SOHO/MDI data).
Fig. 1
Images of AR 10330 in white light (left) and microwave (17 GHz, centre) taken at 23:59 UT on 09 April 2003 and in Hα (right), taken at 01:03 UT on 10 April 2003.
In microwave emission above sunspots, oscillations of tens and hundreds of minutes have been detected (Gelfreikh et al. 2006; Chorley et al. 2010) with the Nobeyama Radioheliograph (NoRH, Nakajima et al. 1994). In particular, Chorley et al. (2010) indicated the presence of two periodicities in each analysed sunspot. Spatial analysis revealed that most of the spectral power was located above the umbral regions and strongly suggested that there were two regions of coherent oscillation that oscillated in anti-phase with each other.
Finally, it may be noted that long period oscillations have also been observed in coronal structures, which all have the source of their magnetic fields in sunspots. For example, Foullon et al. (2004, 2009) detected periods of several hours in extreme ultraviolet (EUV) observations of solar filaments (using SOHO/EIT) and Verwichte et al. (2010) studied transverse oscillations in large coronal loops observed with TRACE and SOHO/EIT, with periods between 24 and 180 min.
In this paper, we study 9 successive observation intervals of one of the sunspots studied by Chorley et al. (2010) in order to investigate the lifetime of the long period oscillations. The paper is organised in the following way: Sect. 2 presents the observations and preprocessing of the data and in Sect. 3, we detail our analysis and results. Finally, in Sect. 4, we discuss our results and propose a simple model for the generation of the observed oscillations.
The sunspot of NOAA active region (AR) 10 330 was observed over intervals of approximately 7.25 h on 9 successive days with NoRH (based in Japan), beginning on 06 April 2003 and ending on 15 April 2003. The observations began at 22:45 UT on each day and ended at around 06:30 UT the following day. At the beginning of the observation period, the region was located at a position of (−572,199)′′, relative to disk centre. For convenience, throughout this paper, we refer to observations on each date (e.g. time series) by a number corresponding to their position in the sequence of 9 days (i.e. 1 for 06 April, 2 for 07 April, etc.).
Figure 1 shows the region in white light (from SOHO/MDI) and microwave on 09 April 2003 and Hα (from the Yunnan Astronomical Observatory) on 10 April 2003. The Hα image shows evidence of a filament associated with the region, located north-west of the main region. This region has been studied by Sainz Dalda & Martínez Pillet (2005) and Zhang et al. (2007), who investigated moving magnetic features and their relation to penumbral filaments and evolution of the parent sunspot. The studies of both groups used data in the interval 09 April 2003 14:00 UT − 10 April 2003 00:50 UT. In addition, the observations used in this work include those used in Chorley et al. (2010) (08 April 2003 22:45 UT − 09 April 2003 06:30 UT).
Sequences of images were obtained for each date from NoRH at a frequency of 17 GHz. The emission is generated by the gyroresonant mechanism, where a low harmonic of the cyclotron frequency is equal to the frequency of the instrument (Shibasaki et al. 1994; Vourlidas et al. 2006). The images are of size 8 × 8 pixels, with a spatial resolution of 10′′ per pixel and the time cadence is 10 s. This is a restricted field of view to minimise the contribution from the quiet Sun. Due to the long intervals of observation, the solar rotation has to be taken into account. The starting position is converted to heliographic longitude and latitude and the change in longitude is found every 10 s. In this way, we obtain new centre coordinates for the next image from the coordinates of the previous one.
From each daily set of images, we generated a time series by computing the mean brightness temperature, TB, of each image. Present in each time series is a large scale trend mainly due to the change in effective area of the instrument as the Sun passes overhead during the course of the local day. The trend is removed by fitting a 4th order polynomial and spectrally filtering the time series to remove oscillations with 3 cycles or fewer (P ≥ 145 min). Figure 2 shows the resulting detrended time series.
Most of the time series generated in this way contain large increases in TB, that are most likely to be flares, and several glitches. All such features are identified and then removed from the time series by interpolation with a cubic spline. To identify the flares, we set a threshold on TB of 8.5 × 104 K for most time series (except for days 5 and 9, for which values of 6.5 × 104 K were used). For the amplitude study described in Sect. 3 below, we did not remove the spikes in the signals.
Time series of microwave intensity generated from sequences of images of AR 10330 obtained with NoRH. The signals have been detrended with a 4th order polynomial. The title for each signal gives the day number in the sequence of the 9 days of observation.
We computed Fourier power spectra, Lomb-Scargle periodograms (Scargle 1982) and global wavelet spectra (see, e.g. Torrence & Compo 1998) for each detrended and interpolated time series in order to investigate the long period oscillations. Figure 3 shows the spectra obtained by each of these methods, for each of the 9 time series. It can be seen that long period oscillations in the range P = 50−120 min are present in all time series and that there are, in general, two long period peaks in the spectra.
Figure 4 presents information related to the solar activity and an analysis of the dominant periods, in order to determine whether any events in the region could have been responsible for changes in the observed period.
We obtained the full disk flux observed by the GOES spacecraft and identified flares and CMEs that occurred in AR 10330, as well as in other regions, during our observation period. This is shown in panel (a) and it is clear that the Sun was quite active during the entire 9 days of observations, as evidenced by the large number of peaks in the GOES flux. However, it can also be seen that there were two events in the region during the observations: a filament disappearance (beginning after 08 April 2003 00:45 UT and ending before 08 April 2003 13:02 UT) and a C class flare that occurred on 13 April 2003 at 08:45 UT. These events are indicated by dashed vertical lines.
In panel (b), we show the original time series generated from the sets of NoRH images. Large increases in brightness temperature can be seen, which do not appear to coincide with peaks in the GOES flux. The reason for this could be that small events (relative to the full disk flux) in the region do not necessarily appear in the full disk GOES flux, but can cause large local brightenings due to the restricted field of view. It can also be seen that there is a trend in the mean intensities in the signals over the 9 days of observations. For the first 7 of those days, the trend is roughly symmetric about the interval between signals 3 and 4, when the sunspot crosses the central meridian. In addition, the mean intensity is seen to decrease for signals 8 and 9, which is attributed to the sunspot being positioned close to the limb on those days and both of these points are suggestive of a projection effect.
In panel (c), we show the dominant periods (i.e. the periods corresponding to the highest spectral peak) in the range P = 50−120 min and all three methods give similar values (within the error bars of the global wavelet), except in the last case. It can also be seen that the dominant period remains quite stable over the course of the observations. The dominant period appears to reach a local minimum in signal 7 before the flare in the region and is seen to rise after it. This decrease in period could be associated with changes in magnetic configuration that may or may not lead to a flare.
In panel (d), the power of each of the 5 long period Fourier components in the range P = 50−150 min is shown for each of the 9 days. The signals were first filtered to contain only periods in this range, using a boxcar function as the filter. The first feature of note is the large rise in power in all 5 components for signal 6. This is artificial since the time series contains large peaks (see Fig. 2) that are of a finite width and as such, the detrending procedure introduces an artificial oscillation whose period is close to those of interest. The amplitudes for all components over the days excluding day 6 do not appear to vary by a large amount.
Normalised power spectra obtained for each of the 9 detrended signals, using the global wavelet (black), Lomb-Scargle periodogram (red) and FFT (blue). Each spectrum has been normalised to its maximum amplitude. As in Fig. 2, the title for each signal gives its position in the sequence of the 9 days of observation.
We also attempted to investigate the change in phase of the long period oscillations over the 9 days of observations in the following way. For each of the 5 Fourier components in the range P = 50−150 min range (after filtering), we found the phase for each of the 9 signals. Naturally, one is interested in the phase of the oscillation at some common reference point, here chosen as the beginning of the observations (06 April 2003 22:45 UT). In order to obtain Fourier phases with respect to this common reference, we made use of the time delay relation of the Fourier transform ℱ, of a signal , (1)where t0 is the time delay and f the frequency. Equation (1) tells us that a time delay is seen as a phase shift in the Fourier transform. In order to obtain the phase of the oscillation at the beginning of the observations, we divide ℱ[I(t − t0)] by e − i2πft0 to give and then find the phase from the real and imaginary parts of the relevant component. Figure 5 shows a polar plot of the phases for each of the 5 components, on each of the 9 days. It is clear that the phases for different components behave in different ways over time and that there does not seem to be any long term stability in the phases (over the entire course of the observations).
a) The GOES X-ray flux during the period 06 April 2003 20:00−15 April 2003 10:00, showing events that occurred in AR 10330 and elsewhere. b) The original time series obtained from NoRH images. The Mt. Wilson classification for AR 10330 is also shown. c) The dominant periods in the range P = 50−120 min, obtained with all three of the methods for computing the power spectrum. The error bars on the global wavelet spectrum were obtained using the full width at half maximum (FWHM) of the corresponding spectral peak. d) The power for each Fourier component in the range P = 50−150 min for each day. In panels c) and d), the points for each day have been plotted at the midpoint of each signal.
We have analysed nine 7.25 h intervals of microwave emission at 17 GHz over NOAA AR 10330, observed with the Nobeyama Radioheliograph. The main finding of this study is that long period oscillations (P ≥ 50 min) are found to be present in each of the analysed time intervals and the dominant long period component appears to be stable over the observations. The apparent change in period between 13 April 2003 06:30 and 13 April 2003 22:45 (the interval between signals 7 and 8) could be due to changes in magnetic configuration in the region. In addition, the spectral amplitude of 5 Fourier components in the range P = 50−150 min shows stability over the course of the observations, when the data are not influenced by changes in magnetic configuration or large flares (as on day 6). The large time gaps between the data sets, together with the noise in the signals do not allow us to draw any firm conclusions about the stability of the phases of the oscillations.
Long period oscillations in sunspots can be associated, for example, with the global oscillations of the sunspots in terms of the shallow sunspot model (Solov'ev & Kirichek 2008). However, the persistence of those oscillations requires the answer to an additional question: what is the physical mechanism that excites those modes in the quiet Sun and how are the oscillations maintained against the damping? One possibility is the resonance between a certain driver and the natural frequency of the sunspot. Such a driver could be associated with the 3 min oscillations of sunspots, which are known to be very persistent narrowband features. Usually, 3 min oscillations are seen to have a fine spectral structure, having multiple peaks (see, e.g. Shibasaki 2001; Gelfreikh et al. 1999). The average spectral width of the cluster of 3 min peaks corresponds to a period of about an hour and hence, it can resonate with the long period oscillations of a sunspot, exciting the long period oscillations and compensating for the damping. However, such a process is possible only in the presence of nonlinear effects.
To illustrate this possibility, we consider a driven simple harmonic oscillator in which the driver is nonlinear, e.g. (2)where k is the damping coefficient, ω0 is the natural frequency of oscillation (corresponding to a period of P ≈ 100 min), the Ai, ωi and φi are the amplitudes, frequencies and phases of the driving oscillations and m is the number of driving oscillations, which represent individual peaks of 3 min oscillations. The nonlinearity represents some physical mechanism responsible for the coupling of 3 min and long period oscillations. For example, it can be the modification of characteristic speeds of long period oscillations by the 3 min oscillations.
We stress that Eq. (2) is an empirical model that reflects the observed properties of the oscillations. As such, we make no attempt to estimate the value of k, but only include damping in the model as we know it is a physical effect (due to, e.g. viscosity or leakage of the oscillations to the corona). In addition, ω0 is related to the magnetic field strength, sunspot depth and mass density as given in Solov'ev & Kirichek (2008).
Expanding the expression on the right hand side of Eq. (2) leads to two kinds of terms, for i ≠ j:
(i): cos2ωit, which can be expressed in terms of cos2ωit;
(ii): cosωitcosωjt, which can be expressed in terms of and .
The first kind of term gives frequency doubling and we suggest that a broadband spectrum of solar 5 min oscillations can contribute to the 3 min oscillations. The second kind of term, in particular the ωi − ωj kind, suggests that two frequencies close together will generate a low frequency oscillation. As explained above, we suggest that the 3 min part of the spectrum is responsible for this effect.
The phases for each Fourier component over the 9 days of observation after filtering the signals to contain only periods in the range P = 50 − 150 min. Phases are given in degrees and the points for each day lie on an annulus at r = 1,2,...,9, corresponding to the day number (i.e. 1 for 06 April 2003, 2 for 07 April, etc.).
The results presented in this paper demonstrate the need for the long-term study of long period oscillations in sunspots, their possible relationship with 3 min oscillations and theoretical modelling of these oscillations.
N.C. is supported by an EPSRC studentship. C.F. acknowledges financial support from the UK Science and Technology Facilities Council (STFC) on the CFSA Rolling Grant. The Nobeyama Radioheliograph is operated by the Nobeyama Solar Radio Observatory (NAOJ).
Berton, R., & Rayrole, J. 1985, A&A, 152, 219 [NASA ADS] [Google Scholar]
Chorley, N., Hnat, B., Nakariakov, V. M., Inglis, A. R., & Bakunina, I. A. 2010, A&A, 513, A27 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Druzhinin, S. A., Pevtsov, A. A., Levkovsky, V. L., & Nikonova, M. V. 1993, A&A, 277, 242 [NASA ADS] [Google Scholar]
Efremov, V. I., Parfinenko, L. D., & Solov'ev, A. A. 2009, Cosm. Res., 47, 279 [NASA ADS] [CrossRef] [Google Scholar]
Efremov, V. I., Parfinenko, L. D., & Solov'ev, A. A. 2010, Sol. Phys., 267, 279 [NASA ADS] [CrossRef] [Google Scholar]
Foullon, C., Verwichte, E., & Nakariakov, V. M. 2004, A&A, 427, L5 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Foullon, C., Verwichte, E., & Nakariakov, V. M. 2009, ApJ, 700, 1658 [NASA ADS] [CrossRef] [Google Scholar]
Gelfreikh, G. B., Grechnev, V., Kosugi, T., & Shibasaki, K. 1999, Sol. Phys., 185, 177 [NASA ADS] [CrossRef] [Google Scholar]
Gelfreikh, G. B., Nagovitsyn, Y. A., & Nagovitsyna, E. Y. 2006, PASJ, 58, 29 [NASA ADS] [Google Scholar]
Nagovitsyna, E. Y., & Nagovitsyn, Y. A. 2001, Ast. Lett., 27, 118 [Google Scholar]
Nakajima, H., Nishio, M., Enome, S., et al. 1994, IEEE Proc., 82, 705 [NASA ADS] [CrossRef] [Google Scholar]
Sainz Dalda, A., & Martínez Pillet, V. 2005, ApJ, 632, 1176 [NASA ADS] [CrossRef] [Google Scholar]
Scargle, J. D. 1982, ApJ, 263, 835 [NASA ADS] [CrossRef] [Google Scholar]
Shibasaki, K. 2001, ApJ, 550, 1113 [NASA ADS] [CrossRef] [Google Scholar]
Shibasaki, K., Enome, S., Nakajima, H., et al. 1994, PASJ, 46, L17 [NASA ADS] [Google Scholar]
Solov'ev, A. A., & Kirichek, E. A. 2008, Astrophys. Bull., 63, 169 [NASA ADS] [CrossRef] [Google Scholar]
Torrence, C., & Compo, G. P. 1998, Bull. Am. Meteorol. Soc., 79, 61 [Google Scholar]
Verwichte, E., Foullon, C., & Van Doorsselaere, T. 2010, ApJ, 717, 458 [NASA ADS] [CrossRef] [Google Scholar]
Vourlidas, A., Gray, D. E., & Shibasaki, K. 2006, PASJ, 58, 11 [NASA ADS] [CrossRef] [Google Scholar]
Zhang, J., Solanki, S. K., Woch, J., & Wang, J. 2007, A&A, 471, 1035 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Leakage of long-period oscillations from the chromosphere to the corona
Long-period oscillations of millimeter emission above sunspots
Long period oscillations in sunspots
Frequency drifts of 3-min oscillations in microwave and EUV emission above sunspots
Long quasi-periodic oscillations of sunspots and nearby magnetic structures


Coláiste na hInse hosted its Oíche Oscailte for incoming dáltaí at the end of September. Our dáltaí led tours on the night, as well as putting on displays of their work in Home Economics, Art, Science and many other subjects. Go raibh maith agaibh to all dáltaí who helped on the night, and to all future dáltaí and their tuismitheoirí who attended on the evening.


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Q: Using attributes to start function I have a function that uses a stopwatch instance and measure time of any method put inside. now, I have to start and stop that for every method. I want to so this now using attribute. I want to place just an attribute over every method which automatically starts and stops my function which measures the time.
The code of function:
 [DataContract]
[Serializable]

public class AppTrace:BaseModel<AppTrace>
{
    [DataMember]
    public string Comment;
    [DataMember]
    public string MethodName;
    [DataMember]
    public DateTime StartTimeStamp;
    [DataMember]
    public int Duration;
    [DataMember]
    public int UserObjectId;
    [DataMember]
    public string MachineName;
    [DataMember]
    public int ToolId;
    private System.Diagnostics.Stopwatch stpWatch;

public AppTrace(string comment,string methodName,int userObjectId ,string machineName = "",int? toolId=null)

    {
        MethodName = methodName;
        UserObjectId = userObjectId;
        StartTimeStamp = DateTime.UtcNow;
        Comment = comment;
        MachineName = machineName;

        stpWatch = new System.Diagnostics.Stopwatch();
        stpWatch.Start();
    }

    public AppTrace()
    {
    }

    public void CloseTrace()
    {
        this.stpWatch.Stop();
        Duration=Convert.ToInt32( this.stpWatch.ElapsedMilliseconds);
    }

A: That probably won't work with only the .NET Framework. Aspect oriented programming is implemented by various third party providers, Postsharp probably being the most used.
You can implement your own attributes, but without an AOP framework, they will not execute any code for you. They are just metadata that you can query with reflection.

A: Another way to solve this, would be something like :
protected void StopwatchThis(Action func)
        {
            //some code
            func.Invoke();
            //more code
        }

So if you are doing some optimization and want to test the run time, you could basicly just delegate your methods to this function and get the output.
question bit too broad


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A superpowered poet meets a conspiracy during the Summer of Love
Lauren Davis
Filed to:saturday webcomic
The year is 1967, and Banning James, a young poet with the ability to psychically inflict his own experiences onto others, thinks he's on his way to Boston. But his plans change when he gets caught up in an anti-Vietnam War protest, one that ends with an act of destruction that never occurred in our timeline.
Just Another Sheep is written by Mat Heagerty and drawn by JD Faith (and supported by a team that handles colors, flats, and letters). The webcomic opens with Banning on the bus to Boston as he's being threatened by a pair of toughs. Banning is a skinny, quiet kid with crappy vision, who writes poetry in his notebook and wears a peace sign on his bag. But he can hold his own in a fight thanks to his bizarre superpower: he can make anyone feel any physical sensation he's ever felt. He can make them feel as sick as he's ever felt, the pain from a broken arm, his greatest memories of euphoria. Threats in Banning's path tend to end up doubled over.
But Banning finds himself not in Boston, but in Washington, DC, where he gets caught up with a group of young protestors. With the promise of a ride to Boston and swept up in their cause (and fun), Banning joins their storming of the White House lawn, an endeavor that goes horribly wrong.
While the backdrop of Lyndon Johnson's America is a familiar one, Just Another Sheep isn't set in our timeline. It's an alternate history of the 1960s, one in which a shadowy secret society is looking to tug violently on the world's strings—a society that's well aware of Banning's powers. Banning James is about to embark on the classic 1960s roadtrip, but it's going to be across an American landscape that has been radically altered.
JD Faith also has a Kickstarter campaign running for another comic he penciled, VIRGIL, about a recently outed gay cop fighting across Jamaica to rescue his lover and get revenge on the people who wronged him.
[Just Another Sheep]


text:
CCTV America | Trending Sports & Global News > Blog > Sports > Ice hockey > Oilers, Coyotes Blues, Panthers, Kings
Oilers, Coyotes Blues, Panthers, Kings
Edmonton Oilers' Future Bright With 3 Top-Scoring Prospects
In today's NHL rumors rundown, there is talk that a coaching change could happen in Edmonton as early as next week. A few teams are now considered the front-runners to acquire Ben Chiarot, defenseman, ahead of the March 21 deadline. Rob Blake, GM of the Los Angeles Kings, and Jakob Chychrun from the Arizona Coyotes are discussing a contract extension.
Tippett Could be Fired in January 10.
According to Emily Kaplan, ESPNIf the Edmonton Oilers decide to make a coaching move, it could be on January 10, if they lose to the Oilers. Kaplan believes that the NHL would take a short break due to issues with attendance. This would allow the team to make a move, and for Ken Holland to introduce a new voice.
She says the team wouldn't go out and hire one of the big, available names on the market but would prefer to promote someone internally with Glen Gulutzan (assistant coach) or Jay Woodcroft (Bakersfield of the AHL) being the leading candidates. She adds, "But it's definitely an inflection point in Edmonton right now."
Leon Draisaitl, asked Leon Draisaitl whether Tippett was losing the Oilers locker-room. "We're not quitting on anyone," Draisaitl snapped him back. He added, "We're not quitting on our coach, we're not quitting on ourselves as players, our team, our goalies, nobody. We're not quitting."
Chychrun talks to Coyotes General Manager about Possible Trades
Bill Armstrong, Coyotes' General Manager, noted this during a spot @AZSportsHe has spoken out with Jakob Chychrun, defenseman, about potential trades. Armstrong confirmed the topic has come up a lot and that he's trying to be upfront and honest with Chychun and his agent about what options are out there. Armstrong said that he must do his job as a GM, and listen to all offers. Armstrong was added, "If there's something on the table that we can't refuse that's going to put this club in the right direction with some impact players, I certainly have to listen."
Arizona Coyotes defenseman Jakob Chychrun (AP Photo/Mark J. Terrill)
Sources like Darren Dreger have confirmed that insider reports still suggest that the Coyotes are looking for a huge return on Chychrun. The asking price is high and has scared some teams away, as Eichel's return is the comparison.
As for whether or not the team is open to trading defenseman Shayne Gostisbehere, Armstrong said the blueliner has garnered a lot of interest but that he's a big part of the Coyotes team and they aren't actively looking to deal him. "…he's been a big piece of our team, and he's got another year with us, too, so we're not that anxious at this point to move him."
Ben Chiarot: Blues and Panthers
According to Frank Seravalli from Daily FaceoffThe St. Louis Blues were among the teams that made the big moves towards Ben Chiarot, Montreal Canadiens. The Florida Panthers are also believed to have shown interest.
Seravalli believes Chiarot will be very popular this season, as the 30-year old defenseman can play a lot and provide a big help to a contending team. The NHL insider hinted that it won't be surprising if teams like the Vegas Golden Knights, Colorado Avalanche, Washington Capitals, or New York Rangers get involved.
Related: Red Wings Should Hold onto 3 Players beyond the 2022 Trade Deadline
Elliotte Friedman and Jeff Marek on The Jeff Marek Show noted that they have both heard Florida, St. Louis, and other states involved in this show. His 32 Thoughts column features these observations. Friedman also wrote, "After watching St. Louis dismantle Minnesota at the Winter Classic, I wonder if the Blues consider someone like Chiarot. It looks like a go-for-it year for them."
Kings and Blake Talking about Extension
As per The Fourth Period, GM of the Los Angeles Kings, Rob Blake confirmed to Dennis Bernstein and John Hoven during the "Kings of the Podcast" that he would like to stay on with the organization and that he a Luc Robitaille will work on an extension. Blake is now in the final year on his contract.
Rob Blake – Los Angeles Kings (Getty Images)
Uncertainty about his future with the team isn't going to stop Blake from making changes as this year's deadline. He noted, "I fully anticipate moves going forward will have impacts on the roster to make us better." As for who the Kings might be looking to move or what they'd like to add, that is still unclear.
Jim Parsons, a senior THW freelance journalist, part-time journalist, and audio/video host, lives, eats and sleeps NHL news and rumors while also writing features about the Edmonton Oilers. He's been a trusted source for five-plus years at The Hockey Writers, but more than that, he's on a mission to keep readers up to date with the latest NHL rumors and trade talk. Jim is a daily must for readers who want to be "in the know."
Additional content contributions include: NHLtradetalk.comThe Sportster, and host of weekly video casts. THW News and Rumors –, plus Oilers Overtime.
Follow these steps to submit content information or request interview questions. Jim on TwitterHis social media accounts. On articles such as this, they appear under his photograph.
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For a backup strategy to be reliable, it needs to be automatic. If the backup relies on a human to start the process, a point of failure exists. The backup should occur automatically every night. There are various backup software programs available, including the free backup program included in various Microsoft Windows versions.Having a good backup is extremely important to help recover from a hardware failure. The second way to protect against hardware failure is to have hardware redundancy.