SPACE AND COSMIC RAY PHYSICS SEMINAR

University of Maryland
Atlantic Building, Room 2400
4:30 PM Monday, April 16, 2012
Coffee, Tea & Snacks 4:15-4:30 PM

Harm Moraal
North-West University, Potchefstroom, South Africa
Atmospheric Cosmic-Ray Measurements in the 21st Century

The cosmic-ray intensity inside the atmosphere forms a well-defined part of the space radiation environment. Neutron monitors in a world-wide network measure this intensity and its variations, augmented by muon telescopes, atmospheric Cherenkov detectors and balloon experiments. It is shown in the talk how these instruments make useful contributions to the field of Space Weather and early warnings of such events.
These atmospheric detectors are complementary to typical space experiments because they measure higher energies, which is important to study acceleration processes in solar cosmic-ray eventsthey have higher counting rates to resolve smaller eventsthey have better directional sensitivity through the extensive worldwide network,they provide a long-term stable baseline which is important to reconstruct solar activity in the distant past.
Most importantly, advances in electronics and neutron counters make it possible to miniaturize these detectors and deploy them in places that were inaccessible to the current instruments. This leads to new possibilities, examples of which will be discussed.


Sponsored by: Department of Physics and the Institute for Physical Science and Technology, University of Maryland. For information call Victoria at (301) 405-4811 or go to the UMD Space Physics group seminar web site.

There is free parking after 4:00 PM in lot B (the big parking garage across the street from the ATL building). There are a limited number of spaces in lot Q next to the new ATL wing with free parking after 4PM even when there is a basketball game on campus.