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The Dangers of Solar Storms and Solar Cycles Radius = 696,000 km Mass = 2E30 kg Luminosity = 3.8E26 W Rotation Rate 25 days at the equator and 30 days at the poles Surface Temp 5,800 K average, 4,000 K sunspots (Ref 1) Nuclear fusion is the source of all the energy released by the sun Steady fusion rates maintain a steady luminosity Hydrogen fusion is the primary mechanism ▪ P-P chain ▪ CNO cycle (Content: Ref 13) (Image: Ref 10) For every 1 million atoms of hydrogen in the entire sun 98,000 atoms of helium 850 of oxygen 360 of carbon 120 of neon 110 of nitrogen 40 of magnesium 35 of silicon 35 of iron (Content: Ref 13) (Image: Ref 11) Plasma Gas whose temperature is so hot it becomes sensitive to magnetism Ionized due to high temperatures Most energy is lost to electromagnetic radiation Visible light Infrared (Ref 13) Particle radiation also emits energy Flares and coronal mass ejections release intense concentrations of energetic particles Hazardous to astronauts in orbit and satellites (Content: Ref 13) (Image: Ref 12) 1. 2. 3. 4. Bennett, Jeffery, Donahue, Megan, Schneider, Nicholas, Voit, Mark, The Cosmic Perspective, 2007 Pearson Education Inc, San Franscisco CA, p.477-496 Pacella, Rena Marie. “Anatomy of a Solar Storm.” Popular Science. May 2007. <http://www.popsci.com/popsci/aviationspace/7250d257d5ed2110vgn vcm1000004eecbccdrcrd.html>. Phillips, Tony. “Solar Storm Warning.” NASA. 15 March, 2006. 9 October, 2007. <http://www.nasa.gov/vision/universe/solarsystem/10mar_stormwarni ng.html >. “SOHO Fact Sheet.” European Space Agency. 30 June, 2003. 4 December, 2007. <http://sohowww.nascom.nasa.gov/about/docs/SOHO_Fact_Sheet.p df>. 5. 6. 7. 8. Phillips, Tony. “Solar Storm Warning.” NASA. 15 March, 2006. 9 October, 2007. <http://www.nasa.gov/vision/universe/solarsystem/10mar_stormwarni ng.html>. Odenwald, Sten. “Solar Storms.” Washington Post. 10 March, 1999. 17 25-Sep-2007 October, 2007. <http://solar.physics.montana.edu/press/WashPost/Horizon/196l031099-idx.html>. “STEREO - Solar TErrestrial RElations Observatory.” NASA. 25 September, 2007. 4 December, 2007. <http://stereo.gsfc.nasa.gov/img/mpb.pdf>. Roth, M. “Future missions for helioseismology.” Modern Solar Facilities – Advanced Solar Science, 85–88. 4 December, 2007. <http://www.mps.mpg.de/projects/seismo/papers/goe_roth.pdf>. 9. 10. 11. 12. 13. Phillips, Tony PhD “Who’s Afraid of a Solar Flare?” NASA Science. October 2005. <http://science.nasa.gov/headlines/y2005/07oct_afraid.htm>. http://atropos.as.arizona.edu/aiz/teaching/a250/pp.html http://webusers.astro.umn.edu/~larry/CLASS/AST2001/pre2007/massi 25-Sep-2007 ve_star_struct.jpg http://www.space.com/scienceastronomy/soho_top10_winners_03112 5-2.html http://www.nasa.gov/worldbook/sun_worldbook.html#backToTop