| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1847090 | Nuclear Physics B - Proceedings Supplements | 2007 | 6 Pages |
Abstract
The observation of Ultra-High Energy Cosmic Radiation (UHECR) from Space might take benefit from some preliminary ancillary measurements. One of the most important is the characterization of the near-UV background, produced in the atmosphere by natural and man-made phenomena, that affects the performances of any UHECR Space-detector. An accurate measurement of these effects is very helpful to design and optimize the instrument, in particular as it affects its duty cycle and signal-to-noise ratio. Here we present some preliminary considerations about the design of a micro-satellite mission devoted to the characterization of this kind of background. We focus in particular on the basic requirements of the measurement apparatus.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
