Identification of Low-Latitude Coronal Plumes in Extreme-Ultraviolet Spectroheliograms

Details Identification of Low-Latitude Coronal Plumes in Extreme-Ultraviolet Spectroheliograms Identification of Low-Latitude Coronal Plumes in Extreme-Ultraviolet Spectroheliograms

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...446l..51w&link_type=abstract

Astrophysical Journal Letters v.446, p.L51

Astronomy and Astrophysics

Astronomy

13

Sun: Corona, Sun: Magnetic Fields, Sun: Solar Wind, Sun: Uv Radiation

Scientific paper

Using Skylab extreme ultraviolet images of the solar disk, we have identified plumelike features inside low-latitude coronal holes undergoing limb passage. Like their polar counterparts, these diffuse Mg IX structures are located above enhancements in the weak neon and helium background emission within the coronal hole. We conclude that coronal plumes are not unique to the polar regions but may occur in open magnetic regions at any latitude.

Affiliated with

Also associated with

No associations

Rating

Identification of Low-Latitude Coronal Plumes in Extreme-Ultraviolet Spectroheliograms 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 Identification of Low-Latitude Coronal Plumes in Extreme-Ultraviolet Spectroheliograms, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Identification of Low-Latitude Coronal Plumes in Extreme-Ultraviolet Spectroheliograms will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1202885