Abstract |
A high angular resolution muon telescope with 6m2 sensitive area
based on 120 cherenkov detectors is proposed to be constructed and
used for estimation of atmosphere parameters, and space weather
investigations. The telescope is foreseen to be placed at ALOMAR
observatory, Norway, and correlation of the variations of the
cosmic rays muon flux with data sets from LIDARs, direct
measurements from balloons, and magnetometer would be studied.
|
References |
1. COSMIC RAYS, S. Eidelman et al., Physics Letters B592, 1
(2004), available on the PDG WWW pages (URL: http://pdg.lbl.gov/) ;
Revised March 2002 by T.K. Gaisser and T. Stanev (Bartol Research
Inst., Univ. of Delaware); revised September 2005 by P.V. Sokolsky
(Univ. of Utah) and R.E. Streitmatter (NASA) 2. Study of
Atmospheric Temperature at Different Altitudes using Muon Angular
Distribution at Sea Level, V. V. Borog et all, Proceedings of the
29th International Cosmic Ray Conference, Pune 2005 3. Gravity
waves in the troposphere and stratosphere during the MaCWAVE/MIDAS
summer rocket program, A. Schлoch et all, GEOPHYSICAL RESEARCH
LETTERS, VOL. ???, XXXX, DOI:10.1029/
|