12054 and 76215 - New measurements of interplanetary dust and solar flare fluxesThe mass distribution and flux of micrometeoroids, variations in solar activity, solar-wind erosion and solar-flare track production are discussed on the basis of lunar sample analyses. A bimodal size frequency distribution of micrometeorites is found; the ratio of the density of craters larger than 0.1 micron to the density of those larger than 500 microns is 50 to 100 million. Solar cosmic-ray track ages determined for the lunar samples through use of the model of Blanford et al. (1975) indicate no variation in solar activity over a period of 2 million years. Solar wind erosion is set at no more than 0.03 A per year.
Document ID
19780057697
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Morrison, D. A. (NASA Johnson Space Center Houston, Tex., United States)
Zinner, E. (Washington University St. Louis, Mo., United States)