PHYSICAL CONSEQUENCES FROM AXISYMMETRICAL MODEL OF THE SOLAR-WIND INTERACTION WITH SUPERSONIC INTERSTELLAR GAS-FLOWстатья
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Дата последнего поиска статьи во внешних источниках: 18 июля 2013 г.
Аннотация:Effects of the local interstellar medium (LISM) ionization degree and the interstellar magnetic field on position and shape of termination shock (TS), heliopause (HP) and bow shock (BS) are considered on the basis of Baranov and Malama /1/ and Baranov and Zaitsev /2/ models. Difference of plasma and H-atoms parameters distribution in up-wind and down-wind directions is analyzed. Some predictions of future experimental results obtained by means of spacecraft are given.