The solar coronal green line as an index of cosmic ray modulation

Details The solar coronal green line as an index of cosmic ray modulation The solar coronal green line as an index of cosmic ray modulation

Oct 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973p%26ss...21.1661p&link_type=abstract

Planetary and Space Science, Volume 21, Issue 10, p. 1661-1670.

Physics

1

Scientific paper

In recent years several papers have indicated that the solar coronal green line emission (λ=5303 Å) is the `best' indicator of cosmic ray modulation. This paper questions this result for the following reasons: (a) the problems of green line measurement obscure the true meaning of the resulting observations; (b) there is a lack of any direct physical mechanism relating green line intensity and modulation; (c) a negative result came from a careful attempt to relate the cosmic ray diurnal variation and green line emission.

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