New PDF release: Advanced Technology and Particle Physics

By M. Barone

ISBN-10: 9812381805

ISBN-13: 9789812381804

Court cases of the seventh foreign convention on ICATPP-7, held October 15-19, 2001 in Villa, Olmo, Como, Italy. gains brand new know-how functions to radiation detection.

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Extra info for Advanced Technology and Particle Physics

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1 The Simulation Particle tracing The tracing code is based on the solution of the Lorentz equation of a charged particle in a static magnetic field starting from particle velocity: FLorentz=m— = Z-q-y$ xBtotal\ (1) In effect geomagnetic field is not static, but eq. (1) can be anyway applied in our case with the requirement of a small time step (typically -^) in relation to the instant gyroradius of the particle (see Subsec. 2 for errors). (l) solved. In this code updated internal (IGRF 2005) and external (Tsyganenko 96) magnetic field models are used, together with a magp analytical shape (Sibeck '91) and a Runge-Kutta 6th order metod to solve Lorentz differential equation.

The resulting picture of the event seen by the detector looks like a narrow track in which the recorded amount of light is proportional to the shower size at the various penetration depth in the atmosphere. From a Low Earth Orbit (LEO) space platform, the UV fluorescence induced in atmospheric Nitrogen by the incoming radiation can be monitored and studied. Other phenomena such as meteors, space debris, lightning, atmospheric flashes, can also be observed; the luminescence coming from the EAS produced by the Cosmic Ray quanta can be on the other hand disentangled from the general background exploiting its fast timing characteristic feature.

When viewed continuously, the object moves on a straight path with the speed of light. The resulting picture of the event seen by the detector looks like a narrow track in which the recorded amount of light is proportional to the shower size at the various penetration depth in the atmosphere. From a Low Earth Orbit (LEO) space platform, the UV fluorescence induced in atmospheric Nitrogen by the incoming radiation can be monitored and studied. Other phenomena such as meteors, space debris, lightning, atmospheric flashes, can also be observed; the luminescence coming from the EAS produced by the Cosmic Ray quanta can be on the other hand disentangled from the general background exploiting its fast timing characteristic feature.

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Advanced Technology and Particle Physics by M. Barone


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