Edited time lapse sequences of the sun’s atmosphere observed by the Solar Dynamics Observatory spacecraft between 2011 and 2015. Music: Una by Murcof Taken form the Album Utopía (2004) | CD: BAY38 CD, Digital: BAY38 E http://www.theleaflabel.com/en/releases/view/98/murcof/utopia Images courtesy of: NASA’s Goddard Space Flight Center, Scientific Visualization Studio www.nasa.gov/centers/goddard | http://sdo.gsfc.nasa.gov Editing: Michael König | http://www.koenigm.com Additionally EARTH is now provided in Full HD: https://vimeo.com/32001208 This montage features excerpts of 4K full-disk pictures in extreme ultraviolet channels, mainly using wavelengths of 30.4 nm (50,000 Kelvin) partially in combination with 17.1 nm (6.3×105 Kelvin), and offers a glance at spicules, solar flares, filaments and an overview of the sun’s atmosphere. The footage was captured by the Atmospheric Imaging Assembly (AIA) maintained by the Joint Science Operations Center (Lockheed Martin Solar and Astrophysics Laboratory in collaboration with Stanford University) Scenes in order of appearance: 1. Long shots of solar activity | October 2013 2. Boiling solar prominence | February 2013 3. Close up active regions | October 2013 4. Launching filament | November 2011 5. Twisting prominence | September 2012 6. Close up solar activity | October 2014 7. Solar prominence | July 2013 8. Lunar transit | January 2014 9. Solar prominence dance | December 2012 10. Solar activity | October 2013 11. Plasma eruption | September 2012 12. Coronal rain | July 2012 13. Close up active regions | October 2013 14. Trebuchet eruption | February 2011 15. Solar prominence | October 2013 16. Venus transit | June 2012 17. Extreme solar eruption | June 2011 18. Filament eruption & ’canyon of fire’ | September 2013 19. Erupting solar filament | March 2015 20. Comet ’lovejoy’ passes sun | December 2011 21. Earth eclipse and dark prominence | September 2012 More information on the Solar Dynamics Observatory mission: http://en.wikipedia.org/wiki/Solar_Dynamics_Observatory
Apr
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