Comet Austin (1989c1) O(1D) and H2O production rates

Details Comet Austin (1989c1) O(1D) and H2O production rates Comet Austin (1989c1) O(1D) and H2O production rates

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992icar...96..190s&link_type=abstract

Icarus (ISSN 0019-1035), vol. 96, no. 2, April 1992, p. 190-197. Research supported by University of Wisconsin and National Sola

Astronomy and Astrophysics

Astronomy

13

Austin Comet, Fabry-Perot Spectrometers, Oxygen Spectra, Sky Surveys (Astronomy), Water, Photodissociation, Spectral Resolution, Telluric Lines, Ultraviolet Astronomy

Scientific paper

The dual-etalon Fabry-Perot spectrometer of Kitt Peak's McMath solar telescope has been used to conduct Comet Austin observations with spectral scan resolutions of 0.21 A; this sufficed for resolution of cometary forbidden O I 6300 A emissions from nearby NH2, as well as telluric emissions of the same type. For these data, an O(1D) production rate is obtained which is noted to be nearly model-independent. The H2O production rate is determined by taking into account the photodissociation of H2O and OH as sources of O(1D).

Affiliated with

Also associated with

No associations

Rating

Comet Austin (1989c1) O(1D) and H2O production rates 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 Comet Austin (1989c1) O(1D) and H2O production rates, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comet Austin (1989c1) O(1D) and H2O production rates will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1736716