Jun 29th: The July 2, 2019, Total Solar Eclipse
by Jay Pasachoff | Jun 29, 2019 | Solar Eclipse | 0 comments
Podcaster: Jay Pasachoff
Title: The July 2, 2019, Total Solar Eclipse
Organization: Williams College and Caltech
Links: http://www.eclipses.info and http://www.totalsolareclipse.org
Description: On July 2, the path of totality of a total solar eclipse will cross the Pacific Ocean, including Oeno Island, and then cross Chile and Argentina. Scientists and tourists will observe the path of totality, especially from the region of Chile that includes La Serena and the Elqui Valley, with the Cerro Tololo Inter-American Observatory among astronomical facilities in totality. The observations at this minimum phase of the sunspot cycle will provide important information about the solar corona, and will fill in the ordinary gaps between on-disk extreme-ultraviolet imaging and satellite imaging of the outer corona.
Bio: Jay Pasachoff is Field Memorial Professor of Astronomy at Williams College and Chair of the International Astronomical Union's Working Group on Eclipses. He is on sabbatical at Carnegie Observatories.
The fifth edition of his textbook The Cosmos: Astronomy in the New Millennium (Pasachoff and Alex Filippenko, and a new book on the intersection of art and astronomy, Cosmos: The Art and Science of the Universe (Roberta J. M. Olson and Pasachoff), have just been published.
See http://solarcorona.com
Bio: Jay Pasachoff is Field Memorial Professor of Astronomy at Williams College and Chair of the International Astronomical Union's Working Group on Eclipses. He is on sabbatical at Carnegie Observatories. The fifth edition of his textbook The Cosmos: Astronomy in the New Millennium (Pasachoff and Alex Filippenko, and a new book on the intersection of art and astronomy, Cosmos: The Art and Science of the Universe (Roberta J. M. Olson and Pasachoff), have just been published. See http://solarcorona.com
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We are looking forward to the next total solar eclipse, July 2nd, 2019. The path of the eclipse will cross South America—Chile and Argentina—after going across the Pacific and we hope to see what we saw at the '17 total solar eclipse, the most recent total solar eclipse in which the path of totality crossed the United States.
What happens during an eclipse is that the moon goes in front of the sun and a total eclipse is a little closer than average in its orbit around the earth and entirely covers the everyday sun so that we see the outer parts of the sun, the solar corona. But sometimes the moon is a little smaller than average and a ring of everyday sunlight, an annulus of sunlight, remains visible and that makes the sky too bright. The blue sky remains and we can't see the corona so we scientists are especially interested in the total solar eclipses when the sky is dark and we can't see the corona, the outer atmosphere of the sun. It is about a million time darker than a normal day so even if one percent of the everyday sun remains visible that's still ten-thousand times brighter than it is during a total eclipse so you really have to get into the path of the total eclipse.
The path on July 2nd, 2019, crosses the Pacific. It passes only one island but is mainly over ocean, and just hits South America, where it is low in the sky. It is only about thirteen degrees above the horizon when it reaches the coast of Chile and then at sunset on the horizon just inside the Atlantic coast of Argentina.
18 months later, in December 2020, which is then summertime in South America, there will be another total solar eclipse a little further south, also crossing Chile and Argentina. At that time, the peak will be over Argentina and the sun will be over 70 degrees high in the sky in Argentina. And my group will be located on the Atlantic coast of Argentina.
In any case, we only occasionally get these total solar eclipses—every 18 months or so on the average—and the sun is different every time. Here, for example, is a series of three different total eclipses that were painted almost 100 years ago by Howard Russell Butler in oils. At that time, the cameras couldn't show with the photographic plates or film the detail of the corona the way they can today, so Butler took notes during the couple of minutes of totality and then used his skills as a portrait painter to translate it into oil paintings. These paintings in particular hung for decades over the entrance of the Hayden Planetarium in New York, part of the American Museum of Natural History. Butler had first been invited by the US Naval Observatory on the 1918 expedition to Oregon, and then he got interested as one might and painted also 1923, 1925 that you just saw, and also in 1932.
In any case, we have many scientific observations that we can make only at total solar eclipses. The corona changes with the sunspot cycle, the roughly 11-year sunspot cycle. We are now at the minimum of the sunspot cycle; most days have no sunspots at all on the surface of the sun and that means there are only a few coronal streamers relatively close to the solar equator and the poles remain visible where there are plumes that come out of the poles looking much like the filings that come out of a bar magnet. All this illustrates how important the magnetic field is for the sun.
The magnetic field in sunspots was discovered by George Ellery Hale at the Mount Wilson Observatory in 1908 and the sunspot regions are regions of especially strong magnetic field. But the coronal magnetic fields, which are weaker, are still strong enough to govern the very hot gas around the sun.
It was discovered at an eclipse in 1869 that there were some special spectral emissions from the corona, in particular a strange one in the green, "the coronal green line." In 1868, they found a yellow line which was soon called helium because it was only from the sun. The next year, in 1869, the coronal green light was seen and they thought it was from "coronium," a new element as helium turned out to be. As you know, helium did turn out to be a fundamental element but they didn't discover that until 1895, when they isolated it on Earth. And coronium took until 1940 to explain, and then it was finally realized that it wasn't a new element but it was really only a form of iron that only existed when it was so hot—over a million degrees—that half of iron's normal 26 electrons had been driven off so this is iron that's 13 times ionized (since the neutral state is Roman numeral I), which is called iron 14. And we now have several spectral lines of different ionization stages and elements.
We will be observing those from our sites in Chile. I will be at a mine at a mountainside at an altitude of about 2200 feet on the centerline as it passes Chile. And unusually, there is actually a couple of major astronomical observatories in the zone of totality. I have permission to have 4 of my colleagues at the Cerro Tololo Inter-American Observatory for the eclipse, and they will have a variety of cameras and telescopes to make images of the sun both in ordinary light—what we call white light, all the sunlight together— and also through some special filters and with some spectrographs. So when we only get a couple of minutes every year and a half or so to see what the corona is like in detail, we want to take advantage of that. And then we can put together these observations at eclipses from what we can get from NASA and European Space Agency spacecraft, which can't observe the region of the sun that we see best at total solar eclipses. So only on the days of total solar eclipses do we get a complete view of the sun including all of its layers.
And we should also remember that the sun is a typical star and that there are billions and trillions of stars like the sun, so when we are observing the details of the solar corona at an eclipse, we're learning what the details are of the coronas of all these distant stars that are all fuzzed out without our ability to see detail.
A total solar eclipse remains a scientifically valuable occasion and also a fantastic occasion for individuals to see.
The 365 Days of Astronomy Podcast is produced by Astronomical Society of the Pacific. Audio post-production by Richard Drumm. Bandwidth donated by libsyn.com and wizzard media. You may reproduce and distribute this audio for non-commercial purposes. Please consider supporting the podcast with a few dollars (or Euros!). Visit us on the web at 365DaysOfAstronomy.org or email us at info@365DaysOfAstronomy.org. This year we will celebrates the Year of Everyday Astronomers as we embrace Amateur Astronomer contributions and the importance of citizen science. Join us and share your story. Until tomorrow! Goodbye!


Tracker's top 10 most stolen cars
30/04/2014 in Market Insight
The BMW X5 remains top of the car thief's shopping list, according to the latest figures from Tracker.
It was the car most frequently stolen and recovered in 2013 - the fifth year in a row that it has topped the table.
Last year Tracker recovered nearly £8,500,000 worth of stolen vehicles and returned them to their owners.
The BMW M3 was the second most stolen and recovered vehicle last year, moving up from third in 2012 and sixth place in 2011.
In 2012, the number two spot was occupied by the Range Rover Sport and Vogue, but in 2013, they sit in seventh and eighth place respectively.
The Mercedes-Benz C-Class makes its first appearance on the table, taking third place, while the Porsche 911 reappears in ninth for the first time since 2011.
BMWs dominated in 2013, with the 5 Series, X5, M3 and 3 Series all making the table.
However, the Audi A4 leapt from ninth position in 2011, up to fourth in 2013, while the Audi RS4 doesn't appear at all. The Audi S3 takes equal eighth with the Range Rover Vogue.
"It's clear from our latest figures that thieves continue to target prestige models with the most expensive car recovered being worth £90,000," said Adrian Davenport, police liaison officer for Tracker.
The chart suggests franchised dealers representing premium brands could have a real opportunity to upsell additional car security systems.
Author: Tim Rose Tim Rose
tim.rose@bauermedia.co.uk
As editor, Tim is responsible for the media content, planning and production of AM's multiple channels (AM print and digital magazines, website, social media and contributing to our events planning). He interviews and writes about as many franchised dealer groups and UK divisions of motor manufacturers as possible, to explore the issues facing UK motor retail and understand what solutions dealers and suppliers are using to overcome these.
Click here for aftersales best practice and procurement insight
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From the page to the stage: The Utica College Theatre Department
Picture of the cast for "Something Rotten!" as it begins rehearsal.
Charles Buckley, Staff Writer
There are many places where people can go on campus to enjoy extracurriculars. One of these places is the theater. The UC Theatre Department has put on many shows for people to enjoy over the years, the latest one, "Something Rotten!" has begun its rehearsal phase even while the pandemic is going on.
The department is run by Professor of Theater Laura Salvaggio. With the help of directors, stagehands and loyal actors she has successfully put on many plays and musicals over the last few years.
"I love the ability to shake everyone's emotional response in the room and have everyone feeling the same way while watching a scene be performed," Salvaggio said.
Many people, especially the actors, also enjoy the theater because it gives them a chance to be creative and let their imagination run wild as they recreate scenes either fictional or historical.
"My favorite thing about the theater is being able to play another character and see things through their point of view," Justin Jones said, a senior business major who acted for the theater during his time at Utica College. "It's very exciting."
One of the most recent productions was the radio play "War Of The Worlds," which was performed over the campus radio station, WPNR, last semester.
Along with the actors, A lot of people who do crew enjoy working on sets. Especially when it comes to making a set that helps enhance the performance.
"A lot of time and consideration goes into building the sets," Salvaggio said. "The crew usually has to work on creating a full-scale set from a not-to-scale model."
Musicals have seen some success for the department as well, such as "Urinetown," which was the last live musical performed in the Strebel Auditorium before the COVID pandemic began. However, one musical that many actors and viewers enjoyed the most and still talk about was "Cabaret," which the department did back in 2018.
"That musical was one of the biggest ones we had ever done," Salvaggio said. "It was fun and very engaging for everyone who was a part of it."
For something like "Cabaret" or any type of play, there is a process that truly helps take it from the page to on the stage in terms of performing.
"What truly brings a piece of theatre from page to stage is a collaborative art," said Hannah DeStefano, a junior and communications and media major. "Of course, you have the most visible part, the actors playing their roles, but you also have a working collaboration of artists in every facet. From set to costumes to orchestrations to lights and so much more. This transformation happens as each part of the working body comes alive and plays its role well."
Another major element brought from the page to stage in terms of a theater performance is everyone coming together.
"The magic of the musicals here is thanks to the collaborative spirit of the cast and crew," said Jason Francey, the assistant director for college engagement and the director of this year's musical "Something Rotten!". There are so many moving pieces and so many people involved that it's hard to pinpoint just one thing. It is truly thanks to the efforts of everyone that the show comes together and wows the audience."
The theater is always looking for people to help out in many different ways. If interested, send an email to Laura Salvaggio at [email protected].
UC Theatre Department
Charles Buckley, Clerk
Name: Charles Buckley
Class Year: Sophomore
Major: Communications and Media
Minors: Creative Writing and Theatre
Previous Position: Staff Writer...
Utica College Archives: A historical treasure


man of the house cast 1995
, man of the house cast tommy lee jones
Man of the House / Cast
Roland Sharp
Cedric the Entertainer
Percy Stevens
Brian Van Holt
Eddie Zane
Shea Whigham
Ranger Holt
Terry Parks
Ranger Riggs
Captain Nichols
Morgan Ball
Tom Reynolds
Who is the cast of Man of the House?
Man of the House (2005) Cast and Crew. Texas Ranger Roland Sharp (Tommy Lee Jones) follows a strict code of behavior and has no patience for those who don't follow suit. When five cheerleaders -- Anne (Christina Milian), Teresa (Paula Garcés), Evie (Monica Keena), Heather (Vanessa Ferlito) and Barb (Kelli Garner) -- witness a murder,...
Man of the House - Cast and Crew | Moviefone
www.moviefone.com/movie/man-of-the-house/17651/credits/
What is the movie Man of the house about?
From Wikipedia, the free encyclopedia Man of the House is a 2005 American crime comedy film directed by Stephen Herek and starring Tommy Lee Jones. The plot revolves around Sgt. Roland Sharp, a lonesome Texas Ranger who goes undercover as an assistant coach to protect a group of college cheerleaders who have witnessed a murder.
Man of the House (2005 film) - Wikipedia
en.wikipedia.org/wiki/Man_of_the_House_(2005_film)
What is the rating of Man of the House?
James Berardinelli of ReelViews panned the film, rating it one star out of four and writing: "The movie is an "action comedy" in name only - there's nothing in Man of the House that could be considered funny or exciting."
Who is the cast of the entertainer?
Cast (in credits order) complete, awaiting verification. Tommy Lee Jones. ... Roland Sharp. Cedric the Entertainer. ... Percy Stevens (as Cedric The Entertainer) Christina Milian.
Man of the House (2005) - Full Cast & Crew - IMDb
www.imdb.com/title/tt0331933/fullcredits/
www.imdb.com/title/tt0331933/fullcredits
Man of the House (2005) cast and crew credits, including actors, actresses, directors, writers and more.
Man Of The House Cast - Image Results
More Man Of The House Cast images
Man of the House Cast and Crew - Cast Photos and Info | Fandango
www.fandango.com/man-of-the-house-86074/cast-and...
Cast + Crew Friday, February 25, 2005 PG-13, 1 hr 37 min
Man Of The House Cast and Crew | TV Guide
www.tvguide.com/movies/man-of-the-house/cast/137851
Meet the cast and learn more about the stars of Man Of The House with exclusive news, pictures, videos and more at TVGuide.com
Man Of The House Cast and Characters | TV Guide
www.tvguide.com/tvshows/man-of-the-house/cast/738625
Meet the cast and learn more about the stars of of Man Of The House with exclusive news, photos, videos and more at TVGuide.com
www.moviefone.com/movie/man-of-the-house/17651/...
See the full list of Man of the House cast and crew including actors, directors, producers and more.
Man About the House (TV Series 1973–1976) - Cast & Crew - IMDb
m.imdb.com/title/tt0069607/fullcredits
Man About the House (1973–1976) Series Cast & Crew. Directed by (1) Writing credits (2) Cast (84) Produced by (2) Production Design by (7) Art Department (1)
"House M.D." Man of the House (TV Episode 2012) - Full Cast ...
"House M.D." Man of the House (TV Episode 2012) cast and crew credits, including actors, actresses, directors, writers and more.
man of the house cast 1995 kelli garner
man of the house cast tommy lee jones monica keena
man of the house cast and crew man of the house
movie man of the house cast anne archer
Man of the House
PG-132005 · Crime · 1h 40m
A taciturn Texas Ranger (Tommy Lee Jones) goes under cover as a coach to protect a group of college cheerleaders who witnessed a murder. en.wikipedia.org
Original release date: February 25, 2005
Director: Stephen Herek
Budget: $40 M
Paula Garcés
Professor Molly McCarthy
U.S. Marshals
Code Name: The Cleaner


Remote sensing of cometary bow shocks: Modelled asymmetric outgassing and pickup ion observations
Markku Alho, Riku Järvinen, Cyril Simon Wedlund, Hans Nilsson, Esa Kallio, Tuija Pulkkinen
Department of Electronics and Nanoengineering
Esa Kallio Group
Despite the long escort by the ESA Rosetta mission, direct observations of a fully developed bow shock around 67P/Churyumov–Gerasimenko have not been reported. Expanding on our previous work on indirect observations of a shock, we model the large-scale features in cometary pickup ions, and compare the results with the ESA Rosetta Plasma Consortium Ion Composition Analyser ion spectrometer measurements over the pre-perihelion portion of the escort phase. Using our hybrid plasma simulation, an empirical, asymmetric outgassing model for 67P, and varied interplanetary magnetic field (IMF) clock angles, we model the evolution of the large-scale plasma environment. We find that the subsolar bow shock standoff distance is enhanced by asymmetric outgassing with a factor of 2 to 3, reaching up to 18000km approaching perihelion. We find that distinct spectral features in simulated pickup ion distributions are present for simulations with shock-like structures, with the details of the spectral features depending on shock standoff distance, heliocentric distance, and IMF configuration. Asymmetric outgassing along with IMF clock angle is found to have a strong effect on the location of the spectral features, while the IMF clock angle causes no significant effect on the bow shock standoff distance. These dependences further complicate the interpretation of the ion observations made by Rosetta. Our data-model comparison shows that the large-scale cometary plasma environment can be probed by remote sensing the pickup ions, at least when the comet's activity is comparable to that of 67P, and the solar wind parameters are known.
Monthly Notices of the Royal Astronomical Society
https://doi.org/10.1093/mnras/stab1940
plasmas
shock waves
methods: numerical
techniques: miscellaneous
comets: individual: 67P
10.1093/mnras/stab1940Licence: CC BY
Alho_Remote_sensing_of_cometary_MNoRASFinal published version, 6 MBLicence: CC BY
Dive into the research topics of 'Remote sensing of cometary bow shocks: Modelled asymmetric outgassing and pickup ion observations'. Together they form a unique fingerprint.
outgassing Physics & Astronomy 100%
bows Physics & Astronomy 90%
remote sensing Physics & Astronomy 86%
interplanetary magnetic fields Physics & Astronomy 65%
shock Physics & Astronomy 61%
ion Earth & Environmental Sciences 50%
sensors Physics & Astronomy 48%
magnetic field Earth & Environmental Sciences 46%
Shocks and Magnetosheaths in the Heliosphere
Alho, M., Järvinen, R., Lakka, A., Knuuttila, O. & Pulkkinen, T.
Project: Academy of Finland: Other research funding
solar wind 100%
coronal mass ejection 82%
upstream 71%
ion 63%
extremely low frequencies 58%
Science-IT
Mikko Hakala (Manager)
Facility/equipment: Facility
Density functional theory 74%
Alho, M., Järvinen, R., Simon Wedlund, C., Nilsson, H., Kallio, E., & Pulkkinen, T. (2021). Remote sensing of cometary bow shocks: Modelled asymmetric outgassing and pickup ion observations. Monthly Notices of the Royal Astronomical Society, 506(4), 4735-4749. https://doi.org/10.1093/mnras/stab1940
Alho, Markku ; Järvinen, Riku ; Simon Wedlund, Cyril ; Nilsson, Hans ; Kallio, Esa ; Pulkkinen, Tuija. / Remote sensing of cometary bow shocks: Modelled asymmetric outgassing and pickup ion observations. In: Monthly Notices of the Royal Astronomical Society. 2021 ; Vol. 506, No. 4. pp. 4735-4749.
@article{23fdd3f2ddc147b7a800d4c86f69e10f,
title = "Remote sensing of cometary bow shocks: Modelled asymmetric outgassing and pickup ion observations",
abstract = "Despite the long escort by the ESA Rosetta mission, direct observations of a fully developed bow shock around 67P/Churyumov–Gerasimenko have not been reported. Expanding on our previous work on indirect observations of a shock, we model the large-scale features in cometary pickup ions, and compare the results with the ESA Rosetta Plasma Consortium Ion Composition Analyser ion spectrometer measurements over the pre-perihelion portion of the escort phase. Using our hybrid plasma simulation, an empirical, asymmetric outgassing model for 67P, and varied interplanetary magnetic field (IMF) clock angles, we model the evolution of the large-scale plasma environment. We find that the subsolar bow shock standoff distance is enhanced by asymmetric outgassing with a factor of 2 to 3, reaching up to 18000km approaching perihelion. We find that distinct spectral features in simulated pickup ion distributions are present for simulations with shock-like structures, with the details of the spectral features depending on shock standoff distance, heliocentric distance, and IMF configuration. Asymmetric outgassing along with IMF clock angle is found to have a strong effect on the location of the spectral features, while the IMF clock angle causes no significant effect on the bow shock standoff distance. These dependences further complicate the interpretation of the ion observations made by Rosetta. Our data-model comparison shows that the large-scale cometary plasma environment can be probed by remote sensing the pickup ions, at least when the comet{\textquoteright}s activity is comparable to that of 67P, and the solar wind parameters are known.",
keywords = "plasmas, shock waves, methods: numerical, techniques: miscellaneous, comets: individual: 67P",
author = "Markku Alho and Riku J{\"a}rvinen and {Simon Wedlund}, Cyril and Hans Nilsson and Esa Kallio and Tuija Pulkkinen",
doi = "10.1093/mnras/stab1940",
journal = "Monthly Notices of the Royal Astronomical Society",
Alho, M, Järvinen, R, Simon Wedlund, C, Nilsson, H, Kallio, E & Pulkkinen, T 2021, 'Remote sensing of cometary bow shocks: Modelled asymmetric outgassing and pickup ion observations', Monthly Notices of the Royal Astronomical Society, vol. 506, no. 4, pp. 4735-4749. https://doi.org/10.1093/mnras/stab1940
Remote sensing of cometary bow shocks: Modelled asymmetric outgassing and pickup ion observations. / Alho, Markku; Järvinen, Riku; Simon Wedlund, Cyril; Nilsson, Hans; Kallio, Esa; Pulkkinen, Tuija.
In: Monthly Notices of the Royal Astronomical Society, Vol. 506, No. 4, 10.2021, p. 4735-4749.
T1 - Remote sensing of cometary bow shocks: Modelled asymmetric outgassing and pickup ion observations
AU - Alho, Markku
AU - Järvinen, Riku
AU - Simon Wedlund, Cyril
AU - Nilsson, Hans
AU - Kallio, Esa
AU - Pulkkinen, Tuija
N2 - Despite the long escort by the ESA Rosetta mission, direct observations of a fully developed bow shock around 67P/Churyumov–Gerasimenko have not been reported. Expanding on our previous work on indirect observations of a shock, we model the large-scale features in cometary pickup ions, and compare the results with the ESA Rosetta Plasma Consortium Ion Composition Analyser ion spectrometer measurements over the pre-perihelion portion of the escort phase. Using our hybrid plasma simulation, an empirical, asymmetric outgassing model for 67P, and varied interplanetary magnetic field (IMF) clock angles, we model the evolution of the large-scale plasma environment. We find that the subsolar bow shock standoff distance is enhanced by asymmetric outgassing with a factor of 2 to 3, reaching up to 18000km approaching perihelion. We find that distinct spectral features in simulated pickup ion distributions are present for simulations with shock-like structures, with the details of the spectral features depending on shock standoff distance, heliocentric distance, and IMF configuration. Asymmetric outgassing along with IMF clock angle is found to have a strong effect on the location of the spectral features, while the IMF clock angle causes no significant effect on the bow shock standoff distance. These dependences further complicate the interpretation of the ion observations made by Rosetta. Our data-model comparison shows that the large-scale cometary plasma environment can be probed by remote sensing the pickup ions, at least when the comet's activity is comparable to that of 67P, and the solar wind parameters are known.
AB - Despite the long escort by the ESA Rosetta mission, direct observations of a fully developed bow shock around 67P/Churyumov–Gerasimenko have not been reported. Expanding on our previous work on indirect observations of a shock, we model the large-scale features in cometary pickup ions, and compare the results with the ESA Rosetta Plasma Consortium Ion Composition Analyser ion spectrometer measurements over the pre-perihelion portion of the escort phase. Using our hybrid plasma simulation, an empirical, asymmetric outgassing model for 67P, and varied interplanetary magnetic field (IMF) clock angles, we model the evolution of the large-scale plasma environment. We find that the subsolar bow shock standoff distance is enhanced by asymmetric outgassing with a factor of 2 to 3, reaching up to 18000km approaching perihelion. We find that distinct spectral features in simulated pickup ion distributions are present for simulations with shock-like structures, with the details of the spectral features depending on shock standoff distance, heliocentric distance, and IMF configuration. Asymmetric outgassing along with IMF clock angle is found to have a strong effect on the location of the spectral features, while the IMF clock angle causes no significant effect on the bow shock standoff distance. These dependences further complicate the interpretation of the ion observations made by Rosetta. Our data-model comparison shows that the large-scale cometary plasma environment can be probed by remote sensing the pickup ions, at least when the comet's activity is comparable to that of 67P, and the solar wind parameters are known.
KW - plasmas
KW - shock waves
KW - methods: numerical
KW - techniques: miscellaneous
KW - comets: individual: 67P
U2 - 10.1093/mnras/stab1940
DO - 10.1093/mnras/stab1940
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
Alho M, Järvinen R, Simon Wedlund C, Nilsson H, Kallio E, Pulkkinen T. Remote sensing of cometary bow shocks: Modelled asymmetric outgassing and pickup ion observations. Monthly Notices of the Royal Astronomical Society. 2021 Oct;506(4):4735-4749. https://doi.org/10.1093/mnras/stab1940


Hidden Details You May Have Missed In The Marvel Movies
Additional Hidden Details You May Have Missed In The...
Every Marvel Cinematic Universe Antagonist, Ranked
Watch: New Fantastic Four Feature Trailer
http://www.wallpapersnewhd.com/the-fantastic-four-2015-movie-wallpaper-hd-free-download/#prettyPhoto Via wallpapersnewhd.com
'Spider-Verse' Director Hints at Identity of Main Villain in Potential Sequel
Comic Con may be over, but that doesn't mean there isn't more to watch and more to talk about. Following yesterday's Suicide Squad trailer release, here's the latest feature trailer for the new Fantastic Four movie.
The film stars Miles Teller, Michael B. Jordan, Kate Mara, Jamie Bell, Toby Kebbell, Reg E. Cathey and Tim Blake Nelson. It is directed by Josh Trank and will hopefully successful reboot the franchise that has been left in the dust since the Rise of The Silver Surfer sequel in 2007.
Wade Wilson has been writing for Goliath since 2015. By day, Wade Wilson discusses comics, movies, and video games and by night... he may or may not be Deadpool.
Robert Downey Jr. & Joe Rogan Discuss Marvel Movies, Iron Man's (Potential) Return & More
Additional Hidden Details You May Have Missed In The Marvel Movies


Talking about depressing website filing
nuprqmghhjdy by admin
himself is a small webmaster, very small kind of, from January 06 began doing web site. By the end of 05, I saw an article on the website making money in a computer magazine with a classmate in the dormitory. It was about how to make money with Google adsense.
freshman, learning web production, using FrontPage, will point special effects, such as text floating over, and so on, and now looks very bad. It's a static page, but at that time I thought it was written better than the others. See this Wangzhuan article, then interest way, just do it. I quickly went to the library to borrow some books, but it was still a static page. I made a website about tea during the vacation. Looking for free space everywhere, using a free two level domain name. Later, know what is dynamic web pages, learning the ASP, bought the space, will change all static into a static. I found the authority of a domain name, so I bought it.
, however, there is the filing problem. At that time, I had learned how to get a forum, found a free version of the mobile network, and made a community with my website. It is not for the record, then she went to the Ministry of information industry (now the Ministry) on the website for the record. The first one was smooth and I didn't submit the electronic bulletin board service. It was successfully passed a week later. But two weeks later, I found a better domain name, so the record had to be done again. But this time it is not so smooth, but it is also a station. This time it has been called electronic bulletin service, and it must go through the pre examination and approval procedures.
After consulting the process,
began to prepare, write materials and query relevant information. The filing was really long. Repeatedly submitted, have been hit back, or the main site may not bring news words, or the number of moderators is not enough, or may not open with the teaching of the section…… All sorts of reasons, I'll go instead. The second submission in August, 06, has dragged on for 07 years in January. At that time, I have to go through the record, or to shut down, or I can first shut down the forum, first "temporary" through…… At the time of the final examination, I had to take a compromise plan, which was closed for the time being.
, make full use of vacation time, look for a person to do moderators everywhere, want the copy of identity card of others…… Go to school, submit in 07 years in March. It was a long time, but it was a smooth pass, and got the cert file. By the end of June, told me that can get the material. Run to the communications authority, and tell me that the process is over here, and ask me to bring some of the materials they provide to the public security department for the record, so go ahead.
birthday is nothing, just ran the public security department, one-way ride two hours of public transportation, no money to play rental, that expensive…… Others this is called efficiency, go in and seat, but also pouring water, let me wait. Half an hour, a little, everything is done. Leave, this is called efficiency.
, this station is finally over. Later on >
Liverpool Lemar pursuit to go 'down to the wire'
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Grand Ole Opry officially welcomes Country Music Hall of Famer Bobby Bare
theadmin April 10, 2018
Photo Courtesy Grand Ole Opry, LLC. Chris Hollo, Photographer The Grand Ole Opry welcomed home Bobby Bare as an official…read more
Larry Gatlin returns to host Opry Country Classics
theadmin March 2, 2018
Season Kicks Off Tomorrow, March 1, with Spotlight on "The Songs of Johnny and June" on Couple's 50th Wedding Anniversary Country…read more
Jillian Jacqueline to make Grand Ole Opry debut February 13
theadmin February 7, 2018
Big Loud Records rising Country songstress JILLIAN JACQUELINE continues her high-profile performance streak with her Grand Ole Opry debut on…read more
Chris Janson, Craig Morgan, Trace Adkins, Dustin Lynch & more head to Grand Ole Opry in February
theadmin January 20, 2018
If you live in the Nashville, or are planning a trip to Nashville in February, take a look at what…read more
Exile kicks off 2018 celebration Of 55th Anniversary as special musical guest on Huckabee
Crossover hit-making band, Exile, is celebrating a distinguished career of 55 years as the longest running self-contained vocal group. This…read more
Chris Young reflects on remarkable year
theadmin December 21, 2017
The Grand Ole Opry's newest member wraps 2017 as surprise guest for Garth Brooks' sold-out show in Nashville Photo credit:…read more
Smith & Wesley to perform on Grand Ole Opry stage; Joining star-studded cast for Dr. Ralph Stanley Tribute
theadmin October 12, 2017
Smith & Wesley has enjoyed many firsts in the last year, including their first Top 25 single and music video…read more
William Michael Morgan launches title track single with renewed sense of self
theadmin October 4, 2017
Much has happened for William Michael Morgan since the release of his first single, "I Met A Girl," and the…read more
Josh Turner Celebrates 10 Years as a Member of the Grand Ole Opry
country September 21, 2017
Josh Turner (center) celebrates 10 years of Grand Ole Opry membership with friends and staff from the Opry, MCA Nashville…read more
Darius Rucker Celebrates 5 Years as a Member of the Grand Ole Opry
Darius Rucker Celebrates his 5 year Opry Anniversaryon September 20, 2017Darius Rucker Celebrates his 5 year Opry Anniversaryon September 20,…read more
'Miss Country Soul' Jeannie Seely Celebrates 50 Years As A Member of the Grand Ole Opry
Michael Guth, Chief Operating Officer, Opry Entertainment Group, Sally Williams, General Manager, Grand Ole Opry / Sr. Vice President, Programming…read more
The Marshall Tucker Band Returns to the Grand Ole Opry
country August 31, 2017
Legendary Southern Rock Group to Perform on Opry Stage on Tuesday, September 26On Tuesday, September 26, for the first time…read more


Rock the Kasbah (2015)
Rock the Kasbah DVD and Blu-ray release date was set for February 2, 2016.
Genre(s): Comedy, War, Music
Danny McBride
Scott Caan
Eugenia Kuzmina
Leem Lubany
Steve Bing
Bill Block
Rock the Kasbah is the story of a down and out music manager who takes off to Afghanistan with his last client on a last ditch effort to tour the country. Penniless, alone and desperate, the protagonist stumbles upon a new client. This time, he has found a young female star of the Afghan version of American Idol. This is the story of how he finds redemption in navigating the young star's career throughout the show.
Release Date February 2, 2016
I Heart Huckabees
Walk Hard: The Dewey Cox Story


NOISETTES AND MINUS THE BEAR INTIMATE SESSIONS ON LAST.FM ORIGINALS
Last.fm are showcasing a new feature that shines a light on original programming features and intimate artist experiences: Last.fm Originals.
The latest sessions on Last.fm Originals will be indie pop band the Noisettes who are about to release their next album 'Contact'.
They are a perfect fit for the Originals sessions, which will see the band perform an intimate set for Last.fm along with an exclusive interview. The Noisettes session is set to go live on August 27th 2012.
Following shortly after and proving Last.fm are diverse and on the pulse as ever, Seattle based alt-rockers Minus The Bear have recorded a very special sessions for music fans, which comes just in time for the release of their latest album 'Infinity Overhead', out September 3rd 2012.
last.fm/music/Noisettes
last.fm/music/Minus+the+Bear
WHAT'S ONFM RECOMMENDSINTERNETBEST NEW MUSICBEST NEW MUSIC


Rochelle News-Leader
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The word of the year
By: Chuck Roberts - Updated: 2 weeks ago
The English language is continually evolving. Words that meant one thing in the past have developed a new meaning now. Check this out: according to the new Cambridge Dictionary, the latest definition of a woman is: "an adult who lives and identifies as a female even though they may have been born as a different sex." Likewise a man is now "an adult who lives and identifies as a male even though they might have been born a different sex." It is interesting to note that the definition refers to a different sex, not the opposite sex suggesting that there are more than two sexes.
New meanings have developed for old words, like the adjective woke. I use to think of woke as a verb: I woke up tired this morning. A woke corporation is an entity that signals its support for progressive policies as a means of maintaining influence and signaling a form of virtue. Woke corporations typically support the leftist side of an issue. The word "woke capitalism" has often been attributed to an article by Ross Douthat in the New York Times in 2015, and the usage of this term has grown exponentially ever since.
But the winner-take-all for this year is the Merriam-Webster Dictionary word of the year: "gaslighting." Gaslighting has its origin in the 1938 English play, "Gaslight" by Patrick Hamilton, where a husband attempts to drive his wife crazy by distorting reality and slowly dimming the gaslights so he can declare her insane, commit her to an institution and collect her inheritance. The wife notices the dimming of the gaslights, but the husband leads her to believe that they are not fading so as to have her question her own sanity. According to Robin Stern, author of "The Gaslight Effect," gaslighting is, "the act of undermining another person's reality by denying facts, the environment around them, or their feelings." According to the American Psychological Association in the past, gaslighting is "manipulation so extreme as to induce mental illness or to justify commitment of the gaslighted person to a psychiatric institution." In recent years, the term, gaslighting, has expanded usage to mean essentially lying with a straight face. Those who participate in gaslighting are often pathological liars and display narcissistic tendencies. They are interested in gaining control over a group or over a particular discussion. Some examples of gaslighting phrases are: "That did not happen," "I never said that," "That's a lie," "You're nuts," "The border is secure," etc. You can often recognize a gaslighter by their need to impose their judgements on you; they feel they are always correct in their assertions; they are constantly complaining; they never accept responsibility; they are constantly calling you names; they say one thing and do another and are intimidating.
These words with new meanings are often put forth by the elite and powerful in our society to reinforce their elitism and perhaps control the conversation. When one of these elitists hits a person with a fancy word that they know nothing about, the listener usually doesn't respond since it is prudent not to talk about something you know nothing about. If clarification is asked of the elitist, a person often runs the risk of being declared an idiot. It may be prudent to just disengage from the conversation and obtain the clarification by other means.
Someday, these words will probably fade into oblivion much like the expression, "it's a Doozy" (referring to the fancy and unusual Duesenberg automobile) and "jeepers creepers" (an expression of surprise which came from the 1938 song by Louis Armstrong). New words or words with new meanings will most likely continue to appear.
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The English language is continually evolving. Words that meant one thing in the past have developed a new meaning now.
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