The Detection of Photospheric Impacts from Chromospheric Impulsive Events

Details The Detection of Photospheric Impacts from Chromospheric Impulsive Events The Detection of Photospheric Impacts from Chromospheric Impulsive Events

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003apj...589l.109m&link_type=abstract

The Astrophysical Journal, Volume 589, Issue 2, pp. L109-L112.

Astronomy and Astrophysics

Astronomy

Sun: Flares, Sun: Oscillations

Scientific paper

Multiwavelength solar observations were carried out at the THEMIS telescope in order to investigate the propagation of the plasma jets during and after a flare occurrence. The data obtained in the Hα, Na I D2, and Fe I 557.6 nm lines show that the perturbations detected in the higher layers due to a B-class flare do penetrate down to the photosphere. The observational evidence of such perturbations is crucial for the identification of the source of the solar oscillations.

Affiliated with

Also associated with

No associations

Rating

The Detection of Photospheric Impacts from Chromospheric Impulsive Events 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 The Detection of Photospheric Impacts from Chromospheric Impulsive Events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Detection of Photospheric Impacts from Chromospheric Impulsive Events will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1820559