The CASSIOPE/e-POP Magnetic Field Instrument (MGF)

Abstract Field-aligned currents couple energy between the Earth’s magnetosphere and ionosphere and are responsible for driving both micro and macro motions of plasma and neutral atoms in both regimes. These currents are believed to be a contributing energy source for ion acceleration in the polar io...
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Autor*in:	Wallis, D. D. [verfasserIn] Miles, D. M. Narod, B. B. Bennest, J. R. Murphy, K. R. Mann, I. R. Yau, A. W.

Format:	Artikel
Sprache:	Englisch

Erschienen:	2014

Schlagwörter:	Magnetometer Fluxgate Satellite Field-aligned currents

Anmerkung:	© The Author(s) 2014

Übergeordnetes Werk:	Enthalten in: Space science reviews - Springer Netherlands, 1962, 189(2014), 1-4 vom: 22. Okt., Seite 27-39
Übergeordnetes Werk:	volume:189 ; year:2014 ; number:1-4 ; day:22 ; month:10 ; pages:27-39

Links:	Volltext

DOI / URN:	10.1007/s11214-014-0105-z

Katalog-ID:	OLC2033701247

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520			\|a Abstract Field-aligned currents couple energy between the Earth’s magnetosphere and ionosphere and are responsible for driving both micro and macro motions of plasma and neutral atoms in both regimes. These currents are believed to be a contributing energy source for ion acceleration in the polar ionosphere and may be detected via measurements of magnetic gradients along the track of a polar orbiting spacecraft, usually the north-south gradients of the east-west field component. The detection of such gradients does not require observatory class measurements of the geomagnetic field. The Magnetic Field instrument (MGF) measures the local magnetic field onboard the Enhanced Polar Outflow Probe (e-POP) satellite by using two ring-core fluxgate sensors to characterize and remove the stray spacecraft field. The fluxgate sensors have their heritage in the MAGSAT design, are double wound for reduced mass and cross-field dependence, and are mounted on a modest 0.9 m carbon-fiber boom. The MGF samples the magnetic field 160 times per sec (∼50 meters) to a resolution of 0.0625 nT and outputs data at 1952 bytes per second including temperature measurements. Its power consumption is 2.2 watts, and its noise level is 7 pT per root Hz at 1 Hz.
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allfields	10.1007/s11214-014-0105-z doi (DE-627)OLC2033701247 (DE-He213)s11214-014-0105-z-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Wallis, D. D. verfasserin aut The CASSIOPE/e-POP Magnetic Field Instrument (MGF) 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2014 Abstract Field-aligned currents couple energy between the Earth’s magnetosphere and ionosphere and are responsible for driving both micro and macro motions of plasma and neutral atoms in both regimes. These currents are believed to be a contributing energy source for ion acceleration in the polar ionosphere and may be detected via measurements of magnetic gradients along the track of a polar orbiting spacecraft, usually the north-south gradients of the east-west field component. The detection of such gradients does not require observatory class measurements of the geomagnetic field. The Magnetic Field instrument (MGF) measures the local magnetic field onboard the Enhanced Polar Outflow Probe (e-POP) satellite by using two ring-core fluxgate sensors to characterize and remove the stray spacecraft field. The fluxgate sensors have their heritage in the MAGSAT design, are double wound for reduced mass and cross-field dependence, and are mounted on a modest 0.9 m carbon-fiber boom. The MGF samples the magnetic field 160 times per sec (∼50 meters) to a resolution of 0.0625 nT and outputs data at 1952 bytes per second including temperature measurements. Its power consumption is 2.2 watts, and its noise level is 7 pT per root Hz at 1 Hz. Magnetometer Fluxgate Satellite Field-aligned currents Miles, D. M. aut Narod, B. B. aut Bennest, J. R. aut Murphy, K. R. aut Mann, I. R. aut Yau, A. W. aut Enthalten in Space science reviews Springer Netherlands, 1962 189(2014), 1-4 vom: 22. Okt., Seite 27-39 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:189 year:2014 number:1-4 day:22 month:10 pages:27-39 https://doi.org/10.1007/s11214-014-0105-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_4306 GBV_ILN_4700 AR 189 2014 1-4 22 10 27-39
spelling	10.1007/s11214-014-0105-z doi (DE-627)OLC2033701247 (DE-He213)s11214-014-0105-z-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Wallis, D. D. verfasserin aut The CASSIOPE/e-POP Magnetic Field Instrument (MGF) 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2014 Abstract Field-aligned currents couple energy between the Earth’s magnetosphere and ionosphere and are responsible for driving both micro and macro motions of plasma and neutral atoms in both regimes. These currents are believed to be a contributing energy source for ion acceleration in the polar ionosphere and may be detected via measurements of magnetic gradients along the track of a polar orbiting spacecraft, usually the north-south gradients of the east-west field component. The detection of such gradients does not require observatory class measurements of the geomagnetic field. The Magnetic Field instrument (MGF) measures the local magnetic field onboard the Enhanced Polar Outflow Probe (e-POP) satellite by using two ring-core fluxgate sensors to characterize and remove the stray spacecraft field. The fluxgate sensors have their heritage in the MAGSAT design, are double wound for reduced mass and cross-field dependence, and are mounted on a modest 0.9 m carbon-fiber boom. The MGF samples the magnetic field 160 times per sec (∼50 meters) to a resolution of 0.0625 nT and outputs data at 1952 bytes per second including temperature measurements. Its power consumption is 2.2 watts, and its noise level is 7 pT per root Hz at 1 Hz. Magnetometer Fluxgate Satellite Field-aligned currents Miles, D. M. aut Narod, B. B. aut Bennest, J. R. aut Murphy, K. R. aut Mann, I. R. aut Yau, A. W. aut Enthalten in Space science reviews Springer Netherlands, 1962 189(2014), 1-4 vom: 22. Okt., Seite 27-39 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:189 year:2014 number:1-4 day:22 month:10 pages:27-39 https://doi.org/10.1007/s11214-014-0105-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_4306 GBV_ILN_4700 AR 189 2014 1-4 22 10 27-39
allfields_unstemmed	10.1007/s11214-014-0105-z doi (DE-627)OLC2033701247 (DE-He213)s11214-014-0105-z-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Wallis, D. D. verfasserin aut The CASSIOPE/e-POP Magnetic Field Instrument (MGF) 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2014 Abstract Field-aligned currents couple energy between the Earth’s magnetosphere and ionosphere and are responsible for driving both micro and macro motions of plasma and neutral atoms in both regimes. These currents are believed to be a contributing energy source for ion acceleration in the polar ionosphere and may be detected via measurements of magnetic gradients along the track of a polar orbiting spacecraft, usually the north-south gradients of the east-west field component. The detection of such gradients does not require observatory class measurements of the geomagnetic field. The Magnetic Field instrument (MGF) measures the local magnetic field onboard the Enhanced Polar Outflow Probe (e-POP) satellite by using two ring-core fluxgate sensors to characterize and remove the stray spacecraft field. The fluxgate sensors have their heritage in the MAGSAT design, are double wound for reduced mass and cross-field dependence, and are mounted on a modest 0.9 m carbon-fiber boom. The MGF samples the magnetic field 160 times per sec (∼50 meters) to a resolution of 0.0625 nT and outputs data at 1952 bytes per second including temperature measurements. Its power consumption is 2.2 watts, and its noise level is 7 pT per root Hz at 1 Hz. Magnetometer Fluxgate Satellite Field-aligned currents Miles, D. M. aut Narod, B. B. aut Bennest, J. R. aut Murphy, K. R. aut Mann, I. R. aut Yau, A. W. aut Enthalten in Space science reviews Springer Netherlands, 1962 189(2014), 1-4 vom: 22. Okt., Seite 27-39 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:189 year:2014 number:1-4 day:22 month:10 pages:27-39 https://doi.org/10.1007/s11214-014-0105-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_4306 GBV_ILN_4700 AR 189 2014 1-4 22 10 27-39
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title_full	The CASSIOPE/e-POP Magnetic Field Instrument (MGF)
author_sort	Wallis, D. D.
journal	Space science reviews
journalStr	Space science reviews
lang_code	eng
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dewey-hundreds	600 - Technology
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publishDateSort	2014
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container_start_page	27
author_browse	Wallis, D. D. Miles, D. M. Narod, B. B. Bennest, J. R. Murphy, K. R. Mann, I. R. Yau, A. W.
container_volume	189
class	600 VZ 16,12 ssgn
format_se	Aufsätze
author-letter	Wallis, D. D.
doi_str_mv	10.1007/s11214-014-0105-z
dewey-full	600
title_sort	the cassiope/e-pop magnetic field instrument (mgf)
title_auth	The CASSIOPE/e-POP Magnetic Field Instrument (MGF)
abstract	Abstract Field-aligned currents couple energy between the Earth’s magnetosphere and ionosphere and are responsible for driving both micro and macro motions of plasma and neutral atoms in both regimes. These currents are believed to be a contributing energy source for ion acceleration in the polar ionosphere and may be detected via measurements of magnetic gradients along the track of a polar orbiting spacecraft, usually the north-south gradients of the east-west field component. The detection of such gradients does not require observatory class measurements of the geomagnetic field. The Magnetic Field instrument (MGF) measures the local magnetic field onboard the Enhanced Polar Outflow Probe (e-POP) satellite by using two ring-core fluxgate sensors to characterize and remove the stray spacecraft field. The fluxgate sensors have their heritage in the MAGSAT design, are double wound for reduced mass and cross-field dependence, and are mounted on a modest 0.9 m carbon-fiber boom. The MGF samples the magnetic field 160 times per sec (∼50 meters) to a resolution of 0.0625 nT and outputs data at 1952 bytes per second including temperature measurements. Its power consumption is 2.2 watts, and its noise level is 7 pT per root Hz at 1 Hz. © The Author(s) 2014
abstractGer	Abstract Field-aligned currents couple energy between the Earth’s magnetosphere and ionosphere and are responsible for driving both micro and macro motions of plasma and neutral atoms in both regimes. These currents are believed to be a contributing energy source for ion acceleration in the polar ionosphere and may be detected via measurements of magnetic gradients along the track of a polar orbiting spacecraft, usually the north-south gradients of the east-west field component. The detection of such gradients does not require observatory class measurements of the geomagnetic field. The Magnetic Field instrument (MGF) measures the local magnetic field onboard the Enhanced Polar Outflow Probe (e-POP) satellite by using two ring-core fluxgate sensors to characterize and remove the stray spacecraft field. The fluxgate sensors have their heritage in the MAGSAT design, are double wound for reduced mass and cross-field dependence, and are mounted on a modest 0.9 m carbon-fiber boom. The MGF samples the magnetic field 160 times per sec (∼50 meters) to a resolution of 0.0625 nT and outputs data at 1952 bytes per second including temperature measurements. Its power consumption is 2.2 watts, and its noise level is 7 pT per root Hz at 1 Hz. © The Author(s) 2014
abstract_unstemmed	Abstract Field-aligned currents couple energy between the Earth’s magnetosphere and ionosphere and are responsible for driving both micro and macro motions of plasma and neutral atoms in both regimes. These currents are believed to be a contributing energy source for ion acceleration in the polar ionosphere and may be detected via measurements of magnetic gradients along the track of a polar orbiting spacecraft, usually the north-south gradients of the east-west field component. The detection of such gradients does not require observatory class measurements of the geomagnetic field. The Magnetic Field instrument (MGF) measures the local magnetic field onboard the Enhanced Polar Outflow Probe (e-POP) satellite by using two ring-core fluxgate sensors to characterize and remove the stray spacecraft field. The fluxgate sensors have their heritage in the MAGSAT design, are double wound for reduced mass and cross-field dependence, and are mounted on a modest 0.9 m carbon-fiber boom. The MGF samples the magnetic field 160 times per sec (∼50 meters) to a resolution of 0.0625 nT and outputs data at 1952 bytes per second including temperature measurements. Its power consumption is 2.2 watts, and its noise level is 7 pT per root Hz at 1 Hz. © The Author(s) 2014
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container_issue	1-4
title_short	The CASSIOPE/e-POP Magnetic Field Instrument (MGF)
url	https://doi.org/10.1007/s11214-014-0105-z
remote_bool	false
author2	Miles, D. M. Narod, B. B. Bennest, J. R. Murphy, K. R. Mann, I. R. Yau, A. W.
author2Str	Miles, D. M. Narod, B. B. Bennest, J. R. Murphy, K. R. Mann, I. R. Yau, A. W.
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doi_str	10.1007/s11214-014-0105-z
up_date	2024-07-03T18:05:16.816Z
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