Physics
Scientific paper
Mar 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..343g&link_type=abstract
In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:
Physics
2
Coronal Holes: Outflows
Scientific paper
This paper presents an attempt to evaluate the use below 1.5 R0 of the Doppler Dimming method, pioneered by the UVCS/SOHO team, who use it at larger radial distances. Following Noci et al. (1987), the theoretical model for this process has been reevaluated, incorporating some of the more recent atomic and solar data. The model is applied to data from SUMER that was recorded above the limb in a classical polar coronal hole, during the solar minimum in May 1996. This 2-dimensional raster is capable of resolving the solar plumes. The interpretation is shown to be critically dependent on the assumed density and spatial homogeneity.
Bely-Dubau Francoise
David Claire
Gabriel Alan H.
No associations
LandOfFree
The determination of coronal hole outflow velocities below 1.5 R0 using the "Doppler Dimming" technique with the SUMER instrument on SOHO 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 The determination of coronal hole outflow velocities below 1.5 R0 using the "Doppler Dimming" technique with the SUMER instrument on SOHO, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The determination of coronal hole outflow velocities below 1.5 R0 using the "Doppler Dimming" technique with the SUMER instrument on SOHO will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-780280