An alternative analysis of low- and high-altitude observations of ring current ions during a storm recovery phase

Details An alternative analysis of low- and high-altitude observations of ring current ions during a storm recovery phase An alternative analysis of low- and high-altitude observations of ring current ions during a storm recovery phase

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jgr....82.2367l&link_type=abstract

Journal of Geophysical Research, vol. 82, June 1, 1977, p. 2367-2370.

Computer Science

Sound

1

Ionospheric Sounding, Magnetic Storms, Proton Energy, Ring Currents, Satellite Observation, Explorer Satellites, Geomagnetism, Helium Ions, Hydrogen Atoms, Hydrogen Ions, Ionospheric Storms, Oxygen Ions, Pitch (Inclination), Proton Precipitation

Scientific paper

Explorer 45 equatorial observations of ring current ions during a storm recovery phase have shown pitch angle distributions and decay rates inconsistent with proton charge exchange with neutral hydrogen. This inconsistency has led to the suggestion that recovery phase ring current ions at L less than or equal to 4 and energies not greater than 50 keV are dominated by He(+) rather than protons. The absence of He(+) on flux tubes from which H(+) and O(+) were precipitating in ion mass spectrometer measurements made during the same period by the low-altitude polar-orbiting satellite 1971-089A led Sharp et al. to suggest a source of H(+) and O(+) to L = 3 during this period. An alternative explanation, in which the magnetic field lines labeled L = 3 at the earth's surface near local midnight were mapped to about 3.7 earth radii in the equatorial plane during the storm recovery phase and during the period of enhanced activity, is proposed. If the proposed explanation is correct, the observations of Sharp et al. are not incompatible with the conclusion that the recovery phase ions at less than 50 keV were dominated by He(+) for L not greater than 3.7.

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