Characteristics of upstream energetic (E≥50 keV) ion events during intense geomagnetic activity

Journal of Geophysical Research: Space Physics

Volumn 103, Issue A5, 1998, Pages 9521-9533

  Anagnostopoulos, G C ^a  

^a DEMOCRITUS UNIVERSITY OF THRACE   (Greece)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000103077     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article

References (3)

1. Anagnostopoulos, G. C., The inverse velocity dispersion of the upstream ions as a result of the magnetospheric activity, in Proceedings of the First Panhellenic Astronomical Meeting, p. 333-338, P. G. Laskarides, Athens, 1993.
2. Anagnostopoulos G. C., On the role of the solar flare generated ions in producing the energetic (E ≥ 300 keV) ion events observed upstream from the Earth's bow shock, Adv. Space Res., 15(8/9), 63, 1995.
3. Anagnostopoulos, G. C., and G. D. Kaliabetsos, Shock drift acceleration of energetic (E ≥ 50 keV) protons and (≥37 keV) alpha particles at the Earth's bow shock as a source of the magnetosheath energetic proton events, J. Geophys. Res., 99, 2335, 1994.