3-11 July 2007
Merida, Mexico
Mexico/General timezone
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Plenaries 6

Place

Location: Merida, Mexico
Room: Gran Salon Yucatan (Fiesta Americana)
Date: 10 Jul 16:30 - 18:30

Timetable | Contribution List

Displaying 3 contributions out of 3
Type: Oral Session: Plenaries 6
Track: Special
The Pierre Auger Observatory is now ~80% completed with all of the fluorescence detectors and 1300 tanks in operation. The exposure accumulated since January 2004 is ~ 5000 km^2 sr yr, approximately 3 times that reached by AGASA and about twice the exposure of HiRes. The hybrid nature of the detector and unparalleled attention to systematic uncertainties has allowed an accurate measurement o ... More
Presented by Dr. Alan A. WATSON on 10/7/2007 at 22:25
Type: Oral Session: Plenaries 6
Track: Special
The past decade has seen enormous progress in the sensitivity TeV gamma-ray survey instruments. With the ability to continuously observe 2sr of the sky, survey instruments hold the promise of fully exploring the transient high-energy universe. After decades of roaming in the desert, survey instruments are now making detailed measurements of the Galactic diffuse gamma-ray emission and discov ... More
Presented by Dr. Gus SINNIS on 10/7/2007 at 22:55
Type: Oral Session: Plenaries 6
Track: Special
The presence of a heliosphere surrounding the Sun was suggested by L. Davis fifty years ago, when there was limited knowledge of interplanetary and interstellar conditions. That suggestion was soon followed by Parker’s prediction of a supersonic solar wind that was observed by Mariner 2, initiating a systematic exploration of the heliosphere that now extends to high solar latitudes and to d ... More
Presented by Prof. E. C. STONE on 10/7/2007 at 21:30
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