Comment on ‘Energetic heavy ions observed upstream of the Earth's bow shock by the STEP/EPACT instrument on WIND’ by G. M. Mason, J. E. Mazur, and T. T. Von Rosenvinge
Author:
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://www.agu.org/journals/gl/v025/i009/98GL00989/98GL00989.pdf
Reference7 articles.
1. Characteristics of upstream energetic (E≥50 keV) ion events during intense geomagnetic activity;Anagnostopoulos;J. Geophys. Res.,1998
2. On the role of the solar flare generated ions in producing the energetic (E≥300 keV) ions events observed upstream from the Earth's bow shock;Anagnostopoulos;Adv. Space Res.,1995
3. Dominant acceleration processes of energetic protons at the Earth's bow shock;Anagnostopoulos;Phys. Scripta,1994
4. «Comment on «Magnetospheric origin of energetic (E≥50 keV) ions upstream of the bow shock: The October 31, 1977, event» by G.C.Anagnostopoulos, E.T. Sarris, and S.M. Krimigis;Ellison;J. Geophys. Res.,1987
5. Energetic heavy ions observed upstream from the Earth's bow shock by the STEP' EPACT instrument on WIND;Mason;Goephys. Res. Lett.,1996
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1. Upstream ion events with hard energy spectra: Lessons for their origin from a comparative statistical study (ACE/Geotail);Planetary and Space Science;2013-09
2. On the origin of the energetic ion events measured upstream of the Earth's bow shock by STEREO, Cluster, and Geotail;Journal of Geophysical Research: Space Physics;2011-02
3. Evidence and features of magnetospheric particle leakage on days 30–36, 1995: Wind, Geotail, and IMP 8 observations compared;Journal of Geophysical Research;2005
4. Characteristics of energetic (≳30 keV/nucleon) ions observed by the Wind/STEP instrument upstream of the Earth's bow shock;Journal of Geophysical Research: Space Physics;2000-01-01
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