The Balloon Array for RBSP Relativistic Electron Losses (BARREL)
Abstract 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 w...
Ausführliche Beschreibung
Autor*in: |
Millan, R. M. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
2013 |
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Anmerkung: |
© The Author(s) 2013 |
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Übergeordnetes Werk: |
Enthalten in: Space science reviews - Springer Netherlands, 1962, 179(2013), 1-4 vom: 26. März, Seite 503-530 |
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Übergeordnetes Werk: |
volume:179 ; year:2013 ; number:1-4 ; day:26 ; month:03 ; pages:503-530 |
Links: |
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DOI / URN: |
10.1007/s11214-013-9971-z |
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Katalog-ID: |
OLC2033700194 |
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520 | |a Abstract 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 (∼20 kg) stratospheric balloons will be successively launched to maintain an array of ∼5 payloads spread across ∼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. | ||
650 | 4 | |a Radiation belts | |
650 | 4 | |a Wave-particle interactions | |
650 | 4 | |a Electron precipitation | |
700 | 1 | |a McCarthy, M. P. |4 aut | |
700 | 1 | |a Sample, J. G. |4 aut | |
700 | 1 | |a Smith, D. M. |4 aut | |
700 | 1 | |a Thompson, L. D. |4 aut | |
700 | 1 | |a McGaw, D. G. |4 aut | |
700 | 1 | |a Woodger, L. A. |4 aut | |
700 | 1 | |a Hewitt, J. G. |4 aut | |
700 | 1 | |a Comess, M. D. |4 aut | |
700 | 1 | |a Yando, K. B. |4 aut | |
700 | 1 | |a Liang, A. X. |4 aut | |
700 | 1 | |a Anderson, B. A. |4 aut | |
700 | 1 | |a Knezek, N. R. |4 aut | |
700 | 1 | |a Rexroad, W. Z. |4 aut | |
700 | 1 | |a Scheiman, J. M. |4 aut | |
700 | 1 | |a Bowers, G. S. |4 aut | |
700 | 1 | |a Halford, A. J. |4 aut | |
700 | 1 | |a Collier, A. B. |4 aut | |
700 | 1 | |a Clilverd, M. A. |4 aut | |
700 | 1 | |a Lin, R. P. |4 aut | |
700 | 1 | |a Hudson, M. K. |4 aut | |
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10.1007/s11214-013-9971-z doi (DE-627)OLC2033700194 (DE-He213)s11214-013-9971-z-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Millan, R. M. verfasserin aut The Balloon Array for RBSP Relativistic Electron Losses (BARREL) 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2013 Abstract 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 (∼20 kg) stratospheric balloons will be successively launched to maintain an array of ∼5 payloads spread across ∼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. Radiation belts Wave-particle interactions Electron precipitation McCarthy, M. P. aut Sample, J. G. aut Smith, D. M. aut Thompson, L. D. aut McGaw, D. G. aut Woodger, L. A. aut Hewitt, J. G. aut Comess, M. D. aut Yando, K. B. aut Liang, A. X. aut Anderson, B. A. aut Knezek, N. R. aut Rexroad, W. Z. aut Scheiman, J. M. aut Bowers, G. S. aut Halford, A. J. aut Collier, A. B. aut Clilverd, M. A. aut Lin, R. P. aut Hudson, M. K. aut Enthalten in Space science reviews Springer Netherlands, 1962 179(2013), 1-4 vom: 26. März, Seite 503-530 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:179 year:2013 number:1-4 day:26 month:03 pages:503-530 https://doi.org/10.1007/s11214-013-9971-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 179 2013 1-4 26 03 503-530 |
spelling |
10.1007/s11214-013-9971-z doi (DE-627)OLC2033700194 (DE-He213)s11214-013-9971-z-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Millan, R. M. verfasserin aut The Balloon Array for RBSP Relativistic Electron Losses (BARREL) 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2013 Abstract 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 (∼20 kg) stratospheric balloons will be successively launched to maintain an array of ∼5 payloads spread across ∼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. Radiation belts Wave-particle interactions Electron precipitation McCarthy, M. P. aut Sample, J. G. aut Smith, D. M. aut Thompson, L. D. aut McGaw, D. G. aut Woodger, L. A. aut Hewitt, J. G. aut Comess, M. D. aut Yando, K. B. aut Liang, A. X. aut Anderson, B. A. aut Knezek, N. R. aut Rexroad, W. Z. aut Scheiman, J. M. aut Bowers, G. S. aut Halford, A. J. aut Collier, A. B. aut Clilverd, M. A. aut Lin, R. P. aut Hudson, M. K. aut Enthalten in Space science reviews Springer Netherlands, 1962 179(2013), 1-4 vom: 26. März, Seite 503-530 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:179 year:2013 number:1-4 day:26 month:03 pages:503-530 https://doi.org/10.1007/s11214-013-9971-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 179 2013 1-4 26 03 503-530 |
allfields_unstemmed |
10.1007/s11214-013-9971-z doi (DE-627)OLC2033700194 (DE-He213)s11214-013-9971-z-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Millan, R. M. verfasserin aut The Balloon Array for RBSP Relativistic Electron Losses (BARREL) 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2013 Abstract 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 (∼20 kg) stratospheric balloons will be successively launched to maintain an array of ∼5 payloads spread across ∼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. Radiation belts Wave-particle interactions Electron precipitation McCarthy, M. P. aut Sample, J. G. aut Smith, D. M. aut Thompson, L. D. aut McGaw, D. G. aut Woodger, L. A. aut Hewitt, J. G. aut Comess, M. D. aut Yando, K. B. aut Liang, A. X. aut Anderson, B. A. aut Knezek, N. R. aut Rexroad, W. Z. aut Scheiman, J. M. aut Bowers, G. S. aut Halford, A. J. aut Collier, A. B. aut Clilverd, M. A. aut Lin, R. P. aut Hudson, M. K. aut Enthalten in Space science reviews Springer Netherlands, 1962 179(2013), 1-4 vom: 26. März, Seite 503-530 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:179 year:2013 number:1-4 day:26 month:03 pages:503-530 https://doi.org/10.1007/s11214-013-9971-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 179 2013 1-4 26 03 503-530 |
allfieldsGer |
10.1007/s11214-013-9971-z doi (DE-627)OLC2033700194 (DE-He213)s11214-013-9971-z-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Millan, R. M. verfasserin aut The Balloon Array for RBSP Relativistic Electron Losses (BARREL) 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2013 Abstract 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 (∼20 kg) stratospheric balloons will be successively launched to maintain an array of ∼5 payloads spread across ∼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. Radiation belts Wave-particle interactions Electron precipitation McCarthy, M. P. aut Sample, J. G. aut Smith, D. M. aut Thompson, L. D. aut McGaw, D. G. aut Woodger, L. A. aut Hewitt, J. G. aut Comess, M. D. aut Yando, K. B. aut Liang, A. X. aut Anderson, B. A. aut Knezek, N. R. aut Rexroad, W. Z. aut Scheiman, J. M. aut Bowers, G. S. aut Halford, A. J. aut Collier, A. B. aut Clilverd, M. A. aut Lin, R. P. aut Hudson, M. K. aut Enthalten in Space science reviews Springer Netherlands, 1962 179(2013), 1-4 vom: 26. März, Seite 503-530 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:179 year:2013 number:1-4 day:26 month:03 pages:503-530 https://doi.org/10.1007/s11214-013-9971-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 179 2013 1-4 26 03 503-530 |
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10.1007/s11214-013-9971-z doi (DE-627)OLC2033700194 (DE-He213)s11214-013-9971-z-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Millan, R. M. verfasserin aut The Balloon Array for RBSP Relativistic Electron Losses (BARREL) 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2013 Abstract 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 (∼20 kg) stratospheric balloons will be successively launched to maintain an array of ∼5 payloads spread across ∼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. Radiation belts Wave-particle interactions Electron precipitation McCarthy, M. P. aut Sample, J. G. aut Smith, D. M. aut Thompson, L. D. aut McGaw, D. G. aut Woodger, L. A. aut Hewitt, J. G. aut Comess, M. D. aut Yando, K. B. aut Liang, A. X. aut Anderson, B. A. aut Knezek, N. R. aut Rexroad, W. Z. aut Scheiman, J. M. aut Bowers, G. S. aut Halford, A. J. aut Collier, A. B. aut Clilverd, M. A. aut Lin, R. P. aut Hudson, M. K. aut Enthalten in Space science reviews Springer Netherlands, 1962 179(2013), 1-4 vom: 26. März, Seite 503-530 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:179 year:2013 number:1-4 day:26 month:03 pages:503-530 https://doi.org/10.1007/s11214-013-9971-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 179 2013 1-4 26 03 503-530 |
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Enthalten in Space science reviews 179(2013), 1-4 vom: 26. März, Seite 503-530 volume:179 year:2013 number:1-4 day:26 month:03 pages:503-530 |
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Millan, R. M. McCarthy, M. P. Sample, J. G. Smith, D. M. Thompson, L. D. McGaw, D. G. Woodger, L. A. Hewitt, J. G. Comess, M. D. Yando, K. B. Liang, A. X. Anderson, B. A. Knezek, N. R. Rexroad, W. Z. Scheiman, J. M. Bowers, G. S. Halford, A. J. Collier, A. B. Clilverd, M. A. Lin, R. P. Hudson, M. K. |
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The Balloon Array for RBSP Relativistic Electron Losses (BARREL) |
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Abstract 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 (∼20 kg) stratospheric balloons will be successively launched to maintain an array of ∼5 payloads spread across ∼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. © The Author(s) 2013 |
abstractGer |
Abstract 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 (∼20 kg) stratospheric balloons will be successively launched to maintain an array of ∼5 payloads spread across ∼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. © The Author(s) 2013 |
abstract_unstemmed |
Abstract 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 (∼20 kg) stratospheric balloons will be successively launched to maintain an array of ∼5 payloads spread across ∼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. © The Author(s) 2013 |
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