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Abstract:
The High Energy Monitor Instrument (HEMI) is being developed
by students at the Pennsylvania State
University to detect
when a gamma ray burst (GRB) occurs and record data on the event.
Ultimately, HEMI is intended to be a student instrument for
measuring GRBs on a future satellite. As the challenges for
developing student satellite hardware are significant, a precursor
balloon flight will provide the necessary heritage to enable a more
costly and complex project.
As GRB events are rare, on this flight, the instrument will
be used to study cosmic showers as a precursor to studying GRBs.
HEMI will collect information as to the number of particles and
their energies that it intercepts per time interval. When this
number increases dramatically, this indicates a cosmic shower. HEMI
will record data in a similar manner as if this were a GRB to
prepare for future GRB instruments.
There are currently 10 undergraduates and one graduate
student participating on this project from physics, astronomy and
astrophysics, and aerospace, mechanical, and electrical engineering.
The project is managed by the Penn State Student Space Programs
Laboratory. HEMI
conforms to all of the requirements specified in the Call for
Proposals and requires no additional resources beyond those already
allocated by the program.
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