Three-dimensional infrared models of the interplanetary dust distribution

Details Three-dimensional infrared models of the interplanetary dust distribution Three-dimensional infrared models of the interplanetary dust distribution

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ep%26s...50..501k&link_type=abstract

Earth, Planets and Space, Volume 50, p. 501-505.

Other

7

Scientific paper

We have calculated the brightness of zodiacal emission by using the three dimensional optical models of zodiacal cloud. By comparing the calculated brightness distribution with the IRASobservations, we found that the cosine model is the best out of the three for describing the helioecliptic latitude dependence of dust distribution. We also found best parameters for the heliocentric variations of the dust temperature and volumetric absorption cross-section. Inclination and ascending node of the symmetry plane were deduced from annual variations of i) the peak offset latitude and ii) the pole brightness difference. Longitudes of the ascending node derived from i) and ii) are shown to be significantly different from each other.

Affiliated with

Also associated with

No associations

Rating

Three-dimensional infrared models of the interplanetary dust distribution 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 Three-dimensional infrared models of the interplanetary dust distribution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three-dimensional infrared models of the interplanetary dust distribution will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1331834