Visibility of the photospheric granulation in Fe I at 6569.2 A

Details Visibility of the photospheric granulation in Fe I at 6569.2 A Visibility of the photospheric granulation in Fe I at 6569.2 A

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...45...35l&link_type=abstract

Solar Physics, vol. 45, Nov. 1975, p. 35-40.

Physics

2

Iron, Photosphere, Solar Granulation, Solar Spectra, Astronomical Photography, Line Spectra, Solar Limb

Scientific paper

High-quality photographs of the granulation obtained at seven wavelengths in the Fe I line at 6569.2 A are presented. The granule contrast attains a maximum considerably exceeding the continuum value around Fe + 0.05 to Fe + 0.10 A; individual granules remain easily visible to within 5 sec of the limb. Only remnants of the granulation pattern are discernible at the line center.

Affiliated with

Also associated with

No associations

Rating

Visibility of the photospheric granulation in Fe I at 6569.2 A 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 Visibility of the photospheric granulation in Fe I at 6569.2 A, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Visibility of the photospheric granulation in Fe I at 6569.2 A will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1377776