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COBE/DIRBE Studies of Scattering By Interplanetary Dust

Published online by Cambridge University Press:  27 February 2018

G. B. Berriman ,
J. L. Weiland ,
C. M. Lisse ,
W. T. Reach ,
M. G. Hauser  and
T. Kelsall
G. B. Berriman
Affiliation:
General Sciences Corp., Code 685.3, NASA Goddard Space Flight Center, Greenbelt, MD 20771
J. L. Weiland
Affiliation:
General Sciences Corp., Code 685.3, NASA Goddard Space Flight Center, Greenbelt, MD 20771
C. M. Lisse
Affiliation:
Hughes STX, Code 685.9, NASA Goddard Space Flight Center, Greenbelt, MD 20771
W. T. Reach
Affiliation:
Universities Space Research Association, Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771
M. G. Hauser
Affiliation:
Code 680, NASA Goddard Space Flight Center, Greenbelt, MD 20771
T. Kelsall
Affiliation:
Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771

Abstract

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The high photometric quality and full-sky coverage in the COBE DIRBE datasets make possible detailed studies of the interplanetary medium. This paper presents a preliminary derivation of the infrared scattering phase function of interplanetary dust. The ultimate purpose of these investigations is to use the DIRBE observations to constrain the composition, size and structure of interplanetary dust grains.

Type
IX. Zodiacal Light and Thermal Emission
Information
International Astronomical Union Colloquium , Volume 150: Physics, Chemistry and Dynamics of Interplanetary Dust , 1996 , pp. 321 - 324
Copyright
Copyright © Astronomical Society of the Pacific 1996

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