Title of article
Shape and Location of Planetary Bow Shocks
Author/Authors
Kotova، G. A. نويسنده , , Verigin، M. I. نويسنده , , Remizov، N. M. Shutter A. P. نويسنده , , Rosenbauer، H. نويسنده , , Riedler، W. نويسنده , , Schwmgenschuh، K. نويسنده , , Szego، K. نويسنده , , Tatrallyay، M. نويسنده , , Styazhkm، V. A. نويسنده , , Shutte، N. M. نويسنده , , Zhang، T.-L. نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 1999
Pages
-33
From page
34
To page
0
Abstract
We developed a semiempirical quantitative model of a planetary bow shock, which describes variations in its location and shape caused by variations in parameters of the solar wind flow and in the shape of the obstacle (magnetopause). Based on this model, we explore the near-Mars bow shock, the experimental data of which were obtained on the Phobos-2 spacecraft. Unusual properties of near-Mars bow shock are analyzed.
Keywords
GFRP , Sandwich beams , Localised effects , Nomex , High-order sandwich beam theory , Surface displacement analysis , Indentation
Journal title
COSMIC RESEARCH (TR)
Serial Year
1999
Journal title
COSMIC RESEARCH (TR)
Record number
5940
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