Astronomy and Astrophysics – Astronomy
Scientific paper
May 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.3203g&link_type=abstract
American Astronomical Society, 194th AAS Meeting, #32.03; Bulletin of the American Astronomical Society, Vol. 31, p.870
Astronomy and Astrophysics
Astronomy
Scientific paper
Polar coronal rays/plumes as long lived structures that extend out to 6 R_sun were first observed during the first flight of SPARTAN 201 spacecraft during April 11-12 of 1993. In this paper we will present detail observations from the WLC aboard Spartan 201 spacecraft (31 Oct.- 2 Nov.,1998) of the north polar coronal hole and comapre its physical properties to the past three Spartan missions. We will present comparisons of the Spartan WL observations with the Mk3 pB observations, SOHO LASCO and EIT observations, and finally the high resolution TRACE 171 Angstroms observations, to characterize the north polar coronal hole all the way from the base of the corona out to 30 R_sun. We will also look for signatures of waves (quasi-period variations) in the coronal hole plumes and interplume regions in the high cadence Spartan pB observations obtained during this mission.
DeForest Craig
Fisher Richard Royal
Gibson Steven
Guhathakurta Madhulika
Kucera Therese
No associations
LandOfFree
Temporal Evolution and Physical Properties of North Polar Coronal Hole from SPARTAN 201-05, SOHO, TRACE and Mk3 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 and Physical Properties of North Polar Coronal Hole from SPARTAN 201-05, SOHO, TRACE and Mk3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Temporal Evolution and Physical Properties of North Polar Coronal Hole from SPARTAN 201-05, SOHO, TRACE and Mk3 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1120194