Steady-state and dynamical features of the electron density distribution in the solar corona emerge from a preliminary analysis of Helios A electron content measurements. There are strong indications that correlations can be established with earth-bound K-coronagraph measurements.
Preliminary analysis of coronal electron content measurements from spacecraft Helios A around first solar occultation
1977-01-01
Miscellaneous
No indication
English
NTRS | 1970
|Tema Archive | 1976
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