West Ford Dipole Belt: Optical Detection at Palomar

Details West Ford Dipole Belt: Optical Detection at Palomar West Ford Dipole Belt: Optical Detection at Palomar

Aug 1963

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1963sci...141..797s&link_type=abstract

Science, Volume 141, Issue 3583, pp. 797-798

Computer Science

1

Scientific paper

Optical detection of the West Ford orbiting dipole belt was accomplished on at least four occasions during the second week in May 1963. The maximum surface brightness was about 4 percent of the night sky radiation at an effective wavelength of overline{λ} = 4400 angstrom. The density of the belt has evidently decreased because it was not detected in a second observation period during the third week in June.

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