Physics
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.2512b&link_type=abstract
American Astronomical Society Meeting 210, #25.12; Bulletin of the American Astronomical Society, Vol. 39, p.133
Physics
Scientific paper
We present an analysis of the spectral emission of Fe XIII between 195 and 210 Å. The Fe XIII lines in this wavelength range are sensitive indicators of plasma density below about 1012 cm-3. Thus solar spectra obtained using the Cosmic Hot Interstellar Plasma Spectrometer (CHIPS) and the EUV Imaging Spectrometer on Hinode, which both cover this wavelength region with high spectral resolution, provide information on the plasma density. In order to test emission models used in the analysis of these observations, we performed high-resolution laboratory measurements at a density of about 1012 cm-3. The laboratory data thus test the calculations at their astrophysically high-density limit. A comparison to model calculations based on the CHIANTI data base showed excellent.
This work was supported in part by NASA's Solar and Heliospheric Physics Supporting Research and Technology Program.
Beiersdorfer Peter
Hurwitz Margaret M.
Lepson J. K.
No associations
LandOfFree
Laboratory Measurement And Modeling Of The Fe XIII Emission In The Extreme Ultraviolet Near 200 Å 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 Laboratory Measurement And Modeling Of The Fe XIII Emission In The Extreme Ultraviolet Near 200 Å, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Laboratory Measurement And Modeling Of The Fe XIII Emission In The Extreme Ultraviolet Near 200 Å will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1029495