Study of the brightness distribution across spicules from observations of the spicule occultation by the moon at the partial solar eclipse

Details Study of the brightness distribution across spicules from observations of the spicule occultation by the moon at the partial solar eclipse Study of the brightness distribution across spicules from observations of the spicule occultation by the moon at the partial solar eclipse

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...79..323a&link_type=abstract

Solar Physics, vol. 79, Aug. 1982, p. 323-326.

Physics

7

Brightness Distribution, Lunar Occultation, Spicules, Solar Eclipses

Scientific paper

Cinematographic observation of the spicule occultation by the Moon
have been carried out at the partial solar eclipse of October 2, 1978.
The relative brightness distribution across a spicule in the light of
Hα + 0.8 Å is first obtained. The diameter values for two
spicules have been found to be of 280 ± 40 km and 1200 km.

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