The colour of the solar corona and dust grains in it

Details The colour of the solar corona and dust grains in it The colour of the solar corona and dust grains in it

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...65..171a&link_type=abstract

Solar Physics, vol. 65, Feb. 1980, p. 171-179.

Physics

2

Astronomical Photometry, Colorimetry, Dust, Solar Corona, Color

Scientific paper

The paper examines the photometry of coronal color negatives and determines the distribution of the coronal brightness in the red, green, and blue wavelength intervals up to distances of 6-7 solar radii. A correlation between the color indexes and diffuse external reinforcement brightness (RED) is indicated, and the results show that RED consists of dust grains with radii of at least 1 micron. It is concluded that the whole dust mass of RED is at least 1% of the coronal mass within the RED region, and the dust grain number density is about 10 to the -11th power/cu cm.

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