Influence of the Solar Activity Cycle on the Gasdynamic Structure of the Heliospheric Interface

Details Influence of the Solar Activity Cycle on the Gasdynamic Structure of the Heliospheric Interface Influence of the Solar Activity Cycle on the Gasdynamic Structure of the Heliospheric Interface

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ap%26ss.274..149z&link_type=abstract

Astrophysics and Space Science, v. 274, Issue 1/2, p. 149-156 (2000).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The effects of the 11 year solar activity cycle on the heliospheric plasma interface in the presence of neutral H-atoms have been investigated. Our calculations show that nonstationary processes of such kind lead to1) a decrease of the mean interstellar plasma density in the interface;2) a sequence of shocks and rarefaction waves moving from the heliopause (HP)to the bow shock (BS); 3) an expansion of the region between the BS and HP;4) the TS excursion along the upwind direction is within 30%of the mean solar distance.

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