On the Meteor Height from Forward Scatter Radio Observations

Details On the Meteor Height from Forward Scatter Radio Observations On the Meteor Height from Forward Scatter Radio Observations

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999baas...31r1590c&link_type=abstract

American Astronomical Society, DPS Meeting #31, late abstracts, #59.38; Bulletin of the American Astronomical Society, Vol. 31,

Physics

Plasma Physics

Scientific paper

It is known from theory that, by means of a plasma physics approach, it is possible to obtain a simple formula to calculate an approximate height of a meteor (Foschini, 1999). This formula applies to the forward scatter of radio waves and has the advantage that it does not depend on the diffusion coefficient. On the other hand, it is possible to apply the formula to a particular type of meteor only (overdense meteor type I), which is a small fraction of the total number observed. We have carried out a statistical analysis of several radio echoes from meteor showers recorded during last years by a radio observer located in Belgium. Results are compared and discussed with those obtained with other methods and available in literature. škip 11pt Foschini L., Astron. Astrophys. 341, (1999), 634

Affiliated with

Also associated with

No associations

Rating

On the Meteor Height from Forward Scatter Radio Observations 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 Meteor Height from Forward Scatter Radio Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Meteor Height from Forward Scatter Radio Observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1725083