Simultaneous Hα and sodium observations at the Kanzelhöhe Solar Observatory

Details Simultaneous Hα and sodium observations at the Kanzelhöhe Solar Observatory Simultaneous Hα and sodium observations at the Kanzelhöhe Solar Observatory

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..147m&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Physics

Solar Flares, Sodium Lines, Hα

Scientific paper

At the Kanzelhöhe Solar Observatory, Hα images are currently obtained simultaneously with sets of intensity, velocity and longitudinal magnetic images in the sodium D lines. Many flares have been detected. The preliminary results of the analysis suggest the events to occur at heights in the solar atmosphere below 1100 km, where the canopy magnetic lines stressed by the photospheric motions can reconnect. The penetration of the downflowing plasma jets is investigated in order to justify the solar background in the photospheric intensity-velocity phase spectrum.

Affiliated with

Also associated with

No associations

Rating

Simultaneous Hα and sodium observations at the Kanzelhöhe Solar Observatory 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 Simultaneous Hα and sodium observations at the Kanzelhöhe Solar Observatory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simultaneous Hα and sodium observations at the Kanzelhöhe Solar Observatory will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-780108