SPACE WEATHER - AGI

Section III: Thermal Effects6. References© SSS Educational Series 2012[1] Williams, D. Sun Fact Sheet. 2004 [cited 2010 May 12]; Available from:http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html.[2] Eddy, J.A. A New Sun: The Solar Results from Skylab. 1979 [cited 2011 May 7];Available from: http://history.nasa.gov/SP-402/contents.htm.[3] Smirnov, B.M., Plasma Processes and Plasma Kinetics. Electrophoresis,2007(7883744296578191625related:CRGO-aqvaG0J).[4] Maalouf, M., M. Durante, and N. Foray, Biological effects of space radiation onhuman cells: history, advances and outcomes. Journal of radiation research, 2011.52(21436608): p. 126-46.[5] Basu, S., Helioseismology and solar abundances. Physics Reports,2008(3553695456915610782related:ntxflTBDUTEJ).[6] Doormann, V., SOLAR SYSTEM GEOMETRIES AND TERRESTRIAL CLIMATE.volker-doormann.org, 2010(related:8eIJdxXsVPYJ).[7] Clark, S., Sun's fickle heart may leave us cold. New Scientist, 2007.[8] Hathaway, D. Solar Physics. 2007 [cited 2011 May 14]; Available from:http://solarscience.msfc.nasa.gov/feature1.shtml.[9] Hassler, D.M., et al., Solar wind outflow and the chromospheric magneticnetwork. Science, 1999(3889806379195337319related:Z4r89Epe-zUJ).[10] Sahraoui, F., M.L. Goldstein, and P. Robert, A, Evidence of a cascade anddissipation of solar-wind turbulence at the electron gyroscale. Physical review letters,2009(18168762412411035511related:d5864CZpJPwJ).[11] Broggini, C., Nuclear processes at solar energy. Arxiv preprint astro-ph,2003(8677295430675503475related:c5mITDjya3gJ).[12] Brokaw, R.S., Approximate formulas for the viscosity and thermal conductivity ofgas mixtures. The Journal of Chemical Physics, 1958 (10584108522416325608related:6EPPxp9O4pIJ).[13] Orrall, F.Q., The Coefficient of Thermal Conductivity in the Sun's Atmosphere.The Astrophysical Journal, 1961(6645977447091387690related:Kr0jt0ZBO1wJ).[14] Bekhti‚ M., Temperature effects on satellite power systems performance.‚European conference of systems, 2010(related:IO8F2VPSRr0J).30