Temporal evolution of the chromospheric electron density in the flare of January 5, 1992

Details Temporal evolution of the chromospheric electron density in the flare of January 5, 1992 Temporal evolution of the chromospheric electron density in the flare of January 5, 1992

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..160...29r&link_type=abstract

Solar Physics, Volume 160, Issue 1, pp.29-40

Physics

5

Scientific paper

The analysis of the dynamic evolution of the chromospheric electron density during solar flares is fundamental for the testing of solar flare models. For this purpose we developed a digital imaging spectrograph for the observation of higher Balmer lines below 400 nm with a time resolution of 1 s and an algorithm for the determination of the electron density from the observed line profiles. On January 5, 1992 a M1/1N flare was observed in Hα, H∈ and Ca ii H and the temporal evolution of the electron density was determined. The chromospheric electron density rises several times from less than 3 × 1019 to 1 × 1020 m-3 during the hard X-ray peaks.

Affiliated with

Also associated with

No associations

Rating

Temporal evolution of the chromospheric electron density in the flare of January 5, 1992 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 Temporal evolution of the chromospheric electron density in the flare of January 5, 1992, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Temporal evolution of the chromospheric electron density in the flare of January 5, 1992 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1568036