Fe XIII Density Diagnostics in the EIS Observing Wavelengths

Details Fe XIII Density Diagnostics in the EIS Observing Wavelengths Fe XIII Density Diagnostics in the EIS Observing Wavelengths

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009apj...692.1294w&link_type=abstract

The Astrophysical Journal, Volume 692, Issue 2, pp. 1294-1304 (2009).

Astronomy and Astrophysics

Astronomy

15

Atomic Processes, Line: Formation, Sun: Corona, Sun: Flares, Sun: Uv Radiation

Scientific paper

The diagnostic capability of Fe XIII line features seen in the 170-210 Å waveband of the EUV Imaging Spectrometer (EIS) on Hinode is investigated, with emphasis on density diagnostics applied to solar active regions. Four diagnostic line pairs are found to yield consistent densities ranging from 108.5 to 109.5 cm-3 across an active region using a new theoretical model of the ion. In separate EIS observations of a small flare, the widely used line pair, Fe XIII λ203.8/λ202.0, is found to reach the high density limit predicted by a new theoretical model of the iron ion.

Affiliated with

Also associated with

No associations

Rating

Fe XIII Density Diagnostics in the EIS Observing Wavelengths 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 Fe XIII Density Diagnostics in the EIS Observing Wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fe XIII Density Diagnostics in the EIS Observing Wavelengths will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-836944