Perseid meteor stream : cross and longitudinal structures from radar observations

Details Perseid meteor stream : cross and longitudinal structures from radar observations Perseid meteor stream : cross and longitudinal structures from radar observations

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999p%26ss...47..281s&link_type=abstract

Planetary and Space Science, Volume 47, Issue 1-2, p. 281-289.

Other

1

Scientific paper

Results of 23 years of observations of the Perseid meteor shower by the Ondřejov meteor radar in the period 1958-1996 are presented. Activity profiles in four categories of echo durations differ slightly in the position of the activity peak and other characteristics of the central core in the range of solar longitudes (Eq.1950.0) 138.0° <= L∘. <= 140.5°. Maximum activity of the central core is allocated at L∘. = 139.17°+/-0.06° in accordance with previous studies. The variation ratio of the year-to-year shower activity along the stream within the above L∘. limits was found to be 2.2 : 1.

Affiliated with

Also associated with

No associations

Rating

Perseid meteor stream : cross and longitudinal structures from radar 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 Perseid meteor stream : cross and longitudinal structures from radar observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Perseid meteor stream : cross and longitudinal structures from radar observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1276723