The EAS-TOP array at E0 = 1014 - 10 16 eV: Stability and resolutions

Details The EAS-TOP array at E0 = 1014 - 10 16 eV: Stability and resolutions The EAS-TOP array at E0 = 1014 - 10 16 eV: Stability and resolutions

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nimpa.277...23a&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 277, Issue 1, p. 23-28.

Physics

34

Scientific paper

The characteristics of the EAS-TOP extensive air shower array as a detector of very high energy cosmic rays (E0 >= 1014 eV) for astrophysical studies are discussed. The array is located on top of the underground Gran Sasso Laboratory in central Italy; a subarray (11 modules of the em detector) has been operating since the end of 1987. From such data the stability of the detector, the timing resolution, the accuracies in the determination of the arrival directions (δθ = 1.2° at E0 ~ 200 TeV in the present configuration) and in the reconstruction of the lateral electron distribution and of the shower size are derived.

Affiliated with

Also associated with

No associations

Rating

The EAS-TOP array at E0 = 1014 - 10 16 eV: Stability and resolutions 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 The EAS-TOP array at E0 = 1014 - 10 16 eV: Stability and resolutions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The EAS-TOP array at E0 = 1014 - 10 16 eV: Stability and resolutions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1739169