Arrival Time Distribution by the New Observation System at Taro

Details Arrival Time Distribution by the New Observation System at Taro Arrival Time Distribution by the New Observation System at Taro

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..207o&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

The arrival time distribution of EAS has been observed by using Ultra Fast Cherenkov detector (UFC) and oscilloscope at Taro observatory since 1995 (sea level 200m). The EAS array is arranged 169 sets of 0.25m2 scintillation detectors in the shape of a lattice at intervals of 1.5m and about 40 scintillation detectors which consists of 1m2 and 0.25m2 is arranged in the peripheral part. Then, it consists of 8 fast timing detectors. The UFC detector is installed in the palce of about 20m from the trigger center. The observation system of a UFC detector was changed from the autumn of 2000. The outline of a new observation system and EAS arrival time distribution are reported.

Affiliated with

Also associated with

No associations

Rating

Arrival Time Distribution by the New Observation System at Taro 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 Arrival Time Distribution by the New Observation System at Taro, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Arrival Time Distribution by the New Observation System at Taro will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1135677