Sodium-line emission in flares and source position relative to magnetic fields

Details Sodium-line emission in flares and source position relative to magnetic fields Sodium-line emission in flares and source position relative to magnetic fields

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..201c&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 48, June 1977, p. 201-211. In Italian.

Physics

Optics

Magnetic Field Configurations, Sodium, Solar Flares, Solar Instruments, Solar Magnetic Field, Astronomical Photography, Electromagnetic Wave Filters, Filtergrams, Light Curve, Magneto-Optics, Polarimeters, Solar Spectra

Scientific paper

The paper reviews the technology and results of the sodium D-line observation of solar flares and the position of the source with respect to magnetic field structure. A magnetooptical filter for obtaining D-line spectrograms is described, which operates in three modes. Consideration is then given to characteristic aspects of flare observation, with emphasis placed on light curves and the sequence of flare photography. Ways in which the obtained filtergrams can be used to study the magnetic field structure in an active region are discussed.

Affiliated with

Also associated with

No associations

Rating

Sodium-line emission in flares and source position relative to magnetic fields 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 Sodium-line emission in flares and source position relative to magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sodium-line emission in flares and source position relative to magnetic fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1596451