3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
Contribution Poster (WITHDRAWN)
Speakers
- Sofia ANDRINGA
Primary authors
- Prof. Mario PIMENTA (Departamento de Fisica, IST and LIP Lisboa, Portugal)
- Sofia ANDRINGA (LIP, Lisbon)
Abstract content
A method to reconstruct the 3-dimensional structure of extensive air showers, seen by fluorescence detectors, is described. The observation of the shower is done in 2-dimensional pixels, for consecutive time bins. Time corresponds to a third dimension. Assuming that the cosmic ray shower propagates as a plane wave front moving at the speed of light, a complex 3D volume in space can be associated to each measured charge (per pixel and time bin). The 3D description in space allows a simultaneous access to the longitudinal and lateral profiles of each shower. In case several eyes observe the same shower, the method gives a straight-forward combination of all the information.
If this papers is presented for a collaboration, please specify the collaboration
The Pierre Auger Collaboration