A High-Temperature Component in Coronal Holes as Confirmed by a Partial-Eclipse Observation

Details A High-Temperature Component in Coronal Holes as Confirmed by a Partial-Eclipse Observation A High-Temperature Component in Coronal Holes as Confirmed by a Partial-Eclipse Observation

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pasj...49..413h&link_type=abstract

Publications of the Astronomical Society of Japan, v.49, p.413-417.

Astronomy and Astrophysics

Astronomy

4

Sun: Corona, Sun: Coronal Hole, Sun: X-Rays

Scientific paper

We confirmed X-ray signals in coronal holes based upon a Yohkoh soft X-ray observation of a partial eclipse on 1993 November 13. The observed X-ray signals cannot be explained by those coming from one-million-degree plasmas alone, which were observed with the Skylab UV and EUV instruments. This suggests that higher-temperature plasmas are necessary to explain the present observation.

Affiliated with

Also associated with

No associations

Rating

A High-Temperature Component in Coronal Holes as Confirmed by a Partial-Eclipse Observation 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 A High-Temperature Component in Coronal Holes as Confirmed by a Partial-Eclipse Observation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A High-Temperature Component in Coronal Holes as Confirmed by a Partial-Eclipse Observation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1478432