
Glenn M. Mason
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Glenn M. MasonProfessor, Joint/Physics
Space Physics
The origin and evolution of the solar system and galaxy can be studied by measuring the
composition of their condensed and gaseous materials. These compositional data contain
information on processes that created the material both in the big-bang, in later
nucleosynthetic processing, and, more recently, in fractionation processes associated with
the condensation of the material from the interstellar medium into stars, planets, and
smaller objects. Since astrophysical objects routinely accelerate ions to high energies,
multiple streams of particles from a wide variety of sites fill the interplanetary space
near Earth. These energetic particle streams may be sampled, studied, and probed for
information about their parent sites and the processes that accelerated and brought them
here. Professor Mason is studying these energetic particle populations in collaboration
with members of the Space Physics group and with experimental groups in U.S. and in
Europe. Professor Mason's experiments on the SAMPEX, WIND,
and Advanced Composition
Explorer (ACE)
spacecraft are studying particle acceleration in solar flares, interplanetary shocks, and
the so-called anomalous cosmic rays, which are interstellar material accelerated in the
outer regions of the heliosphere.
Selected publications:
- Mason, G.M., J.E. Mazur, and T.T. von Rosenvinge, Energetic heavy ions observed upstream
of the Earth's bow shock by the STEP/EPACT instrument on WIND, Geophys. Res. Letters, 23,
1231-1234, 1996.
- Dwyer, J.R., G.M. Mason, J.E. Mazur, J.R. Jokipii, T.T. von Rosenvinge, and R.P.
Lepping, Perpendicular transport of low energy corotating interaction region_associated
nuclei, Astrophys. J. (Letters), 490, L115-L118, 1997.
- Mazur, J.E., G.M. Mason, J.R. Dwyer, and T.T. von Rosenvinge, Solar energetic particles
inside magnetic clouds observed with the Wind spacecraft, Geophys. Res. Letters, 25,
2521-2524, 1998.
Intesities of energetic nuclei measured on the ACE spacecraft following 2 solar flare
explosions in November 1997.
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