Remote sensing of inner heliospheric plasmas

Details Remote sensing of inner heliospheric plasmas Remote sensing of inner heliospheric plasmas

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ucsd.rept.....j&link_type=abstract

Final Technical Report, 15 Nov. 1990 - 14 Nov. 1993 California Univ., San Diego, La Jolla.

Other

Heliosphere, Photometers, Remote Sensing, Solar Corona, Solar Flares, Solar Wind, Stellar Mass Ejection, Helios Satellites, Solar Activity Effects, Solar Terrestrial Interactions, Spacecraft Instruments, Zodiacal Light

Scientific paper

Solar disturbances produce major effects on the corona, the solar wind, the interplanetary medium, and the earth along with its magnetosphere. We have developed new techniques for studying plasma disturbances in the inner heliosphere by remotely sensing them. These techniques use data from the HELIOS spacecraft zodiacal light photometers and in situ data, the ISEE-3 spacecraft in situ and kilometer radio wave experiments, and a variety of other spacecraft and ground-based instruments. We use interplanetary scintillation (IPS) data from the Cambridge, England, radio telescope. The zodiacal-light photometers on board the two HELIOS spacecraft (data coverage from 1974 to 1986) provide the first reliable information about the heliospheric masses and shapes of propagating disturbances.

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