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Comparison of MHD simulation for the February 1986 events with interplanetary observations by the spacecraft SakigakeDuring the period 3-10 February 1986 a series of major solar flares occurred on the Sun and several intense geomagnetic storms took place on the Earth. To examine the causality between the solar activity and the geomagnetic activity in this period, a magnetohydrodynamic (MHD) numerical simulation was performed using a 2 1/2 -D numerical code. In that period of February 1986, the Japanese spacecraft Sakigake was at 0.84 AU, 57 deg west of the Earth. Besides the in-situ measurements of the interplanetary plasma, Sakigake also provided Doppler scintillation observations. Comparisons between the results of the MHD simulation and the measurements made by the spacecraft Sakigake are presented.
Document ID
19880001340
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Smith, Z.
(National Oceanic and Atmospheric Administration Boulder, CO., United States)
Yeh, T.
(Colorado Univ. Boulder., United States)
Dryer, M.
(National Oceanic and Atmospheric Administration Boulder, CO., United States)
Watanabe, T.
(Nagoya Univ. Toyokawa (Japan), United States)
Oyama, K.
(Tokyo Univ. Japan)
Date Acquired
September 5, 2013
Publication Date
September 14, 1987
Publication Information
Publication: Alabama Univ., Huntsville. STIP Symposium on Physical Interpretation of Solar(Interplanetary and Cometary Intervals
Subject Category
Solar Physics
Accession Number
88N10722
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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