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Determination of solar wind elemental abundances from M/Q observations during three periods in 1980
Authors:S. Kunz  P. Bochsler  J. Geiss  K. W. Ogilvie  M. A. Coplan
Affiliation:1. Physikalisches Institut, Universit?t Bern, Sidlerstrasse 5, CH 3012, Bern, Switzerland
2. NASA Goddard Space Flight Center, 20771, Greenbelt, MD, USA
3. Institute of Physical Science and Technology, University of Maryland, 20742, College Park, MD, USA
Abstract:Mass spectra in the range 2 ≦ M/Q ≦ 3 provided by a high resolution mode of the ISEE-3 Plasma Composition Experiment were evaluated for three selected periods during early 1980. The observed Ne/O ratios are compatible with estimated solar abundance ratios. In two of the three periods, the He/Ne-ratios agree with the Apollo foil results. Freezing-in temperatures for oxygen are similar to those obtained by other groups. Possible reasons for an unexpectedly high flux at M/Q = 2.4 are discussed.
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