Published September 15, 1981
| Version v1
Journal article
Identification of new solar OH lines in the 10--12 micron region
- 1. Department of Physics, University of Denver
Description
High-resolution (0.02 cm-1) infrared solar spectra obtained with a balloon-borne interferometer reveal new solar absorption features, which appear as regularly spaced quartets, in the 825--960 cm-1 region. The lines are interpreted as high N'' (25--33) pure rotation lines of solar OH. An effective amount of approx.8 x 1015 molecules cm-2 of OH is estimated from the spectra
Additional details
Publishing Information
- Journal Title
- Astrophys. J., Lett. Ed.
- Journal Volume
- 248
- Journal Issue
- 3
- Series
- Astrophys. J., Lett. Ed.
- Journal Page Range
- L133-L135
- ISSN
- 0571-7248
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 13652070
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- HYDROXIDES; INFRARED SPECTRA; SPECTROSCOPY; SUN
- Descriptors DEC
- HYDROGEN COMPOUNDS; MAIN SEQUENCE STARS; OXYGEN COMPOUNDS; SPECTRA; STARS