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The Balloon Array for RBSP Relativistic Electron Losses (BARREL)

Journal

SPACE SCIENCE REVIEWS
Volume 179, Issue 1-4, Pages 503-530

Publisher

SPRINGER
DOI: 10.1007/s11214-013-9971-z

Keywords

Radiation belts; Wave-particle interactions; Electron precipitation

Funding

  1. NASA Living With a Star program through NASA at Dartmouth College [NNX08AM58G]
  2. Natural Environmental Research Council under the Antarctic Funding Initiative [AFI/11/22]
  3. NERC [bas0100023, NE/H014888/1] Funding Source: UKRI
  4. Natural Environment Research Council [bas0100023, NE/H014888/1] Funding Source: researchfish

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BARREL is a multiple-balloon investigation designed to study electron losses from Earth's Radiation Belts. Selected as a NASA Living with a Star Mission of Opportunity, BARREL augments the Radiation Belt Storm Probes mission by providing measurements of relativistic electron precipitation with a pair of Antarctic balloon campaigns that will be conducted during the Austral summers (January-February) of 2013 and 2014. During each campaign, a total of 20 small (similar to 20 kg) stratospheric balloons will be successively launched to maintain an array of similar to 5 payloads spread across similar to 6 hours of magnetic local time in the region that magnetically maps to the radiation belts. Each balloon carries an X-ray spectrometer to measure the bremsstrahlung X-rays produced by precipitating relativistic electrons as they collide with neutrals in the atmosphere, and a DC magnetometer to measure ULF-timescale variations of the magnetic field. BARREL will provide the first balloon measurements of relativistic electron precipitation while comprehensive in situ measurements of both plasma waves and energetic particles are available, and will characterize the spatial scale of precipitation at relativistic energies. All data and analysis software will be made freely available to the scientific community.

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