Observation of 38-334-keV Interplanetary Protons during Solar Quiet Times

Details Observation of 38-334-keV Interplanetary Protons during Solar Quiet Times Observation of 38-334-keV Interplanetary Protons during Solar Quiet Times

Nov 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973phrvl..31.1268l&link_type=abstract

Physical Review Letters, vol. 31, Issue 20, pp. 1268-1271

Physics

3

Scientific paper

We present the first observations of quiet-time interplanetary protons in the energy range 38 to 334 keV from the Apollo 16 subsatellite. These proton fluxes vary by a factor of ~ 5 over a six-month period. Their spectrum can be represented by a power law dJdE=5.6E-1.3 (cm2 sec ster keV)-1 from 38 to 334 keV during May 1972.

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