Cosmic ray intensity variations at primary rigidities near 1900 GV

Details Cosmic ray intensity variations at primary rigidities near 1900 GV Cosmic ray intensity variations at primary rigidities near 1900 GV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..262l&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 262-265 (SEE N85-34006 22-93)

Physics

Amplitudes, Cosmic Ray Showers, Muons, Sidereal Time, Variations, Anisotropy, Harmonic Analysis, Histograms, Standard Deviation

Scientific paper

Preliminary analysis of an experiment monitoring cosmic ray muons yields
a first sidereal harmonic amplitude for rigidities around 1900 GV of
(7.95±3.97)×10-4 at 5.1±1.9 h right
ascension. A significant anti-sidereal first harmonic is, however, also
seen.

Affiliated with

Also associated with

No associations

Rating

Cosmic ray intensity variations at primary rigidities near 1900 GV 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 Cosmic ray intensity variations at primary rigidities near 1900 GV, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmic ray intensity variations at primary rigidities near 1900 GV will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-754593