3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
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Plenaries 3
Place
Location: Merida, Mexico
Room: Gran Salon Yucatan (Fiesta Americana)
Date:
6 Jul 16:30 - 18:30
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The solution to the origin of the UHECRs, like the solution
to the origin of the galactic cosmic rays, depends on direct
cosmic ray observations in addition to multiwavelength
and UHE neutrino detections of cosmic-ray sources. The
advent of Auger, IceCube, GLAST, and ground-based
gamma-ray telescopes promises multi-channel data that
should solve this problem. In this talk, I review favor
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Presented by Dr. Charles DERMER
on
6/7/2007
at
22:25
There are two kinds of relations between cosmic ray research and investigations of
space weather effects. Since energetic particles in space and low energy cosmic rays
interact with materials of the satellite and airplane systems as well as with the
atmosphere, monitoring of the changes of flux of cosmic particles especially during
solar flares, space storms and geomagnetic disturbances is imp
... More
Presented by Dr. Karel KUDELA
on
6/7/2007
at
22:55
The exclusive Galactic gamma-ray club rallies new members. Supernova remnants,
pulsar wind nebulae, and binary systems hosting a compact object have recently
joined the young pulsars as firmly established sources of gamma rays in the
Milky Way. The first examples of these gamma-ray emitters had been suspected in
the early eighties with COS-B, many more in the nineties with EGRET, but only
the
... More
Presented by Dr. Isabelle GRENIER
on
6/7/2007
at
21:30
The study of transport processes in dilute plasmas in the presence of
magnetic fields is a subject that has attracted astrophysicists for
over five decades.First attempts to deal with this problem date back
to the mid twentieth century with the work of Spitzer and
Braginski. The results obtained by the second author, who dealt with
the problem using Landau's equation, are still regarded as th
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Presented by Prof. Leopoldo GARCÍA-COLÍN