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 ,
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
