Coronal dimming observed with Hinode

Details Coronal dimming observed with Hinode Coronal dimming observed with Hinode

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.6305h&link_type=abstract

American Astronomical Society Meeting 210, #63.05; Bulletin of the American Astronomical Society, Vol. 39, p.172

Astronomy and Astrophysics

Astronomy

Scientific paper

Coronal dimming has been a technique used to determine the source of plasma that forms part of a coronal mass ejection. Generally dimming is detected through imaging instruments such as SOHO EIT by taking difference images. In a few cases the SOHO-CDS has been used to determine outflowing material, and a decrease in density. Hinode tracked active region 10930 from which there were a series of flares. We combine dimming observations from EIT with Hinode data to show the impact of flares and coronal mass ejections on the region surrounding the flaring active region, and we discuss evidence that the eruption resulted in a prolonged steady outflow of material from the corona.

Affiliated with

Also associated with

No associations

Rating

Coronal dimming observed with Hinode 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 Coronal dimming observed with Hinode, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coronal dimming observed with Hinode will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1031260