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chromosphere

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Images

  • line profile which corresponds well to the true centerline profile that we see with the Rakuljic filter Figure 1c The scattered skylight has been subtracted from all the profiles shown Fig 3 Left Limb profiles from three filtergrams obtained with our Zeiss filter in the continuum at H alpha 13 22A solid line at H alpha 0 7A dotted line and
  • to decrease when we approach the sunspot minimum going from 1 August 1994 to 7 September 1995 We do not know if this is a true effect but will monitor it in the future Fig 9 The frequency of macrospicules reaching higher than 7000 Km as a function of position angle The counted numbers are normalized to 150 arcsec intervals The increased
  • gas that emits light in that color It is normally not visible because of the overwhelming brightness of the photosphere but the chromosphere can be seen during a total solar eclipse Image courtesy of National Solar Observatory
  • WHIDDON CHROMOSPHERE S jpg
  • chromosphere composite jpg
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  • as the height of the H alpha chromosphere The disk level is for the slope measure defined as the brightness averaged over a ten arcsec wide interval just inside the photospheric limb Fig 6 Definition of the height measures used in the paper Top The e fold measure is defined as the distance between the photospheric limb and the point where the limb
  • Chromosphere by Sqny Chromosphere by Sqny Masterful use of lines colors and sounds I ve seen lots of prods that do OK at capturing a theme and delivering it in a cohesive way but Chromosphere makes most look
  • Full View Start your own free art collection Sign up here Share This Blog It Available in the Shop Buy This Print Download Send to Mobile Also chromosphere s profile chromosphere s gallery
  • Four other views Zeeman Effect The Corona Traditional Solar Eclipse The Corona Four more views Temperature and Density Structure above the Photosphere
  • galaxies RA 09h 55 5m Dec +69°20 approx centre M81 and M82 in Ursa Major are two of the brightest members of the M81 group of galaxies M81 often called Bode s Nebula after being discovered by Johann Elert Bode in 1774 is a large bright
  • Solar granulation Solar granulation movie Solar Chromosphere Solar Corona
  • The Solar Chromosphere The chromosphere of the Sun is a thin transitional layer between the photosphere and the corona It s thickness is about 8000 km 5000 miles and is comparable to the shell of
  • nebulae RA 05h 35m 17s Dec 5°23 28 The Orion Nebula M42 NGC 1976 M43 is located in the sword of Orion and is a large emission nebula that is easily visible to the *** eye It is an area of star formation the
  • Wort after boil and a short rest
  • sunspot1 jpg
  • recipes Had a successful I think effort at recovering the yeast from a bottle of Fuller s 1845 so now to use it in a version of London Pride from Wheeler and Protz s Brew Your Own British Real
  • but also a lengthy one You do this because you absolutely love it And just to drive home the point that I am not a graphic artist here is the art I made in about 10 minutes in the GIMP Concept Art for Chromosphere
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  • 40 x 40 acrylic on canvas from the Heat of the Moment series $2800 plus gst
  • Chromosphere Prominences at contact II The ephemeral and transitory appearance of the solar chromosphere thin red horizontal layer between the photosphere and the corona surrounded by prominences is captured in this time
  • ar 050515 1049 0035c > 24 Mar 2009 10 32 138k chromosphere t275 jpg 24 Mar 2009 10 32 65k chromosphere t400 jpg 24 Mar 2009 10 32 47k comp101704 jpg 24 Mar 2009 10 32 105k
  • auslöser manuell gemacht während der Totalität wurden die Aufnahmen vom Laptop ferngesteuert Kurz vor dem dritten Kontakt habe ich dann wieder auf manuelle Kontrolle umgeschaltet
  • instead of the average to avoid the influence of sudden short jumps in height due to small scale chromospheric structure This is especially important for the slope measure Fig 8 The chromospheric height in centerline H alpha for 5 days during 1994 and 1995 as a function of position angle according to a the e fold measure and b the slope
  • use the median instead of the average to avoid the influence of sudden short jumps in height due to small scale chromospheric structure This is especially important for the slope measure Fig 8 The chromospheric height in centerline H alpha for 5 days during 1994 and 1995 as a function of position angle according to a the e fold measure and b the
  • Solar Chromosphere
  • A two image composite showing the afore mentioned active regions in a short exposure and a quiescent prominence in a long exposure The two were then blended together in Photoshop A rather unique image of the solar chromosphere in a region where there are no active regions or strong magnetic fields shaping the chromosphere itself Essentially one is looking down onto
  • nebulae RA 06h 41m Dec +9°53 The Cone Nebula and Christmas Tree Cluster are part of a larger star forming complex within the constellation of Monoceros A 2 5 hour exposure in H Alpha light taken 22nd December 2006
  • from Kelling Heath at the 2007 Spring Star Party on an excellent night after we had been fogged out for the previous two nights I m hoping to go again this year to do some more imaging In the region of M81 and M82 and across large parts of the northern sky there is a large faint nebular complex associated with dust and gas expelled from the plane of the galaxy The region
  • I observed this 55 000 mile high prominence during International Astronomy Day May 2 2009 my 55th birthday Here is a small bit of placid chromosphere May 2 2009 Little Big Man 90mm Coronado Solarmax and Astro Physics f5 Stowaway refractor imaged with the DMK41AF02 camera ©
  • kawamura chromosphere jpg
  • Snímek v rozlišení 1024x768 pixelů
  • Saturn chapter 5 The solar chromosphere chapter 6 Download
  • reed bunting m jpg
  • Chromosphere at 2nd Contact
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  • landsat great lakes jpg 16 Sep 2000 20 26 81k ocean currents jpg 16 Sep 2000 20 28 79k chromosphere gif 16 Sep 2000 20 21 78k rad at earth gif 16 Sep 2000 20 30 77k
  • Full disc mosaic of the Sun in H alpha emission Full disc image of the chromosphere and lower corona in H alpha Posted in
  • ar10656prom081804 jpg 24 Mar 2009 10 32 178k ar 050515 1049 0035c > 24 Mar 2009 10 32 138k chromosphere t275 jpg 24 Mar 2009 10 32 65k chromosphere t400 jpg 24 Mar 2009 10 32 47k
  • chromosphere jpg

Videos

  • Chromosphere Extreme While viewing the activity within Active Region NOAA 10953 a roller coaster ride comes to mind. Enjoy the ride as it twist and turns across the plage and white flashes of light called "Ellerman Bombs" explode all around. Now hold on tight as this filament abruptly lifts off the surface only to reverse its direction and quickly plunge into the depths of the Sun. SolarIMAX-style movies @
  • Amazing Solar Videos - The Sun Song Lyrics Below. Videos from various orbiting space observatories set to the music of Astrocapella - The Chromatics' The Sun Song. Including the latest videos from 2010! There are flares, CME's (coronal mass ejections), comets magnetic fields, sunspots, and Jupiter. HINODE (Solar-B): solarb.msfc.nasa.gov TRACE: STEREO: stereo.gsfc.nasa.gov SOHO (amazing site!): sohowww.nascom.nasa.gov CASSINI (end titles): saturn.jpl.nasa.gov Astrocappella: Lyrics - Astrocappella: The Sun Song Music and Lyrics by Karen Smale Our star, the Sun is a big ball of gas And it's 99 percent of our solar system's mass It's an average star in our Milky Way Warming the Earth every day What powers our Sun and makes it so bright? Come on and tell me, what makes all that light? Hans Bethe long ago reached the conclusion It changes Hydrogen to Helium by nuclear fusion When fusion takes place light is created And it makes its way out (although rather belated) Through the Photosphere that's the part that we see The light comes out and shines on you and me About a million Earths could fit in the Sun But if you were there you wouldn't have much fun It's six thousand degrees at the photosphere And much hotter inside the solar atmosphere There are a few places where it's not so hot Like at the center of a big sunspot But heat is relative it's still pretty warm Sitting on a sunspot would do you great harm Galileo discovered sunspots What are those things, those funny dots ...
  • chromosphere (total solar eclipse)2 taken in Yichang China at 0925 on 22072009
  • Sun-Chromosphere.avi Video of the solar chromosphere as imaged using a 12" Meade LX200, the Meade Electronic Eyepiece, and an H-Alpha filter. Unfortunately, the wind was insane the day the video was taken.
  • Hinode Spacecraft Captures Total Solar Eclipse Hinode captured a total eclipse in orbit on 19th March 2007, while it was just a partial eclipse on the ground. These data are used to measure scatterd light of telescopes. X-ray Telescope (XRT) obtained full disk images during the total eclipse in soft X-ray images. Hinode (Sunrise in Japanese), formerly known as Solar-B, is a Japan Aerospace Exploration Agency Solar mission with United States and United Kingdom collaboration. --- It's Never too Late to Study --- Notice This video is copyright by its respectful owners. The website address on the video does not mean anything. ---
  • Sun hot gas fountains Sun hot gas fountains captured at the Sun's south pole, caused by the Alfvén waves in the sun chromosphere. Video recorded by Hinode.
  • Chromosphere (aka silverf*cking around) While I was writing this song I realized it sounded like Pumpkins' Silver*** interlude and a bit like Starla so I didn't felt like using it on any demo or give it any importance but I liked the song so I played with it while recording it and even used the lyrics for the mentioned part. I used Windows Player images as I thought they were great for the psicodelic vibrations of the song. So,the whole song is my kind of tribute to the Pumpkins but the real tribute starts at 01:57 and ends at 02:25
  • Sun chromosphere on december 2006 Sun chromosphere on december 2006. Solar activity. Video release by SOHO.
  • Solar Flare
  • SQNY - CHROMOSPHERE
  • nasa/jaxa - solar flare in chromosphere video 2 solar flare in chromosphere, recorded by JAXA's Hinode spacecraft
  • Chromosphere - MIchelle Chromosphere is the solo project of Digital Poodle and Kinder Atom alumnus Kris Helstrom. Often tightly packed with special guests, Chromosphere is an electro-forum for odd, and sometimes not so odd, musical ideas. Experimental and urbane improvisations jammed loosely over oozing break-beats most easily describes the sound from within the Chromosphere. The third full-length release "Universal Quintessence" is now being released electronically as three EPs from Paper+Sound. Video directed by Heiki Sillaste
  • What's Up for March 2011? Through special solar-safe telescope filters, you can see sunspots on the sun. If you see any large sunspot groups, try to observe them over several days. You may be able to see them march across the sun's photosphere as our star rotates. Flares that explode and prominences that sometimes erupt into space from the sun can be seen with special H-alpha filters. These special narrow-band filters isolate only the hydrogen alpha wavelength. This filter blocks all the other color of light and reveals the sun's chromosphere. You can learn more about Sun-Earth Day events and hands-on activities at solarsystem.nasa.gov/yss, which stands for Year of the Solar System. And you can learn all about NASA missions at www.nasa.gov Read more on www.nasa.gov
  • Dave Robbins - New Age; Chromosphere.mov Good laid back stuff or to relax anytime.
  • Biosphere - Chromosphere from "Microgravity"
  • chromosphere (total solar eclipse)3 taken in Yichang China at 0925 on 22072009
  • Coronal Streamer Model of the Chromosphere and Corona using FLIP3D-MHD ( The chromosphere remains unperturbed in the left end while an arcade is formed by reconneciton and jets of matter and energy are developing towards the right.
  • Solar Chromosphere Explore the Plage, {pronounced: 'pläzh}, surrounding active region NOAA 10930. Plage is the brighter region surounding the SunSpot and is caused by light emitted from clouds of calcium or hydrogen. SolarIMAX-style movies @
  • The Lord of the Rings--{song replaced}--[was Into the West] One of the first few AMVs that I've made using WMM. It's not the best 'cause I used screen shots (captures) instead of the actual movie clips. Edit: Music had to be switched because of Third party claiming the rights to the song I used. To those who really liked this video, I'm sorry. There was nothing else I could do but fix the problem. The new song is called "Goodbye" by Chromosphere. Hope you enjoy it :D . Forgive me if this video gives you a headache. I know the screen shots go by kinda fast but that's how I ended up making it. ^_^; Sorry again. Rate and comment please :D . {Screen Shots/Captures credited to Arwen-} THIS VIDEO IS PURELY FAN-MADE AND IS IN NO WAY ASSOCIATED WITH THE MUSICAL ARTIST OR ANIME/MOVIE COMPANY IN ANY WAY.
  • Physical Science 10.2c - The Structure of the Sun The Structure of the Sun. From the Physical Science course by Derek Owens.
  • Chapter 10B Chromosphere Corona Heliosphere Intro to Astronomy Chapter_10B Chromosphere Corona Heliosphere
  • Chromosphere by SQNY 1st at Stream 2007 Find out more at
  • Our Solar System - The Sun - Solar Flares - The atmosphere of the sun consists of several layers called the photosphere, chromosphere, transition region and corona. The photosphere is the lowest layer and the visible surface of the sun we see. The corona is the outer layer which produces flares and solar winds.
  • YOU - Mummy Wrapped In Love (demo) in a bit of a rush to put this up... ...wrote it on the plane.... words: chromosphere through clouds sheds new colors above the clouds the water looks like land the cloth and clocks are ticking divergent shapes and texture of life mummy wrapped in love smooth and light mountain formation swirling blades of organic strips of steak inside my mouth landscape of the next level mummy wrapped in love chromosphere and clouds shed their new colors mummy wrapped inside of love the distant horizon layers the cloth and clocks unwinding a new light spectrum is unfolding my mummy wrapped inside of love the end of depth is not visible a bead of geometrical.... a mummy wrapped inside of love ADDITIONAL INFO: Obviously about Mother Earth.... ;) And, this hottie from astronomy class at COA with a bangin' body... phew... gonna be on the 2020 vision release (later this year).... Website is switching servers....till I start working on it again...
  • Eddie Halliwell - Winnipeg (September 28, 2007) Eddie Halliwell live @ EEC in Winnipeg Track: Kobbe - Chromosphere ((Thx to bnbkl & techaddict03)) LQF
  • Chromosphere Alessandro Bianconi (Rome).avi Chromospere PST40 + Barlow Apo 2x + DMK031
  • 31 January 2010 Solar Vortex in Chromosphere
  • nasa/jaxa - solar flare in chromosphere video 1 solar flare in chromosphere, recorded by JAXA's Hinode spacecraft
  • SQNY - Chromosphere (Final) Authors: SQNY Compo: Combined demo Awards: 1st place at Stream 2007 awards: Most original concept
  • Cloudland Ballroom - "Chromosphere" Experiment with old-school ***og video feedback. Visuals and soundtrack by James R. Moore (Cloudland Ballroom).
  • Solar Active Region's Farewell Blast (Part 1)- A Trifecta (Flare, Prominence and CME) - Just as sunspot group AR11105 rotated out of the Earth's view it produced a spectacular show. A large prominence erupted along with a C3 solar flare and a Coronal Mass Ejection (CME) blasted away from the sun. This great show was captured by the Solar Dynamics Observatory (SDO) as well as the Solar and Heliospheric Observatory (SOHO) and the Solar Terrestrial Relations Observatory's (STEREO) Ahead spacecraft. This video first shows the 193 Angstrom coronal line, which corresponds to temperatures around ~1.5 million Kelvin and is produced by super heated iron. There is a brightening from the flare and hot loops after the flare but the darker, cooler prominence can also be seen. In the background the curved structure that is the beginning of the CME (coronal mass ejection) is visible. The second part of the video in the cooler 304 Angstrom emission line produced by super heated helium. The cooler chromospheric material making up the prominence is bright in this line around 60000 to 80000 Kelvin. The cross-like patterns are caused when the light produced by the flare and post-flare loops saturates the camera's CCD. Just like when a bright light causes a streak in a digital camera. (Credit SDO, LMSAL and )
  • sun chromosphere The chromosphere
  • SDO AIA M2.0 Solar Flare from Emerging Active Region 1081 beta on 2010-06-12 An M2.0 solar flare as captured in extreme ultraviolet Iron ion lines in the chromosphere (and corona) of the sun. Courtesy of SDO (NASA) and the [AIA, EVE, and/or AIA] consortium, with which I have no association.
  • September Goes Out with a Great Solar Prominence - September 30, 2010 - Around 22 UT on the last day of September 2010 a large prominence erupted on the northwest limb (upper right) of the Sun. The eruption was observed with great detail by the Solar Dynamics Observatory's Atmospheric Imaging Assembly (SDO/AIA). Prominences are composed of hot plasma (ionized gas) from the sun's chromosphere. The material has a temperature of around 60000 Kelvin. This temperature of solar material is best observed with the 304 Å wavelength filter on AIA. This movie shows the 304 Å wavelength images, first showing most of the solar disk and then zooming in on the prominence. This extreme ultraviolet light comes from singly ionized Helium, or He II. At its largest extent the prominence rises above the solar surface a distance equivalent to 30-40 earth stacked end-to-end. A coronal mass ejection (CME) associated with the eruption was observed by LASCO aboard the SOHO spacecraft. (credit: Solar Dynamics Observatory and )
  • NASA Solar Flare video A solar flare is a violent explosion in a star's (like the Sun's) atmosphere releasing up to a total energy of 6 × 1025 Joules.[1] Solar flares take place in the solar corona and chromosphere, heating plasma to tens of millions of kelvins and accelerating electrons, protons and heavier ions to near the speed of light. They produce electromagnetic radiation across the electromagnetic spectrum at all wavelengths from long-wave radio to the shortest wavelength gamma rays.[2] Most flares occur in active regions around sunspots, where intense magnetic fields emerge from the Sun's surface into the corona. Flares are powered by the sudden (timescales of minutes to tens of minutes) release of magnetic energy stored in the corona. X-rays and UV radiation emitted by solar flares can affect Earth's ionosphere and disrupt long-range radio communications. Direct radio emission at decimetric wavelengths may disturb operation of radars and other devices operating at these frequencies. Solar flares were first observed on the Sun in by Carrington and independently by Hodgson in 1859 as localized brightenings in a sunspot group. Stellar flares have also been observed on a variety of other stars. The frequency of occurrence of solar flares varies, from several per day when the Sun is particularly "active" to less than one each week when the Sun is "quiet". Large flares are less frequent than smaller ones. Solar activity varies with an 11-year cycle (the solar cycle). At the peak of the ...
  • more DVD doodles - solar spectrum Hovering the camera above the DVD with sunlight skimming across the disk surface shows dark absorption lines originating in the solar chromosphere eg sun's atmosphere. See also my video Warning/disclaimer included.
  • The Sun on July 6, 2010 NOAA active regions 11084 and 11086 located at mid-latitudes in the chromosphere.
  • Barbican - Chromosphere
  • Chromosphere by SQNY PC demo by SQNY that won the demo comp at Stream 2007
  • Comet crashed into Sun 3D STEREO This is the comet and its tail as observed by NASA's twin STEREO spacecraft between March 12 and 14, 2010. The left side is STEREO B (orbiting behind the Earth) and the right is STEREO A (ahead). The outer images are from Cor2, the middle ones are from Cor1 and the inner ones of the solar disk are from the EUVI instruments onboard STEREO. (NASA. UC Berkeley) Based on the comet's relatively short tail, about 3 million kilometers in length, the researchers believe that the comet contained heavier elements that do not evaporate readily. This would also explain how it penetrated so deeply into the chromosphere, surviving the strong solar wind as well as the extreme temperatures Credits: www.berkeley.edu
  • 2. Total Solar Eclipse Shanghai 22 July 2009 The Total Solar Eclipsed 22 - 7 - 2009 Dishui Lake - Shanghai - China. To all eclipse chasers everywhere on Earth! Despite cloud, one a half minute of totality captured with the video camera this year. A really glorious chromosphere and an amazing second diamond ring that I feel so lucky being there! After four minutes of totality I realized that the exposure settings on the camera were totally wrong to capture the corona through clouds! I replaced this lost time with the best shots of my friends during totality. Hope clear skies next time!
  • chromosphere (total solar eclipse)1 taken in YiChang China at 0925 on 22072009