37:
57:. The MAG instrument includes both the Fluxgate Magnetometer (FGM) and Advanced Stellar Compass (ASC) instruments. There two sets of MAG instrument suites, and they are both positioned on the far end of three solar panel array booms. Each MAG instrument suite observes the same swath of Jupiter, and by having two sets of instruments, determining what signal is from the planet and what is from spacecraft is supported. Avoiding signals from the spacecraft is another reason MAG is placed at the end of the solar panel boom, about 10 m (33 feet) and 12 m (39 feet) away from the central body of the
200:, etc. This style of FGM uses twin wide-range, triaxial flux gate sensors mounted far away from the spacecraft body in which the magnetic flux is periodically switched (hence the ame flux-gate). Two FGM's are used so the separate readings can be combined to make the magnetic field calculation. MAG has two vector fluxgate magnetometers supported by advanced star trackers. The star tracking system allows the orientation of the FGM to be calculated and determined more accurately enhancing the usefulness of the FGM readings.
24:
of a
Fluxgate Magnetometer (FGM) visible just above the 2 Advanced Stellar Compass (ASC) light baffles that look outward at a slight angle. The inboard MAG sensor suit is identical, but rotated 180 degrees and located 2 meters away. When deployed, the two sensor suites will be about 10 and 12 meters from the center of the spacecraft. The spacecraft is shown in launch configuration with solar arrays and MAG boom stowed. Image credit: NASA/JPL-Caltech/LMSS"
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NASA caption for this image: "... The two
Magnetic Field Experiment (MAG) sensor suites can be seen on the 4-meter-long dedicated magnetometer boom in the foreground. The MAG boom is deployed in flight at the outer end of one of the spacecraft's three solar arrays. The outboard sensor suite consists
125:
Another advantage to studying
Jupiter's field is that on Earth, crustal magnetism interferes with measurements of the field generated deep in the core, partially shielding it from measurements. On Earth the field is generated by spinning liquid iron, whereas on Jupiter is generated by hydrogen.
286:
included analysis of data from the Juno magnetometer which passed 10 times closer than previous probes. The nature of
Jupiter's magnetic field was examined, combining the latest results from MAG with a mathematical model called VIP4 spherical harmonic model for the magnetic field of Jupiter.
126:
Jupiter is mostly hydrogen (about 90%), and as it compresses from gravity it turns conductive in a special form. However, it is not known if farther in, where it should compress into metallic form, the hydrogen continues to conduct electricity. That is one of the questions
117:
mission, and in particular the task rests on the
Magnetometer instruments. MAG measures the field about 60 times per second, and records the direction and strength of the field. MAG collected data on Earth during its 9 October 2013 flyby en route to Jupiter (this was a
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141:
spacecraft by NASA's
Goddard Spaceflight Center (GFSC) in October 2010. MAG was overall designed and built at the NASA Goddard Space Flight Center (GFSC) in Greenbelt, Maryland. The Advanced Stellar Compass was built and contributed by the
629:
Connerney, J. E.; Oliversen, R. J.; Espley, J. R.; MacDowall, R. J.; Schnurr, R.; Sheppard, D.; Odom, J.; Lawton, P.; Murphy, S. (2013-12-01). "Juno
Magnetometer Observations in the Earth's Magnetosphere".
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s magnetometers will measure
Jupiter's magnetic field with extraordinary precision and give us a detailed picture of what the field looks like both around the planet and deep within, ...
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Jupiter has the strongest and biggest magnetic fields known to exist in the solar system. Studying these fields is one of the goals of the
88:, and instead diverts it away from the planet, effectively creating a cavity in the solar wind flow, called a magnetosphere, composed of a
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that take a picture of the sky, then compare those images to a catalog of star maps to allow the orientation to be determined.
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s launch on 5 August 2011. The ASC allow a very precise determination of the magnetometers orientation in space. They are
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2015:
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Moore, Kimberly M.; Bloxham, Jeremy; Connerney, John E. P.; Jørgensen, John L.; Merayo, José M. G. (2017-05-25).
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Artist generated diagram showing the location of various instruments. MAG is on the lower right of this graphic
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in the sky despite being nearly 1700 times farther away. Jupiter's internal magnetic field prevents the
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may answer. In addition to studying
Jupiter, the MAG also returned data on the Earth's magnetosphere.
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72:. If one could see Jupiter's magnetic field from Earth, it would appear five times larger than the
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The fluxgate magnetometer (FGM) is similar to previous instruments flown on spacecraft like the
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818:"The analysis of initial Juno magnetometer data using a sparse magnetic field representation"
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The analysis of initial Juno magnetometer data using a sparse magnetic field representation
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154:) commonly known as DTU) The FGM and ASC were turned on in late August after
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determine the three-dimensional structure of the polar magnetosphere and its
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Mission's Deputy
Principal Investigator and head of the magnetometer team
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137:' facility in Denver, Colorado, United States for integration into the
54:
555:. In Bagenal, Fran; Dowling, Timothy E.; McKinnon, William B. (eds.).
475:"The Nine Space Gadgets NASA's Juno Orbiter Is Using to Study Jupiter"
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Jupiter's magnetic fields were previously observed in the 1970s with
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724:"Juno Magnetic Field Investigation – Fluxgate Magnetometer Diagram"
28:
2074:
2010:
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27:
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Graphic of Jupiter's magnetosphere with Io plasma torus in yellow
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of Jupiter, which is one of the largest structures in the
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was working on including a Scalar Helium Magnetometer on
718:
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779:"Instruments and Science Data Systems – Magnetometers"
663:"NASA Goddard Delivers Magnetometers for Juno Mission"
592:
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Khurana, K. K.; Kivelson, M. G.; et al. (2004).
359:(Magnetometer and electrical fields investigation on
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598:"Juno to Show Jupiter's Magnetic Field in High-Def"
196:, Active Magnetospheric Particle Tracer Explorers,
146:. (Technical University of Denmark, or in Danish (
688:"Juno Magnetic Field Investigation - Instruments"
557:Jupiter: The Planet, Satellites and Magnetosphere
1081:Science instruments on satellites and spacecraft
933:(Jupiter Energetic-particle Detector Instrument)
299:(type of instrument to measure magnetic fields)
167:
80:, a stream of ionized particles emitted by the
550:"The configuration of Jupiter's magnetosphere"
1066:
893:
64:The MAG instrument is designed to detect the
16:Scientific instrument on the Juno space probe
8:
559:. Cambridge University Press. pp. 1–3.
102:determine the dynamics of Jupiter's interior
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441:. Archived from the original on 2018-10-31
939:(Jovian Auroral Distributions Experiment)
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122:maneuver, but also was to collect data).
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274:, in addition to the FGM and ASC suite.
18:
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92:different from that of the solar wind.
451:
439:Spaceflight101: Space News and Beyond
367:List of missions to the outer planets
7:
873:Peers Inside a Giant - June 29, 2016
133:The MAG instrument was delivered to
47:(MAG) is an instrument suite on the
2864:Venetia Burney Student Dust Counter
974:(Radio and Plasma Waves Experiment)
435:"Juno Science Payloads/Experiments"
400:"Juno Magnetic Field Investigation"
14:
755:"MAVEN » Magnetometer (MAG)"
99:map the magnetic field of Jupiter
84:, from interacting directly with
986:
981:
945:(Jovian Infrared Auroral Mapper)
2833:International Lunar Observatory
1644:(TRMM, Terra, Aura, Suomi NPP,
144:Technical University of Denmark
507:Reports on Progress in Physics
473:Ferreira, Becky (2016-07-05).
320:Jupiter Magnetospheric Orbiter
1:
2779:High Resolution Stereo Camera
152:Danmarks Tekniske Universitet
135:Lockheed Martin Space Systems
822:Geophysical Research Letters
2900:Goddard Space Flight Center
1710:Radiation Budget Instrument
729:Goddard Space Flight Center
693:Goddard Space Flight Center
405:Goddard Space Flight Center
227:. Magnetometers related to
2921:
2036:Infrared Space Observatory
968:(Ultraviolet Spectrograph)
632:AGU Fall Meeting Abstracts
527:10.1088/0034-4885/56/6/001
500:"Planetary Magnetospheres"
1039:
979:
784:Jet Propulsion Laboratory
458:: CS1 maint: unfit URL (
2859:Inertial Stellar Compass
2224:Raman Laser Spectrometer
310:Magnetosphere of Jupiter
282:In 2017, a paper called
2854:Deep Space Atomic Clock
2113:Venus Emissivity Mapper
303:Spacecraft magnetometer
237:, MGS, Voyager, AMPTE,
2890:Spacecraft instruments
962:(Microwave Radiometer)
498:Russell, C.T. (1993).
334:Microwave Radiometer (
315:Earth's magnetic field
186:
151:
41:
33:
25:
2869:Plasma Wave Subsystem
1980:Multispectral Scanner
1304:Pioneer Venus Orbiter
1108:Pioneer Venus Orbiter
1031:New Frontiers program
39:
31:
22:
1837:Mars Climate Orbiter
1479:RM-08 and MTVZA-OK (
1003:Juno Radiation Vault
926:GS (Gravity Science)
843:10.1002/2017gl073133
198:Mars Global Surveyor
2794:Mars Orbiter Camera
869:NASA News - NASA's
834:2017GeoRL..44.4687M
644:2013AGUFMSM21E..04C
519:1993RPPh...56..687R
53:orbiter for planet
2772:Imagers/telescopes
1920:Spectrophotometers
361:Parker Solar Probe
278:Results and papers
42:
34:
26:
2895:Juno (spacecraft)
2877:
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2814:Rosalind Franklin
2736:
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2723:Rosalind Franklin
2698:Mass spectrometer
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2628:Rosalind Franklin
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2127:UV-visible (UVVS)
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2017:Rosalind Franklin
1955:Visible-IR (VIRS)
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1401:DMSP 5D-2/F13-F15
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828:(10): 4687–4693.
759:lasp.colorado.edu
566:978-0-521-81808-7
2912:
2715:(Europa Clipper)
2703:
2664:(on ExoMars TGO)
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2608:Neutral particle
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1875:Ultraviolet (UV)
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1594:Infrared-visible
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791:. Archived from
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261:Van Allen Probes
247:Lunar Prospector
231:include ones on
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2401:Cassini–Huygens
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1999:
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1927:Long wavelength
1907:
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1795:Mariner 6 and 7
1742:
1671:MESSR and VTIR
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1555:Electra (radio)
1549:Cassini-Huygens
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1189:Cassini–Huygens
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1095:Cassini–Huygens
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2750:(on InSight)
2741:Seismometers
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1668:Kanopus-V-IK
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1263:
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797:. Retrieved
793:the original
782:
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758:
749:
738:. Retrieved
736:. 2017-01-17
727:
702:. Retrieved
700:. 2017-01-17
691:
682:
671:. Retrieved
669:. 2010-10-27
638:: SM21E–04.
635:
631:
610:. Retrieved
608:. 2011-07-31
602:Mission Juno
601:
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297:Magnetometer
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70:Solar System
63:
61:spacecraft.
58:
49:
45:Magnetometer
44:
43:
2826:instruments
2803:Microscopes
1469:Meteor-M2-1
1458:Meteor-3M-1
919:Instruments
479:Motherboard
2884:Categories
2533:Near-Earth
2475:Near-Earth
2445:Pioneer 11
2377:Near-Earth
2315:Pioneer 10
2268:Near-Earth
2153:Mariner 10
1963:Near-Earth
1882:Near-Earth
1835:PMIRR (on
1823:Pioneer 10
1801:Mariner 10
1723:Sentinel-3
1601:Near-Earth
1492:Sentinel-3
1463:MTVZA-GYa
1426:Kanopus-ST
1375:Sentinel-6
1362:Near-Earth
1345:Radiometer
1195:Europa-UVS
1021:(launcher)
912:spacecraft
799:2019-03-09
764:2017-02-07
740:2017-02-07
704:2019-03-09
673:2019-03-09
612:2017-01-06
484:2017-01-06
445:2020-03-20
415:2019-03-09
373:References
212:Pioneer 11
206:Pioneer 10
78:solar wind
2838:MoonLIGHT
2676:Mariner 2
2656:Curiosity
2582:Mariner 2
2519:detectors
2438:MESSENGER
2417:Mariner 2
2329:Voyager 1
2187:Voyager 1
2160:MESSENGER
2069:MESSENGER
2054:(on Juno)
2042:Voyager 1
1985:SCIAMACHY
1854:Voyager 1
1817:2M No.522
1812:2M No.521
1733:Suomi NPP
1561:Mariner 2
1466:Meteor-M2
1453:, MOS-1b)
1354:Microwave
1327:Voyager 1
1285:Pioneer 7
1272:MESSENGER
1229:Mariner 2
852:0094-8276
535:250897924
252:MESSENGER
224:Voyager 2
218:Voyager 1
74:full moon
2755:Viking 1
2674:SPS (on
2624:ADRON-RM
2610:detector
2577:ASPERA-4
2572:ASPERA-3
2517:Particle
2280:QuakeSat
2080:E-THEMIS
1843:Venera 9
1685:Meteor-2
1663:ADEOS II
1475:Nimbus 7
1421:GPM Core
1388:ADEOS II
1321:Venera 9
1309:Sakigake
1223:Magellan
1182:Akatsuki
1133:Venera 4
1102:Magellan
454:cite web
291:See also
190:Voyagers
178:—
2683:Ulysses
2593:Ulysses
2554:Proba-2
2540:DEMETER
2291:Proba-2
2282:1 and 2
2234:SHERLOC
2024:MA-MISS
1901:Proba-2
1807:Mars 96
1790:Luna 13
1777:InSight
1763:Diviner
1737:NOAA-21
1721:SLSTR (
1646:NOAA-20
1637:AVNIR-2
1580:Rosetta
1532:Zond-PP
1481:Sich-1M
1456:MTVZA (
1416:Envisat
1395:Shizuku
1393:AMSR2 (
1373:AMR-C (
1212:InSight
1206:Galileo
1025:Jupiter
1019:Atlas V
830:Bibcode
640:Bibcode
515:Bibcode
343:Waves (
243:CLUSTER
107:auroras
55:Jupiter
2816:rover)
2784:HiRISE
2725:rover)
2713:MASPEX
2669:Nozomi
2630:rover)
2412:Magsat
2407:FIELDS
2354:ICEMAG
2309:FIELDS
2230:rover)
2176:SPICAV
2171:SPICAM
2108:SPICAV
2103:SPICAM
2040:IRIS (
1890:EURECA
1716:GCOM-C
1714:SGLI (
1704:EURECA
1697:JERS-1
1487:Seasat
1440:MOPITT
1386:AMSR (
1383:(AQUA)
1381:AMSR-E
1279:Nozomi
1217:Kaguya
1163:WISDOM
1128:MARSIS
1123:SHARAD
1118:SELENE
1113:REASON
996:Design
850:
563:
533:
357:FIELDS
259:, and
257:STEREO
239:GIOTTO
215:, and
194:Magsat
148:Danish
90:plasma
2789:LORRI
2662:FREND
2482:Swarm
2384:Swarm
2241:rover
2209:Raman
2166:NOMAD
2142:Alice
2098:Ralph
2075:MERIS
2052:JIRAM
2019:rover
2011:AKARI
1888:ORI (
1729:VIIRS
1702:ORI (
1695:OPS (
1690:MODIS
1675:MOS-1
1661:GLI (
1642:CERES
1632:AVNIR
1621:Terra
1613:ASTER
1608:AVHRR
1527:WSF-M
1517:SSMIS
1512:SSM/I
1451:MOS-1
1449:MSR (
1444:Terra
1431:MIRAS
1087:Radar
972:Waves
943:JIRAM
553:(PDF)
531:S2CID
503:(PDF)
325:UVS (
234:MAVEN
173:'
159:'
2847:Misc
2748:SEIS
2719:MOMA
2654:(on
2549:DSLP
2547:and
2545:TPMU
2358:PIMS
2356:and
2347:Juno
2286:SGVM
2275:GOES
2090:(on
2088:SUDA
2084:MISE
2044:and
2029:ISEM
1995:TRMM
1975:MOMS
1970:CASE
1896:LYRA
1785:IRIS
1775:(on
1765:(on
1657:ERSS
1652:ERBS
1627:AIRS
1617:MISR
1572:Juno
1522:TRMM
1507:SMOS
1502:SMMR
1497:SMAP
1436:MISR
1411:ERSS
1369:AQUA
1249:6, 7
1042:NASA
937:JADE
931:JEDI
910:Juno
871:Juno
848:ISSN
789:NASA
734:NASA
698:NASA
667:NASA
606:NASA
561:ISBN
460:link
410:NASA
345:Juno
336:Juno
327:Juno
272:Juno
229:Juno
221:and
209:and
181:Juno
170:Juno
156:Juno
139:Juno
128:Juno
115:Juno
59:Juno
50:Juno
2652:DAN
2587:SPS
2342:MAG
2181:UVS
1990:TES
1941:ISO
1773:HP3
1767:LRO
1567:MWR
966:UVS
960:MWR
954:MAG
838:doi
523:doi
268:JPL
82:Sun
2886::
2432:10
2322:11
2086:,
2082:,
1848:10
1830:11
1735:,
1679:1b
1615:,
1438:,
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