Anticipated Voyager crossing of the termination shock
Author:
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://www.agu.org/journals/gl/v027/i011/2000GL003748/2000GL003748.pdf
Reference23 articles.
1. Motion of the heliospheric termination shock: A gasdynamic model;Barnes;J. Geophys. Res.,1993
2. Solar wind conditions in the outer heliosphere and the distance to the termination shock;Belcher;J. Geophys. Res.,1993
3. Distance to the solar wind termination shock and the source flux of anomalous cosmic rays during 1986-1988;Cummings;J. Geophys. Res.,1994
4. Implication of a weak termination shock;Fisk;Space Sci. Rev.,1996
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1. IMPACT OF PICKUP IONS ON THE SHOCK FRONT NONSTATIONARITY AND ENERGY DISSIPATION OF THE HELIOSPHERIC TERMINATION SHOCK: TWO-DIMENSIONAL FULL PARTICLE SIMULATIONS AND COMPARISON WITHVOYAGER 2OBSERVATIONS;The Astrophysical Journal;2015-08-05
2. SYSTEMATIC INVESTIGATION OF SOLAR MODULATION OF GALACTIC PROTONS FOR SOLAR CYCLE 23 USING A MONTE CARLO APPROACH WITH PARTICLE DRIFT EFFECTS AND LATITUDINAL DEPENDENCE;The Astrophysical Journal;2012-01-10
3. Two sides of the heliopause;Science China Earth Sciences;2011-10-15
4. THE TERMINATION SHOCK MAY HAVE A BOW-SHAPED OPEN GEOMETRY;The Astrophysical Journal;2011-01-13
5. Cosmic rays in the dynamic heliosheath;Advances in Space Research;2008-01
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