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

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:

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/

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

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.

https://www.cfa.harvard.edu/~scranmer/ITC/eaaa_solar_wind_schwenn.pdf

any others?

Geo-effectiveness?

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/

Solar Wind Speed during 2007-2018

http://www.swpc.noaa.gov/products/solar-cycle-progression

Solar Cycle 24

http://spaceweather.com/archive.php?view=1&day=29&month=08&year=2019

http://www.swpc.noaa.gov/products/real-time-solar-wind

http://spaceweather.com/archive.php?view=1&day=29&month=08&year=2019