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作業: 40%專題報告(口頭&書面): 20% (預定日期: 12/30)進度報告(含值週報告&上課表現): 20%上課筆記(手寫一張A4) + 個人書面報告: 20%
繳交日期: 1/10中午前
108-1 日地環境物理 國立中央大學 太空科學與工程研究所 楊雅惠
評分方式:
課程網址: http://www.ss.ncu.edu.tw/~yhyang/108-1/st
上課方式:
版書 + 投影片2hr講課&討論 + 1hr實作&報告
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Solar magneto-hydrodynamics, Eric R. Priest, D. ReidelPublishing Company, 1984.
The solar-terrestrial environment : an introduction to geospace--the science of the terrestrial upper atmosphere, ionosphere, and magnetosphere, J.K. Hargreaves, Cambridge University Press, 1992.
Interplanetary magnetohydrodynamics, L.F. Burlaga, Oxford University Press, 1995.
Introduction to Space Physics, M. G. Kivelson and C. T. Russell, Cambridge University Press, 1995.
Physics of the Space Environment, Tamas I. Gombosi, Cambridge University Press, 1998.
Physics of Space Plasmas: An Introduction, G. K. Parks, Westview Press, 2004.
參考用書:
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Real Time Solar Wind:http://www.swpc.noaa.gov/products/real-time-solar-windhttp://www.swpc.noaa.gov/products/ace-real-time-solar-wind
Space Weather:https://www.ngdc.noaa.gov/stp/mag_pause/http://spaceweather.kma.go.kr/en/current.dohttp://eng.sepc.ac.cn/MBS.phphttp://ccmc.gsfc.nasa.gov/cgi-bin/display/RT_t.cgi
Solar Monitor: http://solarmonitor.org/Helioviewer: https://www.helioviewer.org/SolarHam: http://www.solarham.net/
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日地環境
行星際空間
太陽
地球
http://g-ecx.images-amazon.com/images/G/01/askville/74139061_answers/1306272473581_magnetosphererendition.jpg
磁層
日地距: 1 AU (天文單位) ~ 1.50x108 km太陽半徑: 1 Rs ~ 6.96x105 km ~ 0.005 AU 地球半徑: 1 Re ~ 6.37x103 km ~ 0.009 Rs
~ 100~ 110
Bow shock modelMagnetopause model
Tsyganenko modelGeomagnetic indices
High speed solar windInterplanetary shock
Magnetic cloud………
Solar flareCoronal mass ejection (CME)
Coronal hole
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http://lasp.colorado.edu/reu/docs/solar_wind.jtgosling.ppt
n is proton density, Vsw is solar wind speed, B is magnetic field strength, A(He) is He++/H+ ratio, Tp is proton temperature, Te is electron temperature, T is alpha particle temperature, Cs is sound speed, CA is Alfven speed.
The Sun yearly loses ~6.8 x 1019 g to the solar wind, a very small fraction of the total solar mass of ~2 x 1033 g.
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https://www.cfa.harvard.edu/~scranmer/ITC/eaaa_solar_wind_schwenn.pdf
any others?
Geo-effectiveness?
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Coordinated Data Analysis Web (CDAWeb):http://cdaweb.gsfc.nasa.gov/istp_public/
SPDF-Satellite Situation Center Web (SSCWeb):http://sscweb.gsfc.nasa.gov/cgi-bin/Locator_graphics.cgi
SOHO LASCO CME CATALOG:http://cdaw.gsfc.nasa.gov/CME_list/
World Data Center for Geomagnetism, Kyoto:http://wdc.kugi.kyoto-u.ac.jp/wdc/Sec3.html
OMNI Data Documentation:http://omniweb.gsfc.nasa.gov/html/HROdocum.html(http://omniweb.gsfc.nasa.gov/ftpbrowser/bow_derivation.html)
Interplanetary Shocks:https://www.cfa.harvard.edu/shocks/
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Solar Wind Speed during 2007-2018
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http://www.swpc.noaa.gov/products/solar-cycle-progression
Solar Cycle 24
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http://spaceweather.com/archive.php?view=1&day=29&month=08&year=2019
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http://www.swpc.noaa.gov/products/real-time-solar-wind
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http://spaceweather.com/archive.php?view=1&day=29&month=08&year=2019