picam et la mission bepi colombo j.j. berthelier, j becker, f. leblanc (latmos), f. leblanc (lpp)
DESCRIPTION
PICAM et la MISSION BEPI COLOMBO J.J. Berthelier, J Becker, F. Leblanc (LATMOS), F. Leblanc (LPP) Atelier Pôle Système Solaire IPSL, Avril 2013. MERCURE. La planète la plus proche du Soleil périhélie 0.31AU, aphélie 0.46 AU, période orbitale 88 jours - PowerPoint PPT PresentationTRANSCRIPT
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PICAM et la MISSION BEPI COLOMBO
J.J. Berthelier, J Becker, F. Leblanc (LATMOS), F. Leblanc (LPP)
Atelier Ple Systme Solaire IPSL, Avril 2013
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La plante la plus proche du Soleil prihlie 0.31AU, aphlie 0.46 AU, priode orbitale 88 jours la plus petite (R 2440 km) mais la plus dense d ~ 5.43 (noyau Fe?)- rotation 59 jours (rsonance 3/2 avec priode orbitale, unique dans le Systme Solaire) axe de rotation ~ perpendiculaire au plan de lcliptique atmosphre trs tnue tempratures extrmes +430C, -180C champ magntique interne BMercure~ 1% BTerre, (dynamo, noyau externe liquide) magntosphre et sous-orages analogues ceux de la Terre MERCURE
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BepiColombo Orbites de MMO et MPO autour de Mercure Les satellites BEPICOLOMBOBEPICOLOMBO est constitu de deux sondes diffrentes pour remplir tous ses objectifs scientifiques. Le MPO est une sonde stabilise trois-axes en orbite basse polaire faiblement elliptique dont le priherme sera l'altitude de 400 km et l'apoherme 1500 km. Il est dveloppe sous la responsabilit de l'ESA
Caractristiques de la sonde MPOMasse totale400 kgMasse Charge Utile50 kg MPO Le MMO est une sonde en stabilisation spinne qui sera place en orbite elliptique polaire dont le priherme sera l'altitude de 400 km et l'apoherme 12000 km. Il est dveloppe sous la responsabilit de la JAXA.
Caractristiques de la sonde MMO Collaboration ESA-JAXA 2 satellites MPO (ESA) plantaire, MMO (JAXA) magntosphrique Lancement Aot 2015, arrive Janvier 2022- Propulsion lectrique et assistance gravitationnelle Lune, Terre, VenusMISSION BEPI COLOMBO (1)
BIENVENUE SCIENCE MISSION SATELLITES INSTRUMENTS MPO INSTRUMENTS MMO ORGANISATION CONTACTS AUTRES SITES
PUBLICATIONS
CARACTERISTIQUES MPO Masse totale : 400 kg Masse CU : 50 kg MMO Masse totale : 220 kg Masse CU : 41 kg Cliquer ici pour augmenter ou diminuer la taille des caractres : AAAA
MMO Dernire mise jour le 05/04/2007
Masse totale220 kgMasse Charge Utile41 kg
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MMO (JAXA) 220 kg, CU 41 kgMagnetospheric ScienceChamp MagntiquePlasma Particules EnergiquesOndes(+ observations MPO B, plasma)MPO (ESA) 400 kg, CU 50 kgPlanetary ScienceSurface, Atmosphre neutreChamp magntiquePlasma MISSION BEPI COLOMBO (2)
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PICAMPlanetary Ion CAMeraIWF (Autriche) (K. Torkar, PI)LATMOS (+IKI) (optique ionique et dtecteur)MPS (Allemagne) convertisseurs HV et gatingKFKI (Hongrie) convertisseur DC/DC
Un des 4 Instruments du consortium SERENA(Search for Exospheric Refilling and Emitted Natural Abundances)Objectifs scientifiques de SERENA (PICAM)- Composition lmentaire, chimique et isotopique de lexosphre neutre- Composition lmentaire de lexosphre ionique- Mcanismes de formation et dynamique des exosphres neutre et ionise- Echappement des neutres et des ions Pntration du vent solaire et prcipitations des ions de basse nergie
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PICAM, Objectifs Scientifiques (1) Lexosphre ionise de MercureSourcesVent solaire - pntration travers les frontires de la magntosphre, transportExosphre - missions des constituants par la surfacedsorption thermique, photo-dsorption, criblage)Processus de cration et de pertesProcessus photo-chimiques, collisions sur la surface, chappementTransport du Plasma dans lionosphre de MercureCirculation grande chelle (convection, chappement)Acclration
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Crote jectionstimule parles photonsCriblage par le vent solaire Absorption neutre et ion magntosphrique et apport mtoritiqueMlange induit parimpact mtoritiqueDiffusionExosphre Photo-ionisationEchappementneutreAdapt de Killen et Ip (1999)Formation de lexosphre: le cas de Najectionpar chauffageRgoliteImpactemtoritiquePICAM, Objectifs Scientifiques (2)
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Themis: 13/07/2008Emission Na D2Themis: 22/10/2009Emission Na D2PICAM, Objectifs scientifiques (3)Observations du sodium exosphrique, tlescope THEMIS, Iles Canaries
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PICAM, Objectifs Scientifiques (4) Le Sodium dans lionosphre, modlisation (F. Leblanc et al. , 2004)
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PICAM, Objectifs Scientifiques (5)Lionosphre et la magntosphre de Mercure
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PICAM, Objectifs ExprimentauxMesure des fonctions de distribution des ions de basse nergie gamme dnergie: ~ 3 eV 3 keV, rsolution ~ 10% champ de vue: omnidirectionnel sur un demi-espace (2 st.), rsolution 15/30Donne accs au transport et lacclration du plasmaAvec MMO, 2 points de mesure pour tudier la dynamique de la magntosphre
Mesure de la composition du plasma- masses 1 ~ 130 uma, (H, He, N?, O, Na, Mg, Ca, K, Xe?)- rsolution suffisante pour sparer Na, Mg et Ca, KDonne accs aux sources et aux mcanismes de formation de lionosphre
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Champ de vue dans un plan radial ~ 0-75PICAM, Concept de linstrument
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PICAM, Optique Electrostatique
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PICAM, mesure de la distribution angulaire et en nergie Modlisation numrique, ions 1 keVEssais QM, Ions N2+, 1 keVDistribution angulaireModlisation numrique, ions 1 keVRsolution en nergieEssais QM, Ions N2+, 1 keV
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nombre de coups
Rpartition par pixel sur le secteur 1 par tranche d'lvation,rotation de +/-180, modle de vol, 5mm, fente 0.3mm, 80el, +/-15az
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Nombre d'impacts sur le secteur 1 (+/- 30) de la galette, modle de vol, new M2, 5mm, fente 0.3mm, 80el, +/-15az, 15 points fente, 289800 part
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nombre de coups
Rpartition par pixel sur le secteur 1 par tranche d'lvation,rotation de +/-180, modle de vol, 5mm, fente 0.3mm, 80el, +/-15az, 15 points fente, 289800 part, 3.39%
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nombre de coups
Rpartition par pixel sur le secteur 1 par tranche d'lvation,rotation de +/-180, modle de vol, 5mm, fente 0.5mm, 80el, +/-15az, 15 points fente, 289800 part, 2.38%
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Rpartition par pixel sur le secteur 1 par tranche d'lvation,rotation de +/-180, modle de vol, 5mm, fente 0.3mm, 80el, +/-15az, 15 points fente, 289800 part, 2.38%
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Rpartition par pixel sur le secteur 1 par tranche d'lvation,rotation de +/-180, modle de vol, 5mm, fente 0.3mm, 1.5 entre lamelles, M1 1100V, 80el, +/-15az, 15 points fente, 289800 part, gde fenetre
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Rpartition par pixel sur le secteur 1 par tranche d'lvation,rotation de +/-180, modle de vol, 5mm, fente 0.3mm, 1.5 entre lamelles, M1 1100V, 80el, +/-15az, 15 points fente, 163800 part
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10-20
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Rpartition par pixel sur le secteur 1 par tranche d'lvation,rotation de +/-180, modle de vol,plaque_coupe_10mm, fente 0.5mm, 80el, +/-15az, 15 points fente, 289800 part, new new M2, gatting_X1
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PICAM, Mesure du temps de volSimulation dune mesure de Temps de Volpour les masses 23 (Na) et 24 (Mg)Mesures de temps de vol, QM, ions N2+ 300 eV
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Feuil1
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Feuil1
masse 23
masse 24
Feuil2
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Feuil3
MBD0D85A3C0.xls
Graph3
0
0
4
22
38
111
260
512
918
1548
21720
29330
35450
42140
46204
489318
509940
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5156238
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01332
01059
0870
0625
0540
0385
0286
0206
0131
076
3020-302452
3025-30293
3030-30340
3035-30390
3040-30440
3045-30490
masse 23
masse 24
Temps de vol (ns)
nombre de coups
Temps de vol masse 23 et 24 bande en nergie porte 20 ns
Feuil1
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Feuil1
nergie (keV)
nombre de coups
Bande passante nergie masse 23 porte 20 ns
Feuil2
0-10
11-20
21-30
31-40
41-50
51-60
61-70
axe des y
nombre de coups
Image sur le dtecteur masse 23 bande passante ene nergie porte de 20 ns
Feuil3
2770-27742775-27792780-27842785-27892790-27942795-27992800-28042805-28092810-28142815-28192820-28242825-28292830-28342835-28392840-28442845-28492850-28542855-28592860-28642865-28692870-28742875-28792880-28842885-28892890-28942895-28992900-29042905-29092910-29142915-29192920-29242925-29292930-29342935-29392940-29442945-29492950-29542955-29592960-29642965-29692970-29742975-29792980-29842985-29892990-29942995-29993000-30043005-30093010-30143015-30193020-30243025-30293030-30343035-30393040-30443045-3049
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76037
Feuil3
masse 23
masse 24
Temps de vol (ns)
nombre de coups
Temps de vol masse 23 et 24 bande en nergie porte 20 ns
Feuil4
8900-1011-2021-3031-4041-5051-6061-70
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Feuil4
0-10
11-20
21-30
31-40
41-50
51-60
61-70
axe des y
nombre de coups
Image sur le dtecteur masse 24 bande passante ene nergie porte de 20 ns
Feuil5
Feuil6
17800-1011-2021-3031-4041-5051-6061-70
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Feuil6
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Image dtecteur modle proto temps de vol et bande passante nergie, 2keV masse 23
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Image dtecteur modle proto temps de vol et bande passante nergie, 2keV masse 24
17800-1011-2021-3031-4041-5051-6061-70
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0-10
11-20
21-30
31-40
41-50
51-60
61-70
Image dtecteur modle proto temps de vol et bande passante nergie, 2keV masse 24
19501960197019801990200020102020203020402050206020702080209021002110212021302140215021602170218021902200221022202230224022502260227022802290230023102320233023402350236023702380239024002410242024302440245024602470248024902500251025202530254025502560257025802590260026102620263026402650266026702680269027002710272027302740275027602770278027902800
masse 230000228198795258361021071915609198652212222883221092020017990153821308510111771754193668238313977634152071123714200000000000000000
masse 24001227135814043803799112744175712087022091223942135019125170671459012113953470735099342121471343764435248925060000000000000000000
masse 23
masse 24
tranches de 10 ns
nombre de coups
Sparation masses 23 24 modle proto 2keV, hors mdian et bande passante nergie
-
PICAM, quelques photos du QMQM, vue des protections thermiques Capot suprieur avec OSR Kapton aluminis autour partie infrieureQM dans la chambre avec source dions
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PICAM, quelques photos du QMOptique, partie infrieureAnalyseur lectrostatiqueLamelles miroir M1 lectrodes de gatingOptique, partie suprieureVue de dessous