Analysis of a sequence of energetic ion and magnetic field events upstream from the Saturnian magnetosphere

Author:

Krimigis S.M.,Sergis N.,Dialynas K.,Mitchell D.G.,Hamilton D.C.,Krupp N.,Dougherty M.,Sarris E.T.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference32 articles.

1. Orientation, location, and velocity of Saturn's bow shock: Initial results from the Cassini spacecraft;Achilleos;J. Geophys. Res.,2006

2. Anagnostopoulos, G., Sarris, E.T., Krimigis, S.M., 1986. Magnetospheric origin of energetic (E⩾50keV) ions upstream of the bow shock: The October 31, 1977 event, J. Geophys. Res. 91, 3020–3028.

3. Modeling the size and shape of Saturn's magnetopause with variable dynamic pressure;Arridge;J. Geophys. Res.,2006

4. Outward flow of protons from the Earth's bow shock;Asbridge;J. Geophys. Res.,1968

5. Low frequency waves and associated energetic ions downstream of Saturn;Behannon;J. Geophys. Res.,1985

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