Modeled and observed Perseid radiants

Details Modeled and observed Perseid radiants Modeled and observed Perseid radiants

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jimo...34...67i&link_type=abstract

WGN, Journal of the International Meteor Organization, vol. 34, no. 3, p. 67-70

Computer Science

Scientific paper

The article deals with locations of geocentric radiants of hypothetic particles of the Perseid stream, ejected in 1862 from the comet 109P/Swift-Tuttle. The results obtained have been compared with the data of photographic observations of Perseids in 1993-1994. The spread of location of geocentric radiants of particle models, which could be observed within the Nodal Blanket Filament in 1993-1994, may be equal to RA = 1.4 deg, Dec = 0.7 deg under certain conditions of meteoroid ejections.

Affiliated with

Also associated with

No associations

Rating

Modeled and observed Perseid radiants 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 Modeled and observed Perseid radiants, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeled and observed Perseid radiants will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1064059