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Electromagnetic particles and muons constitute the dominant contribution to the ground detector signals.
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The telescope was proposed in 1998 with the goal of lowering the threshold of observation of gamma rays by ground detectors to 20-30 Genergiesienergies
An interesting frequency range is 0.1 1 Hz, which will be missed by both the ground detectors on the Earth and LISA and would be the best window for searching for stochastic background gravitational waves.
The almost-completed Pierre Auger Observatory on the plains of the Pampa Amarilla in western Argentina comprises more than 1200 ground detectors and 24 telescopes and covers an area of 300 square kilometers (Science, 21 June 2002, p. 2134).
EUSO-TA is an on-ground detector for measuring UV (290 430 nm) light from extensive air showers induced by cosmic rays.
This results in a total (Lambda _{A}=eta_{A}cdotLambda_{H}=60)% (−2.3 dB) and a ground based detector noise rate of less than 100 cps which we ignore in comparison to the total E91 singles rate of (R_{A}approx60mbox{ Mcps}).
Seismic noise from being located on the Earth itself limits how sensitive a ground-based detector can be.
Common ground based detectors used to monitor CR fluxes are neutron monitors and muon detectors measuring, respectively, secondary CR neutrons and muons produced in the atmosphere.
VERITAS is a major ground-based detector of very high energy (VHE, E >100 GeV) gamma rays and cosmic rays.
It said the company would not be permitted to switch off equipment like ground radar detectors or telephone lines for maintenance unless a backup was in place.
The neutron monitor (NM) is a ground-based detector designed to estimate the cosmic ray intensity by measuring secondary particles.
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