Computer Science
Scientific paper
Jun 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977cosp.meets....d&link_type=abstract
COSPAR, Plenary Meeting, 20th, Tel Aviv, Israel, June 7-18, 1977, Paper. 11 p. Centre National d'Etudes Spatiales
Computer Science
Energy Distribution, Interplanetary Medium, Shock Wave Propagation, Solar Activity Effects, Solar Flares, Solar Wind, Energy Transfer, Magnetic Flux, Pioneer 10 Space Probe, Pioneer 9 Space Probe, Solar Magnetic Field, Stellar Mass Ejection, Type 2 Bursts
Scientific paper
The shape of solar flares-associated shock waves on August 1972 was studied by comparing the solar plasma observations on Prognoz, Prognoz-2, Pioneer-9 and Pioneer-10 spacecraft with type II radioburst observations and observations of radio source scintillations. This study showed that the first shocks were almost spherical and displayed strong deceleration (blast waves). Two subsequent shocks were highly nonspherical with low deceleration (piston-driven waves). Energy and mass-ejected quantities obtained from Prognoz-2 measurements are 10 to the 32nd-10 to the 33rd ergs and 10 to the 16th-10 to the 17th g, respectively.
Bosqued Jean Michel
Duston C.
Temnyi V. V.
Zastenker Georgy N.
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