Radar interferometric studies of comets

Details Radar interferometric studies of comets Radar interferometric studies of comets

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991plas.rept..113s&link_type=abstract

In NASA, Washington, Reports of Planetary Astronomy, 1991 p 113-114 (SEE N92-12792 03-89)

Astronomy and Astrophysics

Astronomy

Chemical Composition, Comet Nuclei, Cometary Atmospheres, Cyanoacetylene, Hydrocyanic Acid, Interferometry, Radio Interferometers, Velocity Distribution, Very Large Array (Vla), Antenna Arrays, Austin Comet, Brorsen-Metcalf Comet, Excitation, Masers, Millimeter Waves, Plasma Interactions

Scientific paper

Our objectives are to use radio interferometry to study composition, velocity distribution, maser excitation, and plasma interactions of cometary gas. Two new cometary chemistry programs were started with radio interferometers: (1) the VLA used to search for HC3N emission from Comet Brorsen-Metcalf at 3.3 cm wavelength; and (2) the BIMA millimeter array used to observe Comet Austin in HCN.

Affiliated with

Also associated with

No associations

Rating

Radar interferometric studies of comets 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 Radar interferometric studies of comets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radar interferometric studies of comets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1876958