Small scale structure in the brightness of the zodiacal light - Ground-based observations

Details Small scale structure in the brightness of the zodiacal light - Ground-based observations Small scale structure in the brightness of the zodiacal light - Ground-based observations

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990p%26ss...38..517m&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 38, April 1990, p. 517-527.

Physics

1

Brightness, High Resolution, Night Sky, Space Observations (From Earth), Spatial Resolution, Zodiacal Light, Ecliptic, Error Analysis, Interplanetary Dust, Latitude, Longitude, Spatial Distribution

Scientific paper

Ground-based observations of the evening zodiacal light are used to derive a table of zodiacal light brightnesses at spatial resolutions as small as 0.5 deg in differential ecliptic longitude and 1.0 deg in ecliptic latitude. Significant differences are found in the brightness distribution above and below the ecliptic plane. Attention is given to a feature found in the brightness at all ecliptic latitudes, between differential ecliptic longitudes 39 deg and 42 deg.

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