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Search SA Votes - South Australian Election 2014
Unley Results
92.0% Counted. Updated 2014-03-23T15:29:04
ABC Prediction Liberal retain
2.2 swing to ALP
Labor Party 40.2
Lara Golding
Liberal Party 59.8
David Pisoni
Count After Preferences
Labor Lara Golding 8881 40.2 +2.2 +2.2
Liberal David Pisoni 13195 59.8 -2.2 -2.2
First Preference Count
Dignity Joanne Blesing 854 3.9 +3.9 +3.9
Greens Nikki Mortier 2481 11.2 -2.2 -2.2
Family First .... 0 0.0 -2.0 -2.0
Informal votes 409
Total votes 22485
Torrens | Waite
Adelaide Inner Southern Suburbs
Very Safe Liberal 12.0%
David Pisoni (Liberal) since 2006. Shadow Minister for Education, Families and Training.
Covers the inner southern suburbs of Adelaide immediately south of the CBD. It includes Unley, Hyde Park, Unley Park, Malvern, Parkside, Eastwood, Glenside, Frewville, Glenunga, Fullarton, Myrtle Bank, Highgate, and parts of Wayville, Goodwood, Millswood and Glen Osmond. (Map)
Gains parts of Goodwood and Wayville north of the Glenelg Tramway from Ashford. The Liberal margin falls slightly from 12.2% to an estimated 12.0%.
Unley was a Liberal electorate from its creation in 1938 until being won for Labor by former Australian wicketkeeper Gil Langley at the 1962 election. He was succeeded by Kym Mayes in 1982, a Minister in the Bannon and Arnold government's who lost his seat in the 1993 landslide.
Subsequent redistributions have shifted the seat back into the Liberal camp, Unley held by Mark Brindal from 1993 to 2006 when he was succeeded by David Pisoni.
The name of the electorate is derived from either the family name of the wife of Thomas Whistler who was an early land holder in Unley, or from the English town of Unley.
The 1973 election saw an unusual protest in Unley, when several local activists complained about the quality of candidates by nominating the improbably named Susie Creamcheese on behalf of the Happy Birthday Party. Creamcheese polled 6% of the vote.
Past Boundaries
The graph of past results below reveals that the political geography of Unley was changed by the 1998 redistribution, the boundaries of which were first used at the 2002 election. Areas to the west of Goodwood Road were removed, replaced by areas east of Fullarton Road. This shift eastward added around 5% to the Liberal margin in the electorate, widening the two-party preferred gap between Unley and the rest of the state, a gap that the graph shows has continued to this day.
2014 Ballot Paper (4 Candidates)
Candidate Name
BLESING, Joanne Dignity for Disability
GOLDING, Lara Australian Labor Party
MORTIER, Nikki The Greens
PISONI, David Liberal Party
Joanne Blesing
Dignity for Disability
47 year-old Blesing has lived with Multiple Sclerosis since 2004, her disease having progressed to near quadriplegia. Before her illness she was an architect, managing her own business and with 20 years of architectural design, project management, contract negotiations, and senior management corporate consulting.
Australian Labor Party
Golding has ten years experience teaching in both the private and public systems. She is currently teaching Year 12s and is the head of a Maths faculty. With a Masters Degree in Education, Golding also lectures in Mathematics Education at Adelaide University and volunteers at the Australian Education Union providing professional development in classroom management for new teachers. She won the Inspirational Secondary School Teacher of the year award in 2011 for the Western Adelaide region and in 2003 won a Prime Minster's Centenary Medal for her service to the community.
Nikki Mortier
Also contested this seat at the 2010 state election, neighbouring Adelaide in 2006, and was also on the Green Senate ticket for South Australia in 2007 and 2013.
After completing his apprenticeship, Pisoni started his own furniture manufacturing business and at the time of his election to Parliament in 2006 was Managing Director of his own retail and manufacturing business. He has served on the board of the Women's and Children's Hospital and as Chair of the Unley Primary School Council. In 2006 he defeated high profile journalist and Liberal ministerial adviser Chris Kenny for pre-selection. Pisoni is currently Opposition spokesman on Education, Families and Training as well as Multicultural Affairs
2010 Result
MORTIER, Nikki GRN 2,711 13.2 +3.6
PISONI, David LIB 11,691 56.8 +10.4
VARTTO, Vanessa ALP 5,774 28.1 -8.5
SMOLUCHA, Luke FFP 396 1.9 -0.7
.... DEM 0 0.0 -3.2
.... D4D 0 0.0 -1.7
After Preferences
VARTTO, Vanessa ALP 7,768 37.8 -10.3
2010 Result (Post-redistribution)
Primary %
2CP %
Labor Party ALP 28.2 38.0
Liberal Party LIB 56.4 62.0
Greens GRN 13.4
Family First FFP 2.0
SA Live Election Results
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I've been spending all my "free" time (of which there is very little) working on the restructuring plan for NYC Shiba Rescue and recruiting volunteers to fill the new positions. Snick and I manage to post tidbits on twitter and facebook occasionally, but finding time to write a whole blog post has been difficult.
That got me thinking long and hard about humane education, how important it is, and how no formal, organized plan to teach our children empathy towards animals really exists. An idea popped into my head and I've been formulating a plan. I plan to start a new, national, non-profit organization to promote and support humane education – specifically to teach compassion and empathy for companion animals – in the public school systems across the US.
I'm considering naming it Animal Educators Alliance. I know it sort of sounds like people who educate animals though, so I'm not entirely sure. It means animals who ARE educators. We're not just teaching about companion animals. The animals ARE the teachers. What do you guys think? Good? Bad? Have any better ideas?
To create and distribute a standard curriculum to be used by schools and volunteers throughout the country.
To provide guidelines for volunteers and their animals.
To bridge the gap between schools and volunteers.
To eventually provide training and certification for various levels of volunteers.
Ambitious? Well, yeah. Impossible? I don't think so.
If you start this, it would help so many shelters and rescues, because, as you've found out, they probably don't have the time, the people or the means to do this themselves.
You know you would definitely have mine and Sushi's support!!
I'm not sure what help I would be, but Koji and I are all for it, and I'm sure I have a few friends I could pull in for the greater good.
My first reaction is that it strikes me as weird that there is an identified need to teach kids to be nice to animals. It seems that would go without saying.
My second reaction is that like most programs that try to make kids into better people, it's targeted at the wrong people entirely. It's the parents that should be re-educated, not the kids. Then they'd teach their kids right. Everything I've taught my girls in youth group, they do it great at group, and then they go home and behave exactly as their parents behave. Sad.
My third reaction would be that teaching compassion wouldn't be as useful as teaching kids to understand their pets' thinking, instead of treating them like toys. Cesar Millan for kids.
However, I also think you have to do what you feel called to, and if this is what you feel is needed from you, go for it. It can't hurt, anyway.
Hope – I like that! I have to take AWE into serious consideration as a name.
Mongoose – You are SO right. Like so many other things, this should be taught in the home, not the schools. But, as I'm sure you also know, that isn't going to happen in a lot of homes. What I've found with school visits is that by exposing children to animals they can form a connection with, we're setting them up to think twice before abusing or abandoning an animal. I'm talking mostly about reaching kids who are afraid of animals, many of whom are being taught that in their homes and neighborhoods. It rocks these kids' worlds when you say your dog lives in the house and sleeps on the bed with you. The idea of an animal as a friend – an unconditionally loving friend, at that – is completely foreign to them.
Thank you ALL for your input. This is exactly the kind of stuff I need to think about and figure out before diving into this thing.
what a great idea. It is so desperately needed. I live in Europe now and it is no different here. Education is lacking but as Moongoose correctly spells it out, it is the parents that need to be re-educated. We had two dogs and I always made sure to teach my son that our dogs are indivuals with their own feelings, and just like us humans like to be treated kind and with respect – so DO our dogs too. It would great to see your organisation expand internationally. Not sure how I could help from overseas but we are here for you and ready to help.
Hope – "AWE" is AWEsome. I totally love the name.
We love reading the latest news from Snick…keep em coming.
Thank you Doris! 🙂 I'm sure there will be ways you can help long distance!
I've decided the name Animals Who Educate is definitely AWEsome and I'm planning to use it. 🙂 I hope everyone will stay interested in helping out during the time it takes me to actually get something off the ground. Finding time to work on it is proving very difficult!


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What should I bring for my Backpacking Trip?
Unlike guided tours, Backpacking is all about simplicity, mobility and impulsive. In that case, why should we bother to take so much? So, take only the essential items. Backpackers are keen to explore in depth, mingle with the locals and … Continue reading What should I bring for my Backpacking Trip?
Health Supplements – Are They Necessary?
"If possible, I wish to avoid taking capsules like you all" "We are still young. We do not need to take these health supplement" "You aren't sick, why do u need to take these pills?" Do you realize that, these … Continue reading Health Supplements – Are They Necessary?


Today we start with bugs in PHP's Date/Time extension. There are a fair amount of them and they require some hard needed attention. So this post addresses a number of bugs.
 => string(47) "The timezone could not be found in the database"
Which mentions very clearly  => string(47) "The timezone could not be found in the database" — the key 13 is the position in the original string.
However, there was a bug that needed a fix. Bug #53879, "DateTime::createFromFormat() fails to parse cookie expiration date" talks about parsing a date string such as Mon, 21-Jan-2041 15:24:52 GMT with the factory method DateTime::createFromFormat(). This method takes as first argument a series of format specifiers to signal how the date string should be parsed. It mostly uses the same format letters that the DateTime::format() method uses to output a DateTime object in a specific format.
In this case, the user did not specify his own format, but used one of the predefined constants that is meant for displaying a DateTime object in a format that HTTP Cookies want. The constant DateTime::COOKIE was in fact just the string l, d-M-y H:i:s T. The y here stands for a two-digit year. Specifying the year in two digits appeared in the original RFC 850 but has since then be superseded by a whole bunch of interconnecting and contradicting standards.
In PHP, Wdy, DD-Mon-YYYY HH:MM:SS GMT is represented as l, d-M-Y H:i:s T to which I now changed PHP's DateTime::COOKIE constant.
There are plenty more issues, so we'll be coming back to the DateTime extension.


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Sydney and Canberra likely to host India's limited-over series against Australia: Reports
Australia's Sydney could be Indian cricket team's port of entry for quarantine and training during India's upcoming tour Down Under next month, pending government approval.
Sydney and Canberra likely to host India's limited-over series against Australia. | &nbspPhoto Credit:&nbspIANS
Sydney and Canberra are emerging as options to host India during the upcoming tour next month
Once this gets the government approval, the CA will send the agreement for review to BCCI
Sydney could be finalised as the port of entry for quarantine and training for Team India
Sydney and Canberra are emerging as potential venues to host India's limited-over series against Australia during the upcoming tour starting next month. The Indian team was initially supposed to land in Brisbane but apparently, Queensland state health authorities won't allow the visitors to train during the mandatory 14-day quarantine period.
According to a report in ESPNCricinfo, Sydney could emerge as Indian contingent's port of entry and the city may allow them to train during their quarantine.
It is learnt that the SCG could be hosting four of the six white-ball games (three T20 Internationals and three ODIs) while Canberra's Manuka Oval hosting two games.
New South Wales state's sports minister Stuart Ayres confirmed that they have received a request from Cricket Australia to allow the Indian as well as the Australian team to undergo its mandatory quarantine as well as training.
"Cricket Australia has approached the New South Wales government about quarantining the Indian cricket team and returning Australian cricketers in Sydney," Ayres was quoted as saying by the cricket website.
"That proposal is currently being assessed by NSW authorities including health and police. Fixtures for the Indian tour will be determined by Cricket Australia and won't impact our assessment of the quarantine proposal."
If CA and the NSW state government are able to reach an agreement, a revised plan would then be submitted by Cricket Australia to the BCCI for approval.
ICC demands action in the Sydney racial abuse incident; Cricket Australia to respond
BCCI formally writes to Cricket Australia for quarantine relaxations In Brisbane
Ajinkya Rahane briefs on India-Australia test series, says India performed well despite the hurdles

redpajama_set_name: RedPajamaCommonCrawl


A MEDIA campaign by the QT supporting a mother's eight-year crusade for justice has opened the door to a public inquest into the death of her baby at Ipswich Hospital.
State Coroner Terry Ryan has agreed to review the case following a request from Leichhardt mum Rachelle Lind last month for an inquest into the death of her daughter Caitlin Porter in May, 2007.
It took five years for the State Coroner to hand down its report into the death. The investigation did not progress until the file was transferred from Ipswich to the Brisbane Office of the State Coroner two years after the death.
Records were obtained from Ipswich and two reports from independent specialist doctors were sought as part of the inquiry.
Ipswich Hospital failed to conduct a Root Cause Analysis on the death until late last year when Mrs Lind raised the matter with the Health Ombudsman and The Queensland Times.
The baby was born in poor condition due to the chord being wrapped around her neck. Routine tests in the first five minutes showed Caitlin's initial resuscitation was not effective.
The extent and impact of bleeding at the back of the head was not appreciated as bruising is common after vacuum-assisted deliveries. This combined with a lack of regular monitoring, meant that the circulatory collapse was not acted on in a timely fashion.
There was a delay in appreciating that this baby was not progressing well and a delay in escalating concerns. A lack of structured escalation between medical officers contributed to unclear resuscitation and associated diagnostic tests to confirm baby status.
Due to inexperience in neonatal resuscitation and lack of direct supervision, a tube into the windpipe was incorrectly placed, the baby did not receive sufficient oxygen during resuscitation and developed asphyxia.
The incorrect positioning of the tube was not diagnosed in a timely fashion, partly due to the lack of a new piece of equipment (Pedi-cap) which measures the adequacy of respiration.
Despite the Coroner referring the doctor to the Australian Health Practitioner Regulation Agency (AHPRA) for consideration of disciplinary action in September, 2012, the agency has not been able to shed any light on the investigation.
The doctor is still registered by AHPRA and practising in Ipswich.
Requests for information on the outcome of the investigation have been refused by AHPRA..
Mrs Lind said she would pursue her case until those involved were held accountable.
"People say how do you keep going. I have my moments but I have to stay strong and keep on fighting for my daughter," she said.
"Something has to be done so that this doesn't happen again."


Chef Jim Davis shows us how to use a bread knife to cut a loaf of bread.
Jim Davis: Hi! Jim Davis here for Harris Teeter. I am going to show you now how to use a bread knife. One of the most important things in selecting a bread knife is to select one that has scalloped sharp edges on it. You don't want a knife that's going to tear the bread but one is going to slice it evenly.
This is also called roast slicer; it can also be referred to it as a tomato slicer because it will do all of those jobs equally well but it's great for bread. I like to cut my bread at a slide angle so taking the knife I went down through the bread once or twice, slide it back. Oh! that's nice bread.
I use it to cut my bread about three-quarter of an inch thick. The thing you want to do is make sure that you cut the bread at the same thickness all the way down so we've got one there that's pretty thick here is one is fairly thin. Now, if I've done my job fairly right, see it's about the same thickness top and bottom all the way through.
If you are going to slice for sandwiches somewhere in between there, like that and then two slices and there you have it. That is how you use a bread slicer. Up next, I am going to show you how to use a Santoku.


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U.S. Attorney's Office
Western District of Pennsylvania
Scott W. Brady
, United States Attorney
www.justice.gov/usao-wdpa
Cleveland Brothers Indicted on Robbery and Gun Charges
PITTSBURGH - Two siblings from Cleveland, Ohio, have been indicted by a federal grand jury in Pittsburgh on charges of violating federal robbery and firearms laws, United States Attorney Scott W. Brady announced today.
The seven-count indictment, returned on October 16, named the defendants as Rayshawn Patterson, 19, and Reginald Patterson, 21, both formerly of 12305 Rexford Avenue, Cleveland, Ohio 44105.
According to the indictment, on December 23, 2017, Rayshawn Patterson and Reginald Patterson conspired to commit and committed a theft of a licensed firearms dealer, DSD Sports, located at 328 B. West Main Street, Brookville, PA 15825, stealing 14 pistols and two assault rifles. On that same date, Rayshawn Patterson and Reginald Patterson are charged with transporting the stolen firearms in interstate commerce. On the previous day, Rayshawn and Reginald Patterson are also charged with conspiring to commit and committing a Hobbs Act Robbery at Fastway Gas, located at 22352 Route 68, Clarion, PA 16214, stealing an amount of United States Currency. In the robbery of Fastway Gas, they are charged with using, carrying, and brandishing a firearm during and in relation to a crime of violence. Finally, from December 23, 2017 to December 29, 2017, they are charged with possession of the stolen guns from the robbery of DSD Sports.
The defendants face a total maximum sentence of not less than seven years and up to life in prison, a fine of not more than $250,000, or both. Under the Federal Sentencing Guidelines, the actual sentence imposed would be based upon the seriousness of the offenses and the prior criminal history, if any, of the defendants.
Assistant United States Attorney Timothy M. Lanni is prosecuting this case on behalf of the government. The Bureau of Alcohol, Tobacco, Firearms, and Explosives, the Brookville Police Department, the Pennsylvania State Police, the Cleveland Police Department, and the Cuyahoga Sheriff's Department conducted the investigation leading to the indictment in this case.
This case was brought as part of Project Safe Neighborhoods (PSN), a program that has been historically successful in bringing together all levels of law enforcement to reduce violent crime and make our neighborhoods safer for everyone. Attorney General Jeff Sessions has made turning the tide of rising violent crime in America a top priority. In October 2017, as part of a series of actions to address this crime trend, Attorney General Sessions announced the reinvigoration of PSN and directed all U.S. Attorney's Offices to develop a district crime reduction strategy that incorporates the lessons learned since PSN launched in 2001.
An indictment is an accusation. A defendant is presumed innocent unless and until proven guilty.
Philadelphia Field Division


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Abigails letter to John Adams, 14 August 1776, "We should have learned women". Click the winner in the bracket below to read more about the letter and view images and transcriptions.
Voting ends on March 31, the anniversary of her famous "Remember the Ladies" letter. The winner will be announced on April 1.
For the first round of voting, we grouped the letters into 8 categories: Education & Learning; Parenting & Family; Things Abigail Valued; Friends & Frenemies; Politics & Public Life; War; The World According to Abigail; and Women.
Are you wondering why Abigail's March 31, 1776 letter to her husband John urging him to "Remember the Ladies" is not a part of the competition? It won the MHS Madness bracket in 2016 so we did not include it in this competition.
Discuss! Is your favorite letter amongst the 32 in the bracket? Which letter are you rooting for? Are you just learning about Abigail Adams now or have you been a fan of hers for a long time? Let us know on social media using the hashtag #RememberAbigail.


Do a little digging, and you learn the quickest and most sure-footed path to making a million dollars or more is by finding an online niche — preferably one that actually excites you at your core — and discovering what the people in that niche want.
Too many people do the opposite — they focus on the hottest product or service and try to blast that out to as many people as possible. There's an inherent risk in being left holding a bag of goodies nobody wants. And that's one expensive bag!
Just like the old-fashioned way, you're not buying tons of inventory and then hoping that you sell it. You get the orders and the money first; then you deliver. Online, you learn your market's want or gap in fulfillment, and then you deliver a product or service that the market wants. Social media is a great way to learn more about your market (and pull in very qualified leads!) once you've established what your niche will be and build your website around it.
Making millions online starts by installing the critical Millionaire Blueprint in your mind.
As usual, proceed with caution. Not everything can be sold online. Not every want that might be clear and evident can be fulfilled just by throwing up a website.
The late Cory Rudl, one of the pioneers of Internet marketing and online businesses, used this analogy. If you had a cure for the common cold, in an easy-to-digest pill form, "billionaire" might not even apply to what you'd be worth. That product would be everywhere — 7-Eleven, every grocery store, corner store, market, you name it.
Now try selling those pills online. At minimum it takes at least three to four days for the product to get to you. You're already over your cold by then. It's a failure from day one. Don't start with a product. Start with a market, and then find a product that the market wants.
People spend money on things they want. It's an emotional investment. A necessity can be satisfied by the most convenient and cheapest product or service. People are willing to pay more money for wants, but they're usually very price-conscious with things they have to get or do.
And no different from traditional businesses, there's the backend after that want is fulfilled. It's the product or service you sell after they've bought the first product from you. That's where all the money is.
Been to the movies lately? If not, no one can blame you as expensive as it can be to take your family out for movie night. But just think about all the money being made at the concession stand alone.
Even fast-food workers are routinely taught to upsell. It's no different online — the point is, your customers come in for one thing and walk away with more — because you gave them something they wanted from the beginning.
Once you have the customer's name online, it costs you nothing to sell to that person again and again and again. You can make 100% more net income than you are right now by backend selling.
to gain more customers than you can even handle.
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To know the importance of having a website for your business is one thing. Knowing the purpose behind having a Web presence is a whole other level.
If your business is already up and running, you'll have to cater your strategies to what you already have in place, particularly in terms of your pre-existing customer base. That means getting them to fill out cards in your physical business, or otherwise enticing them to your website with special offers. Then follow-up emails. We're still talking basic marketing and backend selling — making money on those who are the easiest to sell to: those you've sold to before.
But if you're still unsure of what kind of business you'd like to create, take a good, long look at creating an online business.
The easiest way to make money online is to focus on a specific market, find a product that they want, and give it to them. Searching for your best prospects online isn't that much different from doing so offline.
How do you do this? The same way you look for anything else online: surf. Simply search on Google — for example, maybe you have a passion for scuba diving that you'd like to turn into a business. You find all the news groups, forums, and websites regarding scuba diving. Is there anything they're talking about a lot? Any patterns where something is wanted but not easy to find?
That's how you find your target market. It may take you a day, a week, a month, maybe longer. It depends on what your market is and what you're trying to find, but whatever the niche, there's a large enough market that's relatively easy to get to. You know where they are, and after some research, you'll know that they want something specifically. All the gamers are hanging out in one market. All the sports nuts are hanging out in one market. All the people who are interested in holistic medicine are hanging out in one market. All the doctors are hanging out in one market. It's easier to reach people than you might think.
Just try to reach those people through the local newspaper. If 20,000 people view your ad (theoretically), you'd be doing great to get 10 of them to show interest. Online, you can go right to where all of your target market hangs out. Your target market is sitting right in front of you.
There are tons of people who know enough about the money-making potential of the Internet and ask, "So what do I sell online? What's going to be a hot seller?" It's the most common and most fatal mistake.
You never decide on the product. You find an easy, targetable market, find out what they want, and give it to them. It's the easiest method in the world. You have an instantaneously successful business. It is a no-brainer. It doesn't take any smarts to figure that out.
Anybody out there discovered the power of doing business online recently (I know you're there)? What did you find frustrating, or powerful, or even profound? Did you incorporate a Web presence into an existing business? What have been your most important takeaways?
It's a virtual road trip toward business success, the final destination — whatever your next venture will be, because you're done with that last one. It's running on its own, without you.
Until then, cruise control helps. Without cruise control, long road trips would be more tiring for the driver and, for those of us with a lead foot, a lot more speeding tickets.
All you need is a dashboard that has the exact readouts you need to control your business. You choose your top five to 10 critical success factors and come up with a system for how you're going to measure them. If you can't think of five, choose that top factor.
If you're measuring lead generation, for example, how many leads are coming in? You gauge leads per week and per month, at least. Now dig deeper. How many leads from each lead source? How much does each lead cost per source? Is one source cheaper and bringing more return than another? When you have benchmarks — like how much you're willing to pay for each lead — you've got numbers right in front of you that tell you how many leads come in and what you pay for them. What do you have?
You have control over your business.
Consistency, predictability, tracking — systems that can be operated and understood by practically anyone. When you can duplicate these systems, you're on cruise control.
Create a lean, efficient, and profitable business system. Almost automatically.
Now take 15 of the most important things you want to track. It might be lead generation. It might be customer satisfaction. It might be cash-flow management. If you have a business with labor, labor productivity is a good thing to measure. And then the question you want to ask is what's going to enable you to measure whether or not you are being successful at that?
All you do is establish a handful of gauges, tools, or metrics — whatever you want to call them — for whether or not you're executing that critical factor properly.
Then test them to make sure they work. Test them backward and forward. You want to make sure you can get to the benchmarks you set from the steps in your system. The good news about systems is they don't require that much training. A good system is one that you can put in someone's hands and the person knows how to use it.
It can be a simple narrative to describe — for people who like words — how this system works. You do flow charts for people who are the linear and visual thinkers in your business. It's as simple as a checklist. Someone else could operate it because all the person needs to do is go down the list: I did this, check; I did this, check. If you do every step on your checklist, at the end, you've got a system. That simple!
Please understand it's not that easy. There's work required to put systems into practice. Not torturous work; it can be a lot of fun as you refine them. Intuition and creativity can play into this thing, from the artist to the architect. You are the person qualified because you know it inside out. You know all the parts of it. You know what's involved.
Your business is you, and you are in control!
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Medina's testimony to detectives details what became alarmingly clear after the shooting: School officials long knew about Cruz's bouts of rage, obsession with weapons and Nazi imagery and violent outbursts against fellow students. Cruz was also assigned to a controversial program that diverts troubled students to alternative schools over the criminal-justice system — critics contend the program encourages a culture of lax discipline. The Broward County School District says he never showed up for those classes.
Breaking his silence this week, Peterson insisted he was not sure the gunfire was coming from inside the building — and even shifted the blame toward Medina for not giving him enough details about the shooter. That claim also seems to conflict with Medina's interview with detectives on the day of the shooting.


"Hey Looney Clooney Your lawyer wife should have taught you not to make statements without full facts", she Tweeted.
Clooney, 57, addressed the rumours he's going to be the royal baby's godfather. The former actress pulled her hair back in a classy low bun. The great thing is to encourage them.
Five unnamed friends of the duchess spoke to People in an effort to counter the "global bullying" directed at her. Making them even busier, of course, is their baby who's due to join the royal fold around the end of March or early April.
This is in direct contradiction to what her father, Thomas Markle, has always claimed - that Meghan has shut him out of her life. Her estranged half-sister Samantha Markle is once again on the warpath, and this time the Oceans 11 hunk is her number one target.
Witt worked for the Air Force and was a counterintelligence agent for 11 years where she had top-security clearance . But later that year, she helped an unnamed Iranian-American official produce an anti-American propaganda film.


text:
Sportsbook > NBA > Sacramento Kings vs Brooklyn Nets 11/22/2019 Odds Picks and Previews
Sacramento Kings vs Brooklyn Nets 11/22/2019 Odds Picks and Previews
Sacramento Kings vs Brooklyn Nets 11/22/2019 – The Sacramento Kings (6-7) will aim for a critical win on Friday against the Brooklyn Nets (6-8), who are set to miss superstar point guard Kyrie Irving for the fourth consecutive game. The Nets will be 3.5 points NBA Moneyline favorites in the game, but no one now is sleeping on the Kings after their big back-to-back wins against the Boston Celtics and the Phoenix Suns.
Sacramento Kings vs Brooklyn Nets 11/22/2019
November 22, 2019 7:30 PM ET
Barclays Center, Brooklyn, New York
Friday Night Hoopin' 🌃
🆚 | Sacramento
📍 | @barclayscenter
🕢 | 7:30PM ET
📺 | @YESNetwork
📻 | @WFAN660#WeGoHard pic.twitter.com/vjXbW1GO8V
Sacramento Kings vs Brooklyn Nets 11/22/2019 Betting Odds
Sacramento Kings +3.5 (-110) 216 o (-110) +129
Brooklyn Nets -3.5 (-110) 216 u (-110) -159
Sacramento Kings Betting
The Sacramento Kings have won four of their last five games and six of their last eight to move one game below .500. A win against the Nets at the Barclays Center will not only level their record to 7-7, but it could also very well be the breakthrough moment for the Kings this season as they wait for the return of point guard De'Aaron Fox and power forward Marvin Bagley III.
Tweets by SacramentoKings
Players to Watch: Buddy Hield (19.3 PPG, 4.8 RPG, 1.8 APG), De'Aaron Fox (18.2 PPG, 4.0 RPG, 7.0 APG), Bogdan Bogdanovic (14.9 PPG, 2.8 RPG, 4.8 APG)
The Brooklyn Nets sport a 2-1 record ever since Kyrie Irving sat with an injured shoulder. Spencer Dinwiddie, who has been the go-to-guy for the Nets during this stretch, recorded 20 points with 8 assists in Wednesday's 101-91 win over the Charlotte Hornets. Jarrett Allen also provided a much-needed offensive boost, finishing with a career-high 22 points and 17 rebounds in the game. On the bad side, Brooklyn just shot 40 percent from the field and 25.6 percent from beyond the three-point line.
Players to Watch: Kyrie Irving (28.5 PPG, 5.4 RPG, 7.2 APG), Spencer Dinwiddie (18.6 PPG, 2.5 RPG, 5.1 APG), Taurean Prince (13.1 PPG, 6.3 RPG, 1.5 APG)
Sacramento Kings vs Brooklyn Nets 11/22/2019 Betting Numbers
Sacramento are 8-0 ATS in their last 8 games.
Kings are 4-1 SU in their last 5 games.
Sacramento are 4-11 ATS in their last 15 games against Brooklyn.
Sacramento are 6-12 SU in their last 18 games against Brooklyn.
Kings are 4-1 ATS in their last 5 games on the road.
Sacramento are 2-8 ATS in their last 10 games when playing on the road against Brooklyn.
Sacramento are 6-2 SU in their last 8 games this season.
Kings are 4-2 SU in their last 6 games against an opponent in the Eastern conference.
The total has gone UNDER in 15 of Sacramento's last 20 games against an opponent in the Atlantic division.
The total has gone OVER in 7 of Brooklyn's last 10 games against Sacramento.
The total has gone UNDER in 11 of Brooklyn's last 16 games at home.
Brooklyn are 8-2 ATS in their last 10 games when playing at home against Sacramento.
Brooklyn are 2-4 SU in their last 6 games this season.
The total has gone OVER in 8 of Brooklyn's last 12 games against an opponent in the Western conference.
Brooklyn are 4-1 ATS in their last 5 games against an opponent in the Pacific division.
Brooklyn are 5-10 SU in their last 15 games played in November.
De'Aaron Fox PG Ankle is out indefinitely
Bogdan Bogdanovic SG Leg left last game, is "?" Friday vs Brooklyn
Marvin Bagley III PF Thumb is OUT 4-6 weeks
Kyrie Irving PG Shoulder is OUT Friday vs Sacramento
40-41 Straight Up 42-44
78.52 Defensive FT% 79.38
35.73 Defensive 3PT% 35.93
Sacramento Kings vs Brooklyn Nets Betting Picks
Analysis: The Kings are thriving even without two of their starters, and it all starts with their defense. Sacramento stepped up their D during this stretch, holding three of their last four opponents under 100 points. The Nets, meanwhile, aren't the same explosive team with Kyrie Irving on the floor as they averaged just 101 points over the last three games.
Moneyline: The Nets are 2-1 against the Kings in their last three meetings and also 4-3 at the Barclays Center this season. Unfortunately, Sacramento appears to be the wiser NBA bet based on their current form.
ATS: The Kings are on an 8-game ATS winning streak and could extend it to 9 games with a SU win in Brooklyn.
TOTALs: The total for this game will go UNDER 222 points. Again, the Nets aren't the same excellent offensive team they were when they had Kyrie Irving on the floor. The Kings, meanwhile, have been trying to slow down the pace, which has boded well in their favor.
Score Prediction: 110-105 Kings


All honours, graduates and graduate students are invited to be members of the Senior Common Room of Newman College. The College has around eighty students who are in residence who are engaged in graduate or postgraduate studies.
Some of these students are involved in providing tutorials in the College's tutorial programme.
Most of the members of the SCR act as a mentor to a first-year undergraduate.
All members of the SCR receive a scholarship and may remain in residence for the full calendar year.
The SCR has an executive made up of the President, the Vice President, the Secretary and the Treasurer.
There are a number of committees within the SCR (Sustainability, Academic, Community Service, Social, Music, Publications, Art and Literature). Many of these committees operate jointly with NCSC committees.


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text:
\section{Introduction}

Solar Energetic Particles (SEPs) are commonly measured near 1 AU in the interplanetary medium,
in most cases at large distances from the region where they were accelerated, in
solar flares and Coronal Mass Ejection (CME) driven shocks.
Understanding their propagation through space is important to gain information
about the acceleration processes and to test theories of
charged particle transport in turbulent magnetic fields, relevant to
a variety of astrophysical environments.
Since SEPs are a radiation hazard for satellite infrastructure and
humans in space, accurate modelling of their propagation is important also to develop
a Space Weather forecasting capability.

During their motion through interplanetary space, SEPs
undergo changes in their kinetic energy.
At the present time, a well established framework for the description of kinetic energy change of
SEPs exists, based on the theory of adiabatic deceleration within a transport equation, initially developed to
describe galactic cosmic rays.
In its classic description, adiabatic deceleration results from the cooling of an
isotropic energetic
particle gas as it moves outwards in the expanding solar wind \citep{Par1965}.
\cite{Ski1971} derived a focussed transport equation including adiabatic deceleration for the case when
the plasma convection velocity is at an angle with respect to the magnetic field, retaining pitch-angle as a variable.
\cite{Ruf1995} obtained an alternative formulation for a Parker spiral
geometry, again considering
particles of arbitrary pitch-angle.
Both approaches use a deceleration term within a transport equation.
The terms derived by \cite{Ski1971} and \cite{Ruf1995} are equivalent for a
Parker spiral magnetic field.

The majority of modern models of
SEP propagation include adiabatic deceleration by using either the
\cite{Ruf1995} or the \cite{Ski1971} formalism
within the focussed transport equation  [e.g.~\cite{Lar1998,Agu2008,Zha2009,Dro2010,Mas2012,Wan2012}].
Numerical solution of this equation shows
that adiabatic deceleration needs to be taken into account when
studying SEP propagation, as it
affects the decay phase of events
significantly for proton energies up to about 20 MeV \citep{Ruf1995}.
Intensity profiles are affected in a complex way that varies in the
different stages of the event \citep{Koc1998}.
\cite{Mas2012} modelled the transport of heavy ions and showed that the effects of adiabatic cooling
are very strong below 1 MeV nucleon$^{-1}$.
They pointed out that, as a result of deceleration,
particles measured within a given energy channel of a detector located at 1 AU may have
had a much higher energy when originally injected at the Sun.

The standard focussed transport approaches \citep{Ski1971, Ruf1995} assume that energetic particles remain tied to magnetic
field lines during their propagation, so that only a single spatial variable, the
distance travelled along a magnetic field line, needs to be retained to describe the particle's trajectory.
This is a common assumption in many studies involving SEP modelling and data analysis.

However in two recent publications we pointed out that drifts due to the gradient and curvature
of the Parker spiral magnetic field are important for SEPs \citep{Mar2013, Dal2013}.
This result is based on full orbit test particle simulations of SEPs in a Parker spiral configuration (\cite{Mar2013}, Paper I) as well as on analytical expressions for the particle drifts (\cite{Dal2013}, Paper II).
As a result of drift, particles experience transport in longitude and latitude, perpendicular to the magnetic field line on which they were originally injected.
The scattering conditions, described by a mean free path $\lambda$, do not strongly affect the amount of drift experienced. In fact, significant
curvature drift is found to be present even when particles propagate scatter-free.

In this paper we examine an important consequence of drifts for SEPs: the strong
particle deceleration due to drift motion in the direction opposite to that of the solar wind electric field, studied here for the case of protons. The electric field is present in the fixed (observer) frame due to the outward propagation of the solar wind plasma. Drift-induced deceleration has been studied  previously
in the context of galactic cosmic rays \citep{Kot1979, Bar1975}, but has not been discussed for SEPs up
to the present time.
We show that, unlike adiabatic deceleration, drift-induced deceleration is present also in the absence of scattering. We evaluate whether the standard focussed transport equation formalisms  \citep{Ski1971, Ruf1995}
describe the effects of drift-induced deceleration on the particle distribution function.

\section{Energy change for SEPs as derived from test particle simulations}\label{sec.test_simul}

In Paper I, the propagation of SEPs in a Parker spiral configuration in the presence of
scattering was studied by means of a relativistic full orbit test particle code.
The output of the simulations showed that, rather than remaining confined within the magnetic
field lines delimiting the injection region at the Sun, particles experience significant
drift (see e.g. Figures 3 and 5 of Paper I).
The amount of drift, measured in a local Parker spiral coordinate system
as the displacement
from the magnetic field line through the initial position,
increases with energy, i.e.~it is much larger for 100 MeV
than for 1 MeV  protons. It is particularly large for partially ionised
heavy ions due to proportionality of grad B and curvature drift velocities to the charge to mass
ratio.

Here we examine the results of simulations similar to those presented in Paper I,
focussing on the change in kinetic energy experienced by the particles during their
propagation.
We follow four initially monoenergetic populations, each consisting of 1000 protons, characterised by values of the initial kinetic energy $K_0$ of 1 MeV, 10 MeV, 100 MeV and 1 GeV.
The particles are injected from an 8$^{\circ}$$\times$8$^{\circ}$ region at 1 solar radius and
centered at latitude $\delta$=20$^{\circ}$. Their initial velocity directions are randomly chosen in a semi-hemisphere in velocity space pointing away from the Sun.
Particles are scattered with an average frequency defined by a scattering mean free path $\lambda$. During each scattering event the particle's velocity is
randomly reassigned from an isotropic distribution. Particles are scattered in the solar wind frame
and in this frame energy is assumed to be conserved during a scattering event.  This is a reasonable approximation since the majority of scattering events in our simulations take place far from the Sun. For comparison, scatter-free runs are also performed. Other parameters of the simulations have been described in Paper I.

The Parker spiral magnetic field used in the simulations is unipolar (pointing outwards from the Sun, as was assumed in the simulations of Paper I), i.e.~the
presence of the heliospheric current sheet is not modelled.
The Lorentz equation of motion for each particle is solved
in the fixed frame, in which the Sun is rotating
with angular velocity $\Omega$ and the solar wind is moving radially outward at constant speed $v_{sw}$. This
is the frame which is relevant for comparison of simulation results with observations
taken by spacecraft.

Figure \ref{fig.kinenergy_perc_change} shows the kinetic energy change experienced by particles of the four initially monoenergetic populations (one for each panel, with initial energy $K_0$ as labelled) at time $t_f$=102 hours, plotted as a function of the change  in colatitude experienced by each particle.
The mean free path is $\lambda$=1 AU at all energies.
Kinetic energy change $\Delta K$=$K$$-$$K_0$ is shown as percentage of the initial energy $K_0$, as a function of $\Delta \theta$=$\theta$$-$$\theta_0$ where $\theta$ is the particle's colatitude and $\theta_0$ its initial value. Particles in all four populations are seen to have experienced strong deceleration over the time of the simulation, apart from a minority of those with $K_0$=1 GeV, whose kinetic energy increases.

\begin{figure}
\epsscale{.80}
\plotone{dalla_fig1.ps}
\caption{Percentage change in kinetic energy as a function of colatitude change $\Delta \theta$, four days after injection, for protons of four initially monoenergetic populations with initial energy $K_0$ indicated in each panel. Particles are injected from an 8$^{\circ}$$\times$8$^{\circ}$ region at latitude $\delta$=20$^{\circ}$ and the mean free path is $\lambda$=1 AU.\label{fig.kinenergy_perc_change}}
\end{figure}

It should be noted that the scale on the $x$-axes of the panels of Figure \ref{fig.kinenergy_perc_change} is different for the four populations, showing that the 1 MeV particles have
a much smaller $\Delta \theta$ compared to 1 GeV particles.
The observed change in colatitude
is caused by drift due to the curvature and gradient of the
Parker spiral magnetic field (Paper I, Paper II), and the amount of drift increases with particle
energy.

\begin{figure}
\epsscale{.8}
\plotone{dalla_fig2.ps}
\caption{Time variation of $\Delta K / K_0$  averaged over each initially monoenergetic population with $K_0$= 1 MeV, 10 MeV, 100 MeV and 1 GeV. The top panel is for $\lambda$=1 AU and the bottom panel for the
scatter-free case. Other parameters of the simulations are as in Figure \ref{fig.kinenergy_perc_change}.
\label{fig.kinenergy_time_change}}
\end{figure}

Figure \ref{fig.kinenergy_perc_change} shows a trend for the deceleration to increase with $\Delta \theta$ for the cases where  $K_0$= 1 MeV, 10 MeV and 100 MeV, but not for the case $K_0$= 1 GeV.

In Figure \ref{fig.kinenergy_time_change} the kinetic energy change averaged over each of the four particle populations, is plotted versus time. The top panel shows the case $\lambda$=1 AU, corresponding
to the same simulations shown in Figure \ref{fig.kinenergy_perc_change}, while the bottom panel
presents the time dependence of energy change in the scatter-free case.
Figure \ref{fig.kinenergy_time_change} shows that the decrease in  kinetic energy is fast during the first
$\sim$20 hours of the propagation, and continues to take place more slowly at later times.
Deceleration is seen also in the absence of scattering, although it is of a reduced
magnitude compared to the $\lambda$=1 AU scattering case.

\section{Deceleration processes}\label{sec.kinenergy}

\subsection{Energy change due to drift in the electric field potential} \label{sec.driftinduced}

As energetic particles propagate through the interplanetary medium, in the fixed, non-rotating reference frame they are subject to the electric field associated with the outwardly moving solar wind. The solar wind electric field is given by:
\begin{equation}
\mathbf{E} = -  \frac{\mathbf{v}_{sw} \times \mathbf{B}}{c}   \label{eq.electricfield1}
\end{equation}
where $\mathbf{v}_{sw}$ is the solar wind velocity, $\mathbf{B}$ is the interplanetary magnetic field (IMF) and $c$ is the speed of light.

We consider $\mathbf{B}$ to be a unipolar Parker spiral, and the solar wind flow to be radial, uniform over the Sun's source surface and time independent. With these assumptions, the expression for the electric field takes the form \citep{Bur1968, Win1968}:
\begin{equation}
\mathbf{E} = - \frac{A}{c} \, \Omega  \, B_0 \, \frac{r_0^2}{r} \, \sin{\theta} \,\, \mathbf{e}_{\theta}  \label{eq.etheta}  \\
\end{equation}
where $\mathbf{e}_{\theta}$ is the standard unit vector in a ($r,\theta,\phi$) spherical coordinate system centered on the Sun,
with $r$ the radial distance, $\theta$ the colatitude and $\phi$ the longitude. Here $B_0$ is the magnitude of the magnetic field at a reference radial distance $r_0$ and
$\Omega$=2.87$\times$10$^{-6}$ rad s$^{-1}$ is the solar rotation rate.
$A$=1 when $\mathbf{B}$ points outward from the Sun and and $A$=$-$1 when $\mathbf{B}$ points inwards.

The potential associated with the electric field of Eq.~(\ref{eq.etheta}) is given by:
\begin{equation}
\Phi = - \frac{A}{c} \, \Omega \, B_0 \, r_0^2  \, \cos{\theta} \label{eq.epotential}
\end{equation}

In the absence of other effects causing deceleration, the kinetic energy change due to motion in the direction of the solar wind electric field is given by:
\begin{equation}
\Delta K_{(\Phi)} = \frac{q \, A}{c} \, \Omega \, B_0 \, r_0^2 \, (\cos{\theta} - \cos{\theta_0})  \label{eq.delta_ek_potential}
\end{equation}
with $q$ the particle charge, $\theta_0$ its initial colatitude and the subscript ${(\Phi)}$ indicating that this is the energy change associated with the potential of Eq.~(\ref{eq.epotential}).
Expressions equivalent to Eq.~(\ref{eq.delta_ek_potential}) were derived by \cite{Kot1979}.

If particles do not move in colatitude, $\theta$=$\theta_0$ and
the kinetic energy change given by Eq.~(\ref{eq.delta_ek_potential}) is zero.
However Papers I and II demonstrated that curvature and grad-$B$ drift combine to produce a significant component of drift in ${\theta}$, which, from Eq.~(\ref{eq.delta_ek_potential}), will cause kinetic energy change.
The drift in colatitude is present also in the absence of scattering.

Eq.~(\ref{eq.delta_ek_potential}) can be rewritten as:
\begin{equation}
\Delta K_{(\Phi)} = A\,  \mbox{sign}(q) \, \xi_0 \, (\cos{\theta}-\cos{\theta_0})  \label{eq.delta_ek_potential2}
\end{equation}
where:
\begin{equation}  \label{eq.xi0_def}
\xi_0= \frac{|q|}{c} \,  \Omega \, B_0 \, r_0^2
\end{equation}
For a proton or an electron, using the same values for $B_0$ and $r_0$ used in Papers I and II, we obtain that $\xi_0$=247 MeV.

Paper II showed that for the case of a positive polarity of the Parker spiral IMF ($A$$>$0) and particle initial positions not far from the heliographic equatorial plane, ions drift downwards (increasing colatitude) and electrons upwards (decreasing colatitude). Hence from Eq.~(\ref{eq.delta_ek_potential2}) both ions and electrons will experience a negative $\Delta K_{(\Phi)}$, i.e.~a deceleration, as a result of drift motion.

For a negative polarity configuration ($A$$<$0) protons near the equatorial plane drift upwards and electrons downwards, so that the effect of the drift is again deceleration for ions and electrons.

The expression for the energy change (Eq.~(\ref{eq.delta_ek_potential})) does not involve the initial particle energy explicitly, however the latter is an important parameter in determining how much the particle drifts in colatitude, i.e.~the value of $\cos{\theta}-\cos{\theta_0}$.

\begin{figure*}
\epsscale{1.90}
\plotone{dalla_fig3.ps}
\caption{Percentage change in kinetic energy as a function of $\Delta \theta$,
four days after injection,
for three values of the scattering mean free path $\lambda$ and varying initial kinetic energy.
The red dots are from simulations including both adiabatic deceleration and drift-induced deceleration,
the green dots are for simulations without adiabatic deceleration, i.e. scattering taking place in the fixed frame. The blue square represents the scatter-free case.
\label{fig.lambda_dependence}}
\end{figure*}

\subsection{Energy change due adiabatic deceleration}

In standard transport theory, heliospheric energetic particles experience cooling due to the expansion of the solar wind, which carries the turbulence that produces particle scattering. Formalism to describe this adiabatic deceleration within a transport equation was derived by \citet{Par1965} for the case of an isotropic particle distribution function and radially directed magnetic field.

Particle scattering in the solar wind frame is essential for adiabatic deceleration. In the absence of scattering, this process does not take place.

\citet{Ruf1995} generalised the classic treatment to the case of particles of arbitrary pitch angle and a Parker spiral configuration, pointing out how the combination of focussing and scattering produces a deceleration in the solar wind frame.
The rate of deceleration for a single particle is given by \citep{Ruf1995}:
\begin{equation} \label{eqn.ad_decel}
\frac{d p'}{dt}= - p' v_{sw}  \left[  \frac{\sec{\psi}}{2 L(z)} (1-\mu'^2) + \cos{\psi}\frac{d }{dr}\sec{\psi} \mu'^2 \right]
\end{equation}
where $p'$ and $\mu'$ are the particle's momentum and pitch angle in the solar wind frame, $\psi$ is the angle between the Parker spiral magnetic field line and the radial direction and $L(z)$ is the focussing length. Here $z$ is the only spatial variable retained within the model, describing the distance travelled along a magnetic field line.

From Eq.~(\ref{eqn.ad_decel}), the characteristic time of deceleration $\tau$=$-$$(1/p'\, dp'/dt)^{-1}$ depends only on the geometrical parameters, including the colatitude, via the angle $\psi$ and $L$, and on the particle pitch angle, i.e. it does not depend explicitly on the particle's kinetic energy nor species.
However the latter parameters influence the overall trajectory and amount of time that a particle spends at a given location, and as a result the overall energy change experienced.
If the scattering mean free path is small, particles tend to spend a longer time in regions near the Sun, where adiabatic deceleration
is stronger, so that a lower value of $\lambda$ gives rise to more deceleration associated with this process  \citep{Par1965}.

An adiabatic deceleration formalism alternative to Eq.~(\ref{eqn.ad_decel})
had been derived earlier by \cite{Ski1971}, for a generic magnetic field.
For the case of a Parker spiral field, it can be shown analytically that the  \cite{Ski1971} expression
takes the same form as the \citet{Ruf1995} one, so that the two formulations
are equivalent in this case, as noted in the latter paper.

\section{Interpretation of simulation results}

Having introduced the concepts of drift-induced and adiabatic deceleration we can now interpret the results shown in
Figures  \ref{fig.kinenergy_perc_change} and \ref{fig.kinenergy_time_change}.
Our simulations do include adiabatic deceleration because scattering is taking place in the solar wind frame. They also include
drifts which produce changes in colatitude and thus energy change.

In Figure  \ref{fig.kinenergy_perc_change}, the observed trend for deceleration to increase with $\Delta \theta$ (as seen for  $K_0$= 1 MeV, 10 MeV and 100 MeV) is consistent with drift-induced deceleration playing a significant role.
The fact that deceleration is present also in the scatter-free case (Figure \ref{fig.kinenergy_time_change}, bottom panel), when no adiabatic deceleration is taking place, confirms this statement.

Low energy SEPs experience very little drift, however their initial kinetic energy is much smaller than $\xi_0$ (given by Eq.~(\ref{eq.xi0_def})),
the magnitude of the largest possible deceleration associated with drift processes.
Considering Eq.(\ref{eq.delta_ek_potential2}), one can see that
even a small $\Delta \theta$ can produce a significant percentage change in their energy, the behaviour shown in Figure \ref{fig.kinenergy_perc_change} (e.g.~for $K_0$=1 MeV).
SEPs of initial energy 1 GeV typically drift by tens of degrees, however their drift-induced deceleration as percentage of initial energy is much less than for lower energy particles due to the larger ratio $K_0/\xi_0$. As one considers particles of even higher energy, drift-induced deceleration becomes less significant.

The deceleration seen in Figures  \ref{fig.kinenergy_perc_change} and \ref{fig.kinenergy_time_change} is a combination of adiabatic and drift-induced deceleration.
However it is possible to \lq switch off\rq\ adiabatic deceleration by scattering particles in the fixed frame, rather than in the solar
wind frame. When this is done, particle energy is conserved in the fixed frame during a scattering event,
while a change in pitch angle does result, influencing the particle's trajectory.
Scatter-free simulations represent an extreme case:
here no adiabatic deceleration takes place due to the absence of
scattering events and particles propagate together as a beam.
Drift and the deceleration it produces cannot be eliminated in our simulations.

Figure \ref{fig.lambda_dependence} shows the output of simulations carried out in three very different scattering conditions, each corresponding to a column in the figure.
Red points are the results for the cases with adiabatic deceleration (scattering carried
out in the solar wind frame). Points in the central column ($\lambda$=1 AU)
are the same as in Figure \ref{fig.kinenergy_perc_change}, and the
columns on the left and right show the results for $\lambda$=0.3 AU and 10 AU respectively.
The light green points
show the energy change observed when scattering is carried out in the fixed frame, i.e.~no adiabatic deceleration is occuring,
for the same values of the mean free path.
The blue squares represents the deceleration observed in the scatter-free case: here all particles experience
the same $\Delta \theta$ due to drift, resulting in a single point in the plots and no adiabatic deceleration.

Considering first of all the red points in Figure \ref{fig.lambda_dependence}, one can see that as the level of scattering increases
(i.e.~moving from right to left in the figure),
more deceleration is observed and the range of percentage change in $\Delta K$ increases.
The amount of drift, represented by the range of $\Delta \theta$ values also increases, as was noted in Paper I.
Considering that in our simulations the mean free path values
vary by almost 2 orders of magnitude, from 10 AU to 0.3 AU, the amount of deceleration appears to be only a weak function of the
mean free path.

When no adiabatic deceleration is present (light green points), the amount of deceleration observed has much less scatter and follows a line which is found to coincide exactly with that
predicted by Eq.~(\ref{eq.delta_ek_potential2}), i.e.~the observed energy change is purely drift-induced deceleration.
It is also apparent that any effects due to large finite Larmor radius are small in our simulations, as the data points for this case lie
along a single line in   Figure \ref{fig.lambda_dependence}, without significant scatter.

We can now compare the results for the cases with adiabatic deceleration, without it and the scatter-free situation.
Looking at the
low scattering regime ($\lambda$=10 AU), it is apparent that the addition of adiabatic deceleration broadens the distribution around the line predicted by Eq.~(\ref{eq.delta_ek_potential2}), and the
effect becomes more marked for stronger scattering. Switching on adiabatic deceleration eliminates the low values of $|\Delta K / K_0|$ which
are present in the case of purely drift-induced deceleration (e.g.~for $K_0$=1 MeV values of $|\Delta K / K_0|$$<$30$^{\circ}$).
In the strong scattering case, adiabatic deceleration is more efficient, resulting in a distribution
of $\Delta K  / K_0$ values which does not show a clear dependence on $\Delta \theta$, unlike for the $\lambda$=10 AU case.
The weak dependence of the overall deceleration on the value of the mean free path demonstrates that drift-induced deceleration plays a very significant role.

Regarding the reason why a small minority of particles with $K_0$=1 GeV show acceleration (Figure \ref{fig.kinenergy_perc_change}, bottom panel), we note that it is possible for the process responsible for adiabatic deceleration to produce acceleration in the fixed frame in some cases (as can be seen from the qualitative description accompanying Figure 1 of \citet{Ruf1995}).

In the simulation discussed so far, particles were injected at 1 solar radius. We have also carried out simulations with injection at 40 solar radii for $\lambda$=1 AU and the deceleration observed is very similar to that shown in Figure \ref{fig.kinenergy_perc_change}.
Therefore the effects describe above apply both to particles energised in solar flares and to those accelerated in CME driven-shocks at distances up to at least  40 solar radii.

\section{Discussion and conclusions}

Our relativistic full orbit test particle simulations of proton propagation in the Parker spiral have allowed us to analyse, for the first time,
the deceleration associated with drift motion opposite to the solar wind electric field.
We showed that the overall deceleration experienced by SEPs is due to contributions from
adiabatic deceleration (which requires scattering) and drift-induced deceleration (which is present
also in the absence of scattering).

We found that energy changes associated with the combined processes of drift-induced and adiabatic deceleration are very large:
for a scattering mean free path of $\lambda$=1 AU,  $\Delta K / K_0$ at 100 hours after injection ranges between $-$35\% and $-$90\%
for particles with $K_0$=1 MeV, between  $-$30\% and $-$70\% for $K_0$=10 MeV and between  $-$20\% and $-$55\% for $K_0$=100 MeV.

It is interesting to note that while the magnitude
of drift, as measured by the change in colatitude,  is very small for protons at $\sim$1 MeV, its effect
on particle energy is large,
meaning that drift effects cannot be ignored even at these low energies.

With reference to the very large values of deceleration obtained from our simulations for  particles of initial energy of 1 MeV,
e.g.~values close to 100\%, the test particle approximation breaks down once the particle energy has reached values close enough to
that of solar wind particles, so that a different modelling approach is required.

Deceleration is fast during the first $\sim$20 hours following injection and continues at a slower rate in the subsequent hours.
The fact that it is taking place also for scatter-free propagation means that it cannot be ascribed to standard adiabatic
deceleration only.
In addition, the simulations with scattering taking place in the fixed frame (i.e.~with scattering present but
adiabatic deceleration \lq switched off\rq) demonstrate the large magnitude of drift-induced deceleration.

The magnitude of the constant $\xi_0$ appearing in the expression for the solar wind electric potential (Eq.~(\ref{eq.delta_ek_potential2})) determines the particle energy
range over which the effect of drift-induced deceleration is most prominent.
It appears that for protons this is the range between $\sim$1 and a few hundred MeV, which is the typical SEP energy range.
At proton energies larger than 10 GeV the energy change becomes negligible, therefore its importance for galactic cosmic rays is for modulated cosmic rays in the solar wind with energies in the $\sim$1 MeV -- 1 GeV range.

We also emphasize that drift additional to that due to the large scale Parker spiral field and  any other process which is able to produce transport in the latitudinal direction will cause
changes in kinetic energy.

Is drift-induced deceleration included within the standard transport equations \citep{Ski1971, Ruf1995} used in SEP modelling, data analysis and Space Weather forecasting? Answering this question requires
analysis of the derivation of the focussed transport equation \citep{Ski1971}. This equation describes the evolution of the distribution function of the particles' guiding centres and
is obtained by averaging the Vlasov equation over gyrophase (e.g.~\citet{Zan2014}).
\citet{LeR2009} showed that the focussed transport equation is equivalent to the guiding centre kinetic equation \citep{Kul1983}. The latter is derived by means of the standard assumptions of first order
guiding centre theory, including the assumption that the grad B and curvature drift velocities are much smaller than the {\bf E}$\times${\bf B} drift velocity.
As shown by \citet{LeR2009}, the guiding centre kinetic equation includes a contribution from grad B and curvature drift in its energy change term, while the latter drifts are not included in the
spatial convection term. This means that the energy change associated with drift is taken into account in an approximate way, with the deceleration rate being calculated along the \lq undrifted\rq\ orbit, at constant colatitude.
To our knowledge, all current SEP transport models (e.g.~\citet{Zha2009}, \citet{Mas2012}) make use of this approximation, which we expect to be fairly accurate for low energy SEPs but less accurate for high energy ones, due to their substantial latitudinal drift.
A more precise solution would be obtained by solving a transport equation that includes the grad B and curvature drifts within the spatial convection term, i.e. by solving eqs.~(30)--(34) of \citet{Zha2006}.

It should also be noted that in Paper II we showed that the grad B and curvature drift velocities in the Parker spiral can be of the same
order of magnitude as the {\bf E}$\times${\bf B} drift velocity, and in some cases even larger. Therefore the standard guiding centre theory assumption
that the {\bf E}$\times${\bf B} drift is the dominant one may not be valid for the case of heliospheric propagation.

We conclude that the extent to which the  drift-induced deceleration observed in our test particle simulations is accounted for by SEP models based on the focussed transport equation needs to be evaluated, and this will be the subject of future work.

Strong SEP deceleration such as the one we reported, has an impact on the analysis of measurements, because it introduces a scenario
where particles detected in a given energy channel at 1 AU actually left the Sun having a much higher energy, as was emphasized
by \cite{Mas2012} for heavy ions in the $\sim$MeV/nucleon range. Our results show that this may be taking place for protons
in the 10-100 MeV range too.

Overall, our results demonstrate that drift-induced deceleration is an important process in SEP propagation and needs accurate inclusion within SEP modelling and data analysis.

\acknowledgments

This work has received funding from the European Union Seventh
Framework Programme (FP7/2007-2013) under grant agreement n.~263252
[COMESEP] and from the UK Science and Technology Facilities Council (STFC) (grants ST/J001341/1 and
ST/M00760X/1). SD acknowledges support from ISSI through funding for the International Team on \lq Superdiffusive transport in space plasmas and its influence
on energetic particle acceleration and propagation\rq.
We thank R.~Vainio for useful discussions.

\bibliographystyle{apj}

redpajama_set_name: RedPajamaArXiv


text:
Home Entertainment John Barrowman Dancing On Thin Ice: Judge Faces Axe Over Allegations
John Barrowman Dancing On Thin Ice: Judge Faces Axe Over Allegations
John Barrowman is facing a dismissal from Dancing On Ice, following claims of inappropriate behavour made against the judge.
Barrowman who joined the show last year, has come under fire following claims he exposed himself whilst on set for Doctor Who. Barrowman was accused of inappropriate behaviour along with co-star Noel Clarke.
Following allegations made by up to 20 women who worked with the producer whilst on Doctor Who and his recently cancelled show Viewpoint, Clarke was dropped by Sky and ITV from future projects.
These allegations included, bullying, sexual harrassment and unwanted sexual contact.
Clarke himself released a statement.
"Some of my actions have affected people in ways I did not intend or realise", he said.
Recently, Barrowman claimed that his actions were nothing more than "tomfoolery".
"With the benefit of hindsight, I understand that upset may have been caused by my exuberant behaviour and I have apologised for this previously", Barrowman said.
"No way we can invite him back": Source on the future of John Barrowman
Regarding Barrowman's future on Dancing On Ice, a source had this to say.
"Ever since allegations against John came to light, discussions have been ongoing over his future on the panel of Dancing On Ice".
"But the feeling now is there is no way we can invite him back", the source also added. "ITV has shown they are prepared to act decisively when stars are accused of inappropriate behaviour. And it seems this situation will not be the exception to the rule".
These allegations against Barrowman come after a video resurfaced online of Noel Clarke talking about Barrowman exposing himself.
According to the Guardian, a number of women who worked with the Captain Harkness actor on Doctor Who and his BBC spin-off Torchwood, claimed that they regularly witnessed him expose himself.
"He would get his genitals out on a regular basis", one witness said.
Another witness described Barrowman's conduct as "inappropriate", rather than predatory.
Regarding these allegations and Barrowman's future, ITV released this statement.
"Any discussions regarding the 2022 series of Dancing on Ice are very premature. Production has yet to commence".
Dancing On Ice
Noel Clarke
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Today In Music History – August 14th.


This Opera Monte-Carlo production fascinates with a contemporary stage direction by Jean-Louis Grinda and a buoyant conducting by Daniele Callegari.
Rarely performed Mozart Opera conducted by Marc Minkowski and staged by Marshall Pynkoski at Teatro alla Scala.
In his 'new life' as a baritone, Plácido Domingo has triumphed in Los Angeles, London and Vienna. Now he takes the role of Francesco Foscari to La Scala, Milan, the theatre that is the symbol of Italian opera.
The highlight of the Paris Opera's season includes an all-star cast: Jonas Kaufmann, Sonya Yoncheva, Elīna Garanča, Ildar Abdrazakov and Ludovic Tézier.
Bring the 109 musicians in the Gothenburg Symphony wherever you are. Try the new premium version for 7 days for free!
For this glittering premiere, Vienna and Paris pull close together: the 200 year-old mdw and the 222 year-old CNSM Paris present a joint orchestra.
Glyndebourne Tour 2017 opens this month with another chance to see Brett Dean's hit new opera Hamlet.


text:
Q: I use OR to form a multiple condition IF ELSE statement on VBA, it's not working Dim cat As Integer
For cat = 2 To last
    Range("AB" & cat).Select

    If Selection.Value = " " Then
        ActiveCell.Offset(0, -2).Value = "-"
        ActiveCell.Offset(0, -1).Value = "-"

    ElseIf Selection.Value = "Address in local wording" Then
        ActiveCell.Offset(0, -2).Value = "Customer"
        ActiveCell.Offset(0, -1).Value = "Incomplete information or awaiting more info from customer"

    ElseIf (Selection.Value = "hold to console" Or "Hold to console" Or "Allocated 14/12 and ship next day") Then
        ActiveCell.Offset(0, -2).Value = "Depot"
        ActiveCell.Offset(0, -1).Value = "Allotment delay"

    ElseIf (Selection.Value = "Backorder" Or "backorder" Or "Back order" Or "back order") Then
        ActiveCell.Offset(0, -2).Value = "Inventory"
        ActiveCell.Offset(0, -1).Value = "Material not available causing backorder"

    End If
Next cat

The result I get is when Selection.Value is empty,  "-" , "-"
and the rest all show "Depot" , "Allotment delay" only.
What's wrong with this code ?

A: Using the line below is incorrect:
ElseIf (Selection.Value = "hold to console" Or "Hold to console" Or "Allocated 14/12 and ship next day") Then

You need to add Selection.Value = before each condition, see line below:
ElseIf Selection.Value = "hold to console" Or Selection.Value = "Hold to console" Or Selection.Value = "Allocated 14/12 and ship next day" Then

Note: the same applies to all other ElseIfs you have.

Edit 1
However,I would suggest to use the code below. Your code is "screaming" for Select Case. Also, there is no need to Range("AB" & cat).Select and later use ActiveCell, instead you could just use fully qualifed Range.
Code
Dim cat As Long

For cat = 2 To last
    Select Case Range("AB" & cat).Value
        Case " "
            Range("AB" & cat).Offset(0, -2).Value = "-"
            Range("AB" & cat).Offset(0, -1).Value = "-"

        Case "Address in local wording"
            Range("AB" & cat).Offset(0, -2).Value = "Customer"
            Range("AB" & cat).Offset(0, -1).Value = "Incomplete information or awaiting more info from customer"

        Case "hold to console", "Hold to console", "Allocated 14/12 and ship next day"
            Range("AB" & cat).Offset(0, -2).Value = "Depot"
            Range("AB" & cat).Offset(0, -1).Value = "Allotment delay"

        Case "Backorder", "backorder", "Back order", "back order"
            Range("AB" & cat).Offset(0, -2).Value = "Inventory"
            Range("AB" & cat).Offset(0, -1).Value = "Material not available causing backorder"
    End Select

Next cat

A: I think you need to express equality in each condition.  In other words, instead of this:
(Selection.Value = "hold to console" Or
 "Hold to console" Or
 "Allocated 14/12 and ship next day") Then

you need to use this:
(Selection.Value = "hold to console" Or
 Selection.Value = "Hold to console" Or
 Selection.Value = "Allocated 14/12 and ship next day") Then

redpajama_set_name: RedPajamaStackExchange


While neither federal law nor state law requires that you register your protection order in order to get it enforced, if your order is not entered into the Connecticut state registry, it may be more difficult for a Connecticut law enforcement official to determine whether your order is real. Meaning, it could take longer to get your order enforced.
If you are unsure about whether registering your order is the right decision for you, you may want to contact a local domestic violence organization in your area. An advocate there can help you decide what the safest plan of action is for you in Connecticut. To see a list of local domestic violence organizations, go to our CT Advocates and Shelters page.


Sometimes life gets complex. Many times we just keep on going even though we are pulled between the demands of the people we love - Feed me! Love me! - with those feelings festering just under the surface.
Many of you, like me, probably talk to God throughout the day. But is there a sacred place set aside for you and God?
Don't set a time limit, or make it a duty.
Settle in with Him. Close the door.
Talk to Him about your day. Praise Him for His great love.
Breathe in the presence of the Holy Spirit. Don't rush it.
Let God do His work inside of You.


text:
Netflix Shares First Teaser for 'Ozark' Season 2, Sets August Premiere Date
Jason Bateman-Laura Linney drama returns August 31
Reid Nakamura | June 21, 2018 @ 8:00 AM	Last Updated: June 21, 2018 @ 8:31 AM
Ten months after renewing "Ozark" for a second season, Netflix has finally set the premiere date for the second outing of the Jason Bateman-led drama.
In addition to four new photos, Netflix has also released a short new teaser for "Ozark" Season 2, revealing that the series will finally make its return on August 31.
The second season will continue to follow Marty Byrde (Bateman) and his family as they navigate the murky waters of life within a dangerous drug cartel.
Also Read: 'Ozark' Star Laura Linney on Pushing Jason Bateman to Flesh Out Her Role: 'She Was Basically Just a Wife'
With Del (Esai Morales) out, the crime syndicate sends their ruthless attorney Helen Pierce (Janet McTeer) to town to shake things up just as The Byrdes are finally settling in. Marty and Wendy (Laura Linney) struggle to balance their family interests amid the escalating dangers presented by their partnerships with the power-hungry Snells, the cartel and their new deputy, Ruth Langmore (Julia Garner), whose father Cade (Trevor Long) has been released from prison. The stakes are even higher than before and The Byrdes soon realize they have to go all in before they can get out.
Sofia Hublitz, Skylar Gaertner, Julia Garner, Jordana Spiro, Jason Butler Harner, Peter Mullan and Lisa Emery also star.
Bateman also serves as an executive producer on the series, alongside Chris Mundy, Bill Dubuque and Mark Williams. Patrick Markey is a producer. "Ozark" is produced by Media Rights Capital and Aggregate Films.
Also Read: 'Ozark:' Ruth Langmore Teaches You How to be the Perfect Criminal (Exclusive Video)
Netflix in June: What's Coming and What to Watch Before It's Gone (Photos)
Arriving June 3: "The Break With Michelle Wolf"
"The Daily Show" alum made waves with her White House Correspondence Dinner jokes, and now she's landed on Netflix for a weekly show.
Arriving June 5: "Thor: Ragnarok"
The third "Thor" movie from Marvel Studios Ragna-rocked our world (sorry), and now you can stream it on Netflix.
Arriving June 8: "Sense8: The Series Finale"
Find your cluster and buckle in for the much anticipated two-hour finale of "Sense8."
Arriving June 15: "Queer Eye" Season 2
We're not crying -- you're crying! Grab your tissues, because we were not expecting to get more heartfelt makeover this soon. But we are so ready for more of the Fab 5.
Arriving June 22: "Marvel's Luke Cage" Season 2
Luke is going viral in Season 2, and going up against new villain Bushmaster. Oh, yeah -- did we mention he also works out with New York Jets coach Todd Bowles?
Arriving June 29: "Glow" Season 2
The critically acclaimed comedy is back, and the gorgeous ladies of wrestling are stepping it up a notch this time around with a television series.
Leaving June 1: "8 Mile"
Load up on mom's spaghetti and re-watch Eminem's coming up story before it leaves next month.
Leaving June 25: "Captain America: Civil War"
"Civil War" is one of our highest-ranked Marvel movies, and we'll definitely have to re-watch it before it leaves the streamer at the end of June.
Second seasons of "Queer Eye," "Marvel's Luke Cage" and "Glow"
'Ozark' Star Laura Linney on Pushing Jason Bateman to Flesh Out Her Role: 'She Was Basically Just a Wife'
By Steve Root | May 30, 2018 @ 5:00 PM
'Dunkirk,' 'Baby Driver,' 'Game of Thrones' and 'Ozark' Win Location Managers Awards
By Steve Pond | April 7, 2018 @ 9:39 PM
Golden Globes TV Predictions: From 'The Handmaid's Tale' to 'Ozark' (Photos)
By Steve Pond | January 7, 2018 @ 11:58 AM