On the wavelength dependence of apparent emissivity of asteroid microwave emissions - Ceres and Vesta

Details On the wavelength dependence of apparent emissivity of asteroid microwave emissions - Ceres and Vesta On the wavelength dependence of apparent emissivity of asteroid microwave emissions - Ceres and Vesta

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101..122w&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, Jan. 1989, p. 122-125.

Astronomy and Astrophysics

Astronomy

6

Astronomical Photometry, Ceres Asteroid, Emissivity, Microwave Emission, Vesta Asteroid, Wavelengths, Dielectric Properties, Infrared Spectra, Signal To Noise Ratios, Surface Properties

Scientific paper

Observations of Ceres and Vesta demonstrate the need for modifying the physical parameters of the standard model procedure in treating single-wavelength observations. It is suggested that simultaneous IR and cm-wavelength data should be used in order to determine such properties as the surface dielectric characteristics, layer depth, and radio emissivity. If using the standard model, an emissivity of 0.8 should be adopted for wavelengths of longer than 1 cm.

Affiliated with

Also associated with

No associations

Rating

On the wavelength dependence of apparent emissivity of asteroid microwave emissions - Ceres and Vesta 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 On the wavelength dependence of apparent emissivity of asteroid microwave emissions - Ceres and Vesta, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the wavelength dependence of apparent emissivity of asteroid microwave emissions - Ceres and Vesta will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-828369