The Near-Infrared Coronal Spectrum

Details The Near-Infrared Coronal Spectrum The Near-Infrared Coronal Spectrum

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...456l..67k&link_type=abstract

Astrophysical Journal Letters v.456, p.L67

Astronomy and Astrophysics

Astronomy

15

Sun: Corona, Sun: Infrared, Line: Identification

Scientific paper

Sensitive measurements of the near-infrared coronal spectrum were obtained from the 1994 total solar eclipse. A new [S IX] emission line at 1.25249 +/- 0.00003 mu m has been detected, and a bright, potentially important diagnostic, [Si X] line at 1.43 mu m has been confirmed. Upper limits on the intensity of several other predicted IR emission lines have been established. Also, diffuse He I emission, perhaps geocoronal, has been observed with a significant heliocentric redshift.

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