Correction for the observed intensity distribution in solar corona

Details Correction for the observed intensity distribution in solar corona Correction for the observed intensity distribution in solar corona

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984basi...12..190a&link_type=abstract

Astronomical Society of India, Bulletin, vol. 12, June 1984, p. 190-195.

Astronomy and Astrophysics

Astrophysics

1

Atmospheric Turbulence, Solar Corona, Solar Eclipses, Solar Flux Density, Photographic Emulsions

Scientific paper

A modification to the method proposed by Abhyanakr and Subrahmanyam (1982) to correct for atmospheric-turbulence, emulsion-scattering, and focusing-error broadening effects in intensity profiles from solar-corona observations is presented. The calculated intensity distributions near the north, south, east, and west limbs are plotted along with observations obtained at the Raichur station of the Indian Institute of Astrophysics during the total eclipse of February 16, 1980. The spread of the observed intensity distributions is found to lie between 3 and 4 arcsec.

Affiliated with

Also associated with

No associations

Rating

Correction for the observed intensity distribution in solar corona does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Correction for the observed intensity distribution in solar corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Correction for the observed intensity distribution in solar corona will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1853355