Ultraviolet Spectropolarimetry of Comet Mueller Split of 4549 -- Cycle 3 Medium

Details Ultraviolet Spectropolarimetry of Comet Mueller Split of 4549 -- Cycle 3 Medium Ultraviolet Spectropolarimetry of Comet Mueller Split of 4549 -- Cycle 3 Medium

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.5296s&link_type=abstract

HST Proposal ID #5296

Physics

Hst Proposal Id #5296

Scientific paper

Spectropolarimetric observations will be made of comet WKI over a wide range in phase angle, as well as comet Encke at high phase. The observations will be used to investigate the light scattering properties of cometary dust grains as a function of scattering angle and wavelength. These data can be compared to models and laboratory measurements of various materials to help determine their physical and chemical nature. These data will be free of contamination by molecular emission. Furthermore, the relation between the polarization and phase angle of the molecular bands, which differs from that of the grains, can be determined. These data will can be used to help correct future broad-band polarization measurements, and to provide additional information about the importance of fluorescence to the production of the various emission bands. After failure of first observations, additional ACQ image added and target changed to comet Mueller (1993p).

Affiliated with

Also associated with

No associations

Rating

Ultraviolet Spectropolarimetry of Comet Mueller Split of 4549 -- Cycle 3 Medium 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 Ultraviolet Spectropolarimetry of Comet Mueller Split of 4549 -- Cycle 3 Medium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet Spectropolarimetry of Comet Mueller Split of 4549 -- Cycle 3 Medium will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1071894