Highlights of the NASA Particle Astrophysics Program



Document title: Highlights of the NASA Particle Astrophysics Program
Journal: Brazilian journal of physics
Database: PERIÓDICA
System number: 000379553
ISSN: 0103-9733
Authors: 1
Institutions: 1National Aeronautics and Space Administration, Science Mission Directorate, Washington, Distrito de Columbia. Estados Unidos de América
Year:
Season: Oct
Volumen: 44
Number: 5
Pages: 534-539
Country: Brasil
Language: Inglés
Document type: Conferencia o discurso
Approach: Analítico, descriptivo
English abstract The NASA Particle Astrophysics Program covers Origin of the Elements, Nearest Sources of Cosmic Rays, How Cosmic Particle Accelerators Work, The Nature of Dark Matter, and Neutrino Astrophysics. Progress in each of these topics has come from sophisticated instrumentation flown on long duration balloon (LDB) flights around Antarctica over the past two decades. New opportunities including Super Pressure Balloons (SPB) and International Space Station (ISS) platforms are emerging for the next major step. Stable altitudes and long durations enabled by SPB flights ensure ultra-long duration balloon (ULDB) missions that can open doors to new science opportunities. The Alpha Magnetic Spectrometer (AMS) has been operating on the ISS since May 2011. The CALorimetric Electron Telescope (CALET) and Cosmic Ray Energetics And Mass (CREAM) experiments are being developed for launch to the Japanese Experiment Module Exposed Facility (JEM-EF) in 2015. And, the Extreme Universe Space Observatory (EUSO) is planned for launch to the ISS JEM-EF after 2017. Collectively, these four complementary ISS missions covering a large portion of the cosmic ray energy spectrum serve as a cosmic ray observatory
Disciplines: Física y astronomía
Keyword: Astronomía,
Física de partículas y campos cuánticos,
Astrofísica,
Rayos cósmicos,
Observatorios astronómicos
Keyword: Physics and astronomy,
Astronomy,
Particle physics and quantum fields,
Astrophysics,
Cosmic rays,
Astronomical observatories
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