A precise knowledge of the angular resolution of scintillator arrays used to observe extended air showers (EAS) is of key importance in the search for VHE/UHE \(\gamma\) point sources. Four independent methods have been used to determine the mean resolution for which a value of \(\left\langle\Delta
β¦ LIBER β¦
The optimum distance at which to determine the size of a giant air shower
β Scribed by D. Newton; J. Knapp; A.A. Watson
- Publisher
- Elsevier Science
- Year
- 2007
- Tongue
- English
- Weight
- 354 KB
- Volume
- 26
- Category
- Article
- ISSN
- 0927-6505
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Methods to determine the angular resolut
β
M. Merck; A. Karle; S. Martinez; F. Arqueros; K.H. Becker; M. Bott-Bodenhausen;
π
Article
π
1996
π
Elsevier Science
π
English
β 836 KB
Energy determination of cosmic ray showe
β
G. Ros; G. Medina-Tanco; L. del Peral; J.C. DβOlivo; F. Arqueros; M.D. RodrΓguez
π
Article
π
2009
π
Elsevier Science
π
English
β 817 KB
In most high energy cosmic ray surface arrays, the primary energy is currently determined from the value of the lateral distribution function at a fixed distance from the shower core, r 0 . The value of r 0 is mainly related to the geometry of the array and is, therefore, considered as fixed indepen
The Size Distribution of HII Regions as
β
I. A. Issa
π
Article
π
1981
π
John Wiley and Sons
π
English
β 242 KB
π 2 views
A method to determine the size of surfac
β
Jadranka TomaiΔ; Tarzan LegoviΔ; Vera Ε½utiΔ
π
Article
π
1992
π
Elsevier
π
English
β 748 KB
How to determine the grade of expansion
β
L. D'Auria
π
Article
π
1884
π
Elsevier Science
π
English
β 179 KB
On the possibility of a simultaneous mea
β
G. Rose; H.U. Widdel
π
Article
π
1972
π
Elsevier Science
π
English
β 886 KB