日球层内外能量中性原子的探测
详细信息    查看全文 | 推荐本文 |
  • 英文篇名:Detecting Energetic Neutral Atoms in and out of the Heliosphere
  • 作者:谢克强
  • 英文作者:K C Hsieh;Department of Physics,The University of Arizona;
  • 关键词:能量中性原子 ; 空间等离子体 ; 遥测 ; 日球层 ; 星际介质 ; 电荷交换 ; 粒子探测器
  • 英文关键词:Energetic Neutral Atom(ENA);;Space plasma;;Remote sensing;;Heliosphere;;Interstellar medium;;Charge exchange;;Particle detectors
  • 中文刊名:KJKB
  • 英文刊名:Chinese Journal of Space Science
  • 机构:亚利桑那大学物理系;
  • 出版日期:2015-05-15
  • 出版单位:空间科学学报
  • 年:2015
  • 期:v.35
  • 语种:中文;
  • 页:KJKB201503001
  • 页数:40
  • CN:03
  • ISSN:11-1783/V
  • 分类号:3-42
摘要
能量中性原子(Energetic Neutral Atoms,ENA,简称能原子)是指在日球层内外空间,拥有>0.1 keV动能的原子.在此空间领域并没有温度>10~6K的中性气体,但却充满动能>0.1 keV的正离子.因此能原子A应该是A~+离子与原地稀薄气体B原子或分子交换电荷所产生的,即A~++B→A+B~+.电荷交换涉及极小的动能变化,新生的能原子A和离子B~+基本上各自保持原有动能.离子B~+随即被当地磁场俘获,能原子A则脱离磁场约束并携带其原属离子群的成分和能量信息而直线运动,成为遥测空间等离子体的有效媒介.美国人造卫星IBEX(Interstellar Boundary Explorer)直接探测得到来自日球层以外星际空间的能原子,大幅延伸了利用能原子遥测空间等离子体的领域.本文据此论述了空间能原子的发现,综述了探测空间能原子的基本概念与实例、取得的主要成果、仪器设计和研制进展以及未来空间利用能原子遥测的发展趋势.
        By Energetic Neutral Atoms(ENA),we mean atoms having kinetic energies > 0.1 keV found in and out of the heliosphere.In the regions lacking any neutral gas of temperatures > 10~6 K,while abundant in ions of kinetic energies > 0.1 keV,surely an ENA has to be the product of charge exchange between an ion and an atom or molecule B of the local gas,i.e.A~++B → A+B~+.Because energy exchange is minute during charge exchange,the newly formed ENA A and ion B~+ can be considered keeping their respective original kinetic energies.Instantly,ion B~+ is trapped by the local magnetic field,but ENA A is liberated and flies yonder,to be a sample of its originating plasma in mass and energy,thus providing a precious medium for remote sensing the parent plasma.The recent success of NASA's IBEX(Interstellar Boundary EXplorer) Mission in directly detecting ENA coming from the local interstellar medium greatly expanded the scope of ENA remote sensing.Here,we review the discovery of ENA in high altitudes,the basic concept and existing examples of remote sensing of ENA,recent results,and the designs and development of the necessary instruments,and also offer a prospective on ENA-sensing in the near future.
引文
[1]Wang L,Lin R P,Larson D E,Luhmann J G.Domination of heliosheath pressure by shock-accelerated pickup ions from observation of neutral atoms[J].Nature,2008,454:81
    [2]McComas D J,Alegrini F,Bochsler P,et aL Global observations of the interstellar interaction from the Interstellar Boundary Explorer(IBEX)[J].Science,2009,326:959-962
    [3]Fuselier S A,AUegrini F,Funsten H O,et al.Width and variation of the ENA flux ribbon observed by the Interstellar Boundary Explorer[J].Science,2009,326:962-964
    [4]Funsten H O,AUegrini F,Crew G B,et al.Structures and spectral variations ofthe outer heliosphere in IBEX energetic neutral atom maps[J].Science,2009,326:964-966
    [5]Schwadron N A,Bzowski M,Crew G B,et al.Comparison of Interstellar Boundary Explorer observations with3D global heliospheric models[J].Science,2009,326:966-968
    [6]Mobius E,Bochsler P,Bzowski M,et al.Direct observations of interstellar H,He,and O by the Interstellar Boundary Explorer[J].Science,2009,326:969-971
    [7]Krimigis S M,Mitchell D G,Roelof E C,et al.Imaging the intersection of the heliosphere with the interstellar medium from Saturn with Cassini[J].Science,2009,326:971-973
    [8]McComasD J,Punsten H O,Puselier S A,et al.IBEX observations of heliospheric energetic neutral atoms:current understanding and future direction[J].Geophys.Res.Lett,2011,38:L18101-L18109
    [9]Gurnett D A,Persoon A M,Randall R F,et al.The POLAR plasma wave instrument[J].Space Sci.Rev.,1995,71:597-622
    [10]Gurnett D A,Kurt W S.Electron plasma oscillations upstream of the solar wind termination shock[J].Science,2005,309:2025-2027
    [11]Reinisch B W,Haines D M,Bibl K,et al.The radar plasma imager investigation on the IMAGE spacecraft[J].Space Sci.Rev.,2000,91:319-359
    [12]Green J L,Reinisch B W.An overview of results from RPI on IMAGE[J].Space Sci.Rev.,2003,109:183-210
    [13]Dessler A J.Solar wind and interplanetary magnetic field[J].J.Geophys.Res.,1967,5(1):1-41
    [14]Davis Jr.L.Interplanetary magnetic fields and cosmic rays[J].Phys.Rev.Lett,1955,100:1440-1444
    [15]Parker E N.Interplanetary Dynamical Processes[M].New York:Interscience Publishers,John Wiley&Sons,1963
    [16]Axford W I.The interaction of the solar wind and the interstellar medium[C]//Proceedings of Asilomar Conference.Pacific Grove,CA:NASA,1971:609-660
    [17]Jokipii J R.A shock for Voyager 2[J].Nature,2008,454:38-39
    [18]Patterson T N L,Johnson F S,Hanson W B.The distribution of interplanetary hydrogen[J].Planet.Space Sci.,1963,11:767
    [19]Bertaux J L,Blamont J E.Observation of Lyman-αemission in interplanetary space[C]//Proceedings of Asilomar Conference.Pacific Grove,CA:NASA,1971:661-667
    [20]Thomas G E.Properties of nearby interstellar hydrogen deduced from Lyman-asky background measurements[C]//Proceedings of Asilomar Conference.Pacific Grove,CA:NASA,1971:668-683
    [21]Weller C S,Meier R R.Observation of helium in the interplanetary/interstellar wind:The solar-wake effect[J].Astrophys.J.,1974,193:471-476
    [22]Lallement R,Bertaux J L,Dalaudier F.Interplanetary Lyman-aspectral profiles and intensities for both repulsive and attractive solar force fields:Predicted absorption pattern by a hydrogen cell[J].Astron.Astrophys.,1985,150:21-32
    [23]Ajello J M,Stewart A L,Thomas G E,Graps A.Solar cycle study of interplanetary Lyman-αvariations:Pioneer Venue orbiter sky background results[J].Astrophys.J.,1987,317:964-986
    [24]Lallement R.Relationship between ISM inside and outside the heliosphere[J].Adv.Space Scl,1993,13(6):361-374
    [25]Prisch P C,LISM structure-Fragmented superbubble shell?[J].Adv.Space Set.,1993,13(6):213-222
    [26]Witte M,Rosenbauer H,Banaszkiewicz M,Fahr H.The ULYSSES Neutral Gas Experiment:determination of the velocity and temperature of the interstellar helium[J].Adv.Space Scl,1993,13(6):121-130
    [27]Witte M,Banaszkiewicz M,Rosenbauer H.Recent results on the parameters of the interstellar helium from the ULYSSES/GAS experiment[J].Space Sci.Rev.,1996,78(l/2):289-296
    [28]Geiss J,Witte M.Properties of the interstellar gas in the heliosphere[J].Space Sci.Rev.,1996,78(l/2):229
    [29]Witte M.Kinetic parameters of interstellar neutral helium review of results obtained during one solar cycle with the Ulysses/GAS-instrument[J].Astron.Astrophys.,2004,426:835-844
    [30]Vasyliunas V M,Siscoe G L.On the flux and the energy spectrum of interstellar ions in the solar system[J].J.Geophys.Res.,1976,81:1247
    [31]Mobius E,Hovestadt D,Klecker B,et al.Direct observation of He~+pick-up ions of interstellar origin in the solar wind[J].Nature,1985,318:426-429
    [32]Gloeckler G,Geiss J,BalsigerH,et al.Detection of interstellar pick-up hydrogen in the solar system[J].Science,1993,261:70
    [33]Kallenbach R,Geiss J,Gloeckler G,Steiger Von R.Pickup ion measurements in the heliosphere-A review[J].Astrophys.Space Sci.,2000,274:97
    [34]Gloeckler G,Mobius E,Geiss J,et al.Coordinated observation of local interstellar helium in the heliosphere:Observations of the helium focusing cone with pickup ions[J].Astron.Astrophys.,2004,426:845-854
    [35]Gloeckler G,Geiss J.Composition of the local interstellar medium as diagnosed with pickup ions[J].Adv.Space Res.,2004,34(l):53-60
    [36]Bzowski M,Sokot J M,Tokumaru M,et al.Solar parameters for modeling interplanetary background[R]//Crosscalibration of Past and Present Far UV Spectra of Solar System Objects and the Heliosphere.New York:Springer,2013:67-138
    [37]Gruntman M.Elastic collisions of interstellar helium atoms with solar wind protons[J].J.Geophys.Res.,2013,118:1-13
    [38]Scherer K,Fichter H,Marsch E.Anomalous cosmic rays[M]//The Outer Heliosphere:Beyond the Planets.Katlenburg-Lindau:Corpernicus Gesellschaft,2000:191-216
    [39]Gruntman M.Energetic neutral atom imaging of space plasmas[J].Rev.Sci.Instrum.,1997,68(10):3617-3656
    [40]Meinel A B.Doppler shifted auroral hydrogen emission[J].Astrophys.J.,1951,113:50-54
    [41]Meinel A B,Fan C Y.Laboratory reproduction of auroral emission by proton bombardment[J].Astrophys.J.,1952,115:330-331
    [42]Fan C Y,Meinel A B.Laboratory ionic-impact emission spectra[J].Astrophys.J.,1953,118:205-213
    [43]Fan C Y,Schulte D H.Variations in the auroral spectrum[J].Astrophys.J.,1954,120:563-565
    [44]Bernstein W,Inouye G T,Sanders N L,Wax R L.Measurements of precipitated 1~20 keV protons and electrons during a breakup aurora[J].J.Geophys.Res.,1969,74(14):3601-3608
    [45]Allison S K.Experimental results on charge-changing collisions of hydrogen atoms and ions at kinetic energies above 0.2keV[J].Rev.Mod.Phys.,1958,30(4):1137-1168
    [46]Chamberlain J W.Physics of Aurora and Airglow[M].New York:Academic Press,1961
    [47]Evans D S.Low energy charged particle detection using the continuous channel electron multiplier[J].Rev.Sci.Instr.,1965,36(3):375-382
    [48]Wax R L,Simpson W R,Bernstein W.Large fluxes of1~4 keV atomic hydrogen at 800 km[J].J.Geophys.Res.,1970,75(31):6390-6393
    [49]Wax R L,Bernstein W.Energy-independent detector for total hydrogen fluxes in the range l~10keV for space and laboratory applications[J].Rev.Sci.Instr.,1967,38(11):1612-1615
    [50]Bernstein W,Wax R L,Sanders N L,Inouye G T.An energy spectrometer for energetic(1~25 keV)neutral hydrogen atoms[C]//Small Rocket Instrument Technology,Proceedings of COSPAR Symposium.Amsterdam,NorthHolland:COSPAR,1969
    [51]Moritz J.Energetic protons at low equatorial altitude:A newly discovered radiation belt phenomenon and its explanation[J].Z.Geophys.,1972,38:701
    [52]Hovstadt D,Hausler B,Scholer M.Observation of energetic particles at very low altitudes near the geomagnetic equator[J].Phys.Rev.Lett.,1972,28(20):1340-1344
    [53]Mizera P F,Blake J B.Observation of ring current protons at low altitudes[J].J.Geophys.Res.,1973,78(7):1058-1062
    [54]Stuart G W.Satellite-measured radiation[J].Phys.Rev.Lett,1959,2:417-418
    [55]Dessler A J,Parker E N.Hydromagnetic theory of geomagnetic storms[J].J.Geophys.Res.,1959,64(12):2230-2252
    [56]Tinsley B A.Neutral atom precipitation-A review[J].J.Atmos.Terr.Phys.,1981,43(5/6):617-632
    [57]Roelof E C,Mitchell D G,Williams D J.Energetic neutral atoms(E~50 keV)from the ring current:IMP 7/8 and ISEE 1[J].J.Geophys.Res.,1985,90(11):10991-11008
    [58]Roelof E C.Energetic neutral atom image of a storm-time ring current[J].Geophys.Res.Lett,1987,14(6):652-655
    [59]Sullivan J D.Geometrical factor of directional response of single and multi-element particle telescopes[J].Nucl.Instr.Meth.,1971,95:5-11
    [60]Barnett C F,Hunter H T,Kirkpatrick M I,et al.Collisions of H,H_2,He and Li atoms and ions with atoms and molecules[R]//Atomic Data for Fusion,ORNL-6086-VI.Oak Ridge,Tennessee:Oak Ridge National Laboratory,1990
    [61]Lindsay B G,Stebbings R F.Charge transfer cross sections for energetic neutral atom data analysis[J].J.Geophys.Res.,2005,110:A12213,doi:10.1029/2005JA011298
    [62]Hu W,Fang D,Wang Y,Yang F.Electron-impactionization cross section for the hydrogen atom[J].Phys.Rev.A.,1994,49(2):989-991
    [63]Palenius H P,Kohl J L,Parkinson W H.Absolute measurement of the photoionization cross section of atomic hydrogen with a shock tube for the extreme ultraviolet[J].Phys.Rev.A,1976,13(5):1805-1816
    [64]Yan M,Sadeghpour R,Dalgarno A.Photoionization cross sections of He and H_2[J].Astrophys.X,1998,496:1044-1050
    [65]Zoennchen J H,Nass U,Lay G,FahrH J.3-D-geocoronal hydrogen density derived from TWINS Ly-α-data[J].Ann.Geophys.,2010,28:1221-1228
    [66]McComas D J,Dayeh M A,Allegrini F,et al.The first three years of IBEX observations and our evolving heliosphere[J].Astrophys.J.Supp.,2012,203:1-36
    [67]Mitchell D G,Hsieh K C,Curtis C C,et al.Imaging of the Earth's ring current in energetic neutral atoms[J].Geophys.Res.Lett,2001,28(6):1151-1154
    [68]Burch JL.Magnetospheric Imaging-The IMAGE Prime Mission[M].Dordrecht,the Netherlands:Kluwer Academic Publishers,2003
    [69]Kirsch E,Krimigis S M,Kohl J W,Keath E P.Upper limits for X-ray and energetic neutral particle emission from Jupiter:Voyager 1 results[J].Geophys.Res.Lett,1981,8:169
    [70]Kirsch E,Krimigis S M,Ip WH,Gloeckler G.X-ray and energetic neutral particle emission from Saturn's magnetosphere[J].Nature,1981,292:718-721
    [71]Cheng A F.Energetic particles from Jupiter and Saturn[J].J.Geophys.Res.,1986,9:4524-4530
    [72]Hsieh K C,Curtis C C.A model for the spatial and energy distributions of energetic neutral atoms produced within the Saturn/Titan plasma[J].Geophys.Res.Lett,1988,15(8):772-775
    [73]Acuan M H,Connerney J E P,Ness N F.The ZS zonal harmonic model of Saturn's magnetic field:analysis and implications[J].J.Geophys.Res.,1983,88(A11):8771-8789
    [74]Armstrong T P,Paonessa M T,BellII E V,Krimigis S M.Voyager observations of Saturnian ion and electron phase space densities[J].J.Geophys.Res.,1983,88(A11):8893-8904
    [75]Hilton D A,Hunten D M.A partial collisional model of the Titan hydrogen torus[J].Icaurus,1988,73:248-268
    [76]Krimigis S M,Mitchell D G,Hamilton D C,et al.Magnetosphere Imaging Instrument(MIMI)on the Cassini Mission to Saturn/Titan[J].Space Sci.Rev.,2004,114:233-329
    [77]Krimigis S M,MitchellDG,Hamilton DC,et al.Dynamics of Saturn's Magnetosphere from MIMI during Cassini's orbital insertion[J].Science,2005,307(5713):1271-1273
    [78]Lundin R,Barabash S,Andersson H,et al.Solar windinduced atmospheric erosion at Mars:first results from ASPERA-3 on Mars Express[J].Science,2004,305:1933-1936
    [79]Mura A,Orsini S,Milillo A,et al.ENA detection in the dayside of Mars:ASPERA-3 NPD statistical study[J].Planet.Space Sci.,2008,56(6):840-845
    [80]Galli A,Wurz P,Bochsler P,et al.First observation of energetic neutral atoms in the Venus environment[J].Planet.Space Sci.,2008,56(6):807-811
    [81]Galli A,Fok M C,Wurz P,et al.Tailward flow of energetic neutral atoms observed at Venus[J].J.Geophys.Res.,2008,113,E00B15doi:10.1029/2008JE003096
    [82]Yoshifumi F,Chaufray J Y,Smith H T,et al.Exospheres and energetic neutral atoms of Mars,Venus and Titan[J].Space Sci.Rev.,2011,162(l-4):213-266
    [83]Fahr H J.Influence of interstellar matter on the density of atmospheric hydrogen[J].Ann.Geo-phys.,1969,25:475
    [84]Blum P W,Fahr H J.Interaction between interstellar hydrogen and the solar wind[J].Astron.Astrophys.,1970,4:280
    [85]Baranov V B,Krasnobaev K V.Gidrodinamicheskaya Teoriya Kosmicheskoj Plazmy[M].Nauka,Moskva,1977(in Russian)
    [86]Holzer T E.Neutral hydrogen in interplanetary space[J].Rev.Geophys.Space Phys.,1977,15:467-490
    [87]Thomas G E.The interstellar wind and is influence on the interplanetary environment[J].Ann.Rev.Earth Planet.Sci.,1978,6:173
    [88]Holzer T E.Interaction between the solar wind and the interstellar medium[J].Ann.Rev.Astron.Astrophys.,1989,27:199-234
    [89]Suess S T.The heliopause[J].Rev.Geophys.,1990,28(1):97-115
    [90]Baranov V B.Gas dynamics of the solar wind interaction with the interstellar medium[J].Space Sci.Rev.,1990,52:90-120
    [91]Grzedzielski,S,Page D E.COSPAR Colloquia Series Volume 1-Physics of the Outer Heliosphere[M].Oxford:Pergamon Press,1990
    [92]Hsieh K C,Shih K L,Jokipii J R,Grzedzielski S.Probing the heliosphere with energetic hydrogen atoms[J].Astrophys.J.,1992,393:756-763
    [93]Hsieh K C,Shih K L,Jokipii J R,Gruntman M A.Sensing the solar-wind termination shock from the Earth's orbit[C]//Proceedings of the Third COSPAR Symposium.New York:Pergamon,1992:365-368
    [94]Hsieh K C,Curtis C C,Fan C Y,Gruntman M A.Techniques for the remote sensing of space plasma in the heliosphere via energetic neutral atoms:A review[C]//Proceedings of the Third COSPAR Symposium.New York:Pergamon,1992:357-364
    [95]Hsieh K C,Gruntman M A.Viewing the outer heliosphere in energetic neutral atoms[J].Adv.Space Res.,1993,33(6):131-139
    [96]Hovestadt D,Hilchenbach M,Burgi A,et al.CELIAS-Charge,Element and Isotope Analysis System for SOHO[J].Solar Physics,1995,162:441-481
    [97]Hilchenbach M,Hsieh K C,Hovestadt D,et al.Detection of 55~80 keV hydrogen atoms of heliospheric origin by CELIAS/HSTOF on SOHO[J].Astrophys.J.,1998,503(2):916-922
    [98]Hilchenbach M,Hsieh K C,Hovestadt D,Kallenbach R,Czechowski A,Mobius E,Bochsler P.Energetic neutral hydrogen of heliospheric origin observed with SOHO/CELLIAS at 1AU[C]//Proceedings of COSPAR Colloquium.Amsterdam:Pergamon,2001:273-276
    [99]Hilchenbach M,Czechowski A,Hsieh K C,Kallenbach R.Observations of energetic neutral atoms and their implications on modeling the heliosheath[J].AIP Conf.Proc,2006,858:276-281
    [100]Czechowski A,Fichtner H,Grzedzielski S,et al.Anomalous cosmic rays and generation of energetic neutrals in the region beyond the terminations shock[J].Astron.&Astrophys.,2001,368:622-634
    [101]KotaJ,Hsieh K C,Jokipii J R,et al.Viewing co-rotating interaction regions globally using energetic neutral atoms[J].J.Geophys.Res.,2001,106:24907-24 914
    [102]Fan C Y,Gloeckler G,Simpson J A.Proton and helium nuclei within interplanetary regions which corotate with the Sun[J].Proc.Int.Conf.Cosm.Ray,1965,1:109
    [103]Tsurutani B T,Smith E J,Pyle K R,Simpson J A.Energetic protons accelerated at corotating shocks from 1 to6AU[J].J.Geophys.Res.,1982,87:7389
    [104]Smith E J.Interplanetary shock phenomena beyond1 AU[R]//Collisionless Shocks in the Heliosphere:Reviews and Current Research.Washington,DC:American Geophysical Union,1985:69-83
    [105]Gosling J T,Bame S J,McComasD J,et al.Latitudinal variation of solar wind corotating interaction stream regions:Ulysses[J].Geophys.Res.Lett.,1993,20:2789
    [106]Mason G M,Sanderson T R.CIR-associated energetic particles in the inner and middle heliosphere[J].Space Sci.Rev.,1999,98:11
    [107]Keppler E.The acceleration of charged particles in corotating interaction regions(CIR)-A review with particular emphasis on the Ulysses mission[J].Surv.in Geophys.,1998,19:221
    [108]Mobiusl E,Bzowski M,Chalov S,et al.Coordinated observation of local interstellar helium in the heliosphere:Synopsis of the interstellar He parameters from combined neutral gas,pickup ion and UV scattering observations and related consequences[J].Astron.Astrophys.,2004,426:879-907
    [109]Hsieh K C,Giacalone J,Czechowski A,et al.Thickness of the heliosheath,return of the pick-up ions,and Voyager l's crossing the heliopause[J].Astrophys.J.Lett.,2010,718:L185-L188
    [110]Czechowski A,Hilchenbach M,Hsieh K C,et al.Estimating the thickness of the heliosheath form CELIAS/HSTOF and Voyager 1 data[J].Astrophys.J.Lett.,2006,647(1):L69-L72
    [111]Czechowski A,Hilchenbach M,Hsieh K C,et al.Imaging the heliosphere using HSTOF energetic neutral atoms and Voyager 1 ion data[J].Astron.&Astrophys.,2008,487:329-335
    [112]Stone E C,CummingsA C,McDonald F B,et al.Voyager 1 observes low-energy galactic cosmic rays in a region depleted of heliospheric ions[J].Science,2013,341(6142):150-152
    [113]Bzowski M,Mobius E,Tarnopolski S,et al.Neutral H Density at the Termination Shock:A Consolidation of Recent Results[J].Space Sci.Rev.,2009,143:177-190
    [114]McComas D J,Zank G P,Schwadron N A.Interstellar Boundary Explorer(IBEX)[M].New York:SpringerVerlag,2009
    [115]Fuselier S A,Funsten H O,Heirtzler D,et al.Energetic neutral atoms from the Earth's sub-solar magnetosphere[J].Geophys.Res.Lett,2010,37:L13101-L13105
    [116]Petrinec S M,Dayeh M A,Funsten H O,et al.Neutral atom imaging of the magnetospheric cusps[J].J.Geophys.Res.,2011,116:A07203-A07210
    [117]McComas D J,Dayeh M A,Funsten H O,et al.First IBEX observations of the terrestrial plasma sheet and a possible disconnection event.J.Geophys.Res.,2011,116:A02211-02217
    [118]McComas D J,Allegrini F,Bochsler P,et al.Lunar backscatter and neutralization of the solar wind:first observations of neutral atoms from the Moon[J].Geophys.Res.Lett,2009,376:L12104-L12107
    [119]McComas D J.Interstellar Boundary Explorer(IBEX):Direct sampling of the interstellar medium[J].Astrophys.J.Supp.Ser.,2012,198(2):8,doi:10.1088/0067-0049/198/2/8
    [120]Desai M I,Allegrini F,Bzowski M,et al.Energetic neutral atoms measured by the Interstellar Boundary Explorer(IBEX):evidence of multiple heliosheath population[J].Astrophys.J.,2014,780(1):98-110
    [121]Heerikhuisen J,Pogorelov N V,Zank G P,et al.Pickup ions in the heliosphere:A possible mechanism for the Interstellar Boundary Explorer ribbon[J].Astrophys.J.Lett,2010,708(2):L126-L130
    [122]Schwadron N A,Allegrini F,Bzowski M,et al.Separation of the IBEX ribbon from globally distributed energetic neutral atom flux[J].Astrophys.J.,2011,731:56-77doi:10.1088/0004-637X/731/l/56.
    [123]Jokipii J R,Giacalone J,Hsieh K C,Kota J.The structure of the IBEX ribbon:a reflection of interstellar turbulence[J].AIP Conf.Proc,2010,1302:92-97
    [124]McComas D J,Lewis W S,Schwadron N A.IBEX's enigmatic Ribbon in the sky and its many possible sources[J].Rev.Geophys.,2014,52:118-155
    [125]Bzowski M,Kubiak M A,Mobius E,et al.Neutral interstellar helium parameters based on IBEX-Lo observations and test particle calculations[J].Astroph.J.,Suppl.Ser.,2012,198(2):27,doi:10.1088/0067-0049/198/2/12
    [126]Saul L,Wurz P,Rodriguez D,et al.Local interstellar neutral hydrogen sampled in-situ by IBEX[J].Astrophys.J.Supp.,2012,198:9,doi:10.1088/0067-0049/198/2/14
    [127]Bochsler P,Petersen L,Mobius E,et al.Estimation of the neon/oxygen abundance ratio at the heliospheric termination shock and in the local interstellar medium from IBEX observations[J].Astrophys.J.Suppl.Ser.,2012,198(2):5,doi:10.1088/0067-0049/198/2/13
    [128]Cummings A C,Stone E C,Steenberg C D.Composition of anomalous cosmic rays and other heliosphere[J].Astrophys.J.,2002,578:194-210
    [129]Izmodenov V V,Lallementl R,Geiss J.Interstellar oxygen in the heliospheric interface:Influence of electron impact ionization[J].Astron.&Astrophys.,1999,344:317-321
    [130]Slavin,J D,Frisch P C.The boundary conditions of the heliosphere:photoionization models constrained by interstellar and in situ data[J].Astron.Astrophys.,2008,491(1):53-68,doi:10.1051/0004-6361:20078101
    [131]Glockler G,Fisk L A.Johannes Geiss'investigations of solar,heliospheric and interstellar matter[J].Space Sci.Rev.,2007,130:489-513
    [132]Miiller H R,Zank G P.Heliospheric filtration of interstellar heavy atoms:Sensitivity to hydrogen background[J].J.Geophys.Res.,2004,109:A07104,doi:10.1029/2003-JA010269
    [133]Izmodenov V,Malama Y,Gloecler G,Geiss J.Filtration of interstellar H,O,N atoms through the heliospheric interface:Inferences on local interstellar abundances of the elements[J].Astron.&Astrophys.,2004,414(3):L29-L32
    [134]Hllond M,Bzowski M,Mobius E,et al.Precision pointing of IBEX-Lo observations[J].Astroph.J.,Suppl.Ser.,2012,198(2):14,doi:10.1088/0067-0049/198/2/9.
    [135]Lee M A,Kucharek H,Mobius E,et al.An analytic model of interstellar gas in the heliosphere tailored to Interstellar Boundary Explorer observations[J].Astrophys.J.Suppl.Ser.,2012,198(2):13,doi:10.1088/0067-0049/198/2/10
    [136]Mobius E,Bochsler P,Bzowski M,et al.Interstellar gas flow parameters derived from Interstellar Boundary Explorer-Lo observations in 2009—2010:Analytical analysis[J].Astrophys.J.Suppl.Ser.,2012,198(2):(18pp)doi:10.1088/0067-0049/198/2/ll
    [137]McComas D J,Alexashov D,Bzowski M,et al.The heliosphere's interstellar interaction:No bow shock[J].Science,2012,336:1291-1923
    [138]Gurnett D A,Kurth W S,Burlaga L F,Ness N F.In-situ observations of interstellar plasma with Voyager 1[J].Science,2013,341:1489-1492,doi:10.1126/science.l241681
    [139]Burlaga L F,Ness N F.Voyager 1 observations of the interstellar magnetic field and the transition from the heliosheath[J].Astrophys.J.,2014,784(8):146-159,doi:10.1088/0004-637X/784/2/146
    [140]Pfaff R F,Borovsky J E,Young D T.Measurement techniques for space plasma:Fields and particles[J].Geophys.Monogr.Ser.,1998,103:235-304
    [141]Voss H D,Hertzberg E,Ghielmetti A G,et al.Medium energy ion mass and neutral atom spectrometer[J].J.Spacecr.Rockets,1992,29(4):566-569
    [142]Barabash S,Norberg O,Lundin R,et al.Energetic neutral atom imager on the Swedish Microsatellite Astrid[M]//Measurement Techniques in Space Plasma Fields.Washington DC:American Geophysical Union,1998,doi:10.1002/9781118664391.ch32
    [143]Mitchell D G,Jaskulek S E,Schlemm C E,et al.High energy neutral atom(HENA)imager for the IMAGE mission[J].Space Sci.Rev.,2000,91:67-112
    [144]Pollock C J,Asamura K,Baldonado J,et al.Medium energy neutral atom(MENA)imager for the IMAGE mission[J].Space Sci.Rev.,2000,91:113-154
    [145]Moore T E,Chornay D J,Collier M R,et al.The lowenergy neutral atom imager for IMAGE[J].Space Sci.Rev.,2000,91:155-195
    [146]Barabash S,Lundin R,Andersson H,et al.The analyzer of space plasmas and energetic atoms(ASPERA-3)for the Mars Express Mission[J].Space Sci.Rev.,2006,126(1-4):113-164
    [147]Barabash S,Sauvaud J J,Gunell H,et al.The analyzer of space plasmas and energetic atoms(ASPERA-4)for the Venus Express Mission[J].Planet.&Space Sci.,2007,55(12):1772-1792
    [148]Orsini S,Cerulli-Irelli P,Maggi M,et al.Imaging Earth's magnetosphere:Measuring energy,mass,and direction of energetic neutral atoms with the ISENA instrument[M]//Measurement Techniques for Space Plasma:Fields and Particles.Washington D C:American Geophysical Union,1998:269-274
    [149]GloecklerG,Hsieh K C.Time-of-flight technique for particle identification at energies from 2~400 keV/nucleon[J].Nucl.Instr.Meth.,1979,165:537-544
    [150]Martin C,Jelinsky P,Lampton M,et al.Wedge-andstrip anodes for centroid-finding position-sensitive photon and particle detectors[J].Rev.Sci.Instrum.,1981,52(7):1067-1074
    [151]Wilken B,Stiidermann W.A compact time-of-flight mass spectrometer with electrostatic mirror[J].Nucl.Meth.Instr.,1984,222:587-600
    [152]Hsieh K C,Keppler E,Schmidtke G.Forward photoemission from thin carbon foils[J].Appl.Opt.,1979,18:3732-3733
    [153]Hsieh K C,Keppler E,Schmidtke G.Extreme ultra-violet induced forward photoemission from thin carbon foils[J].J.Appl.Phys.,1980,51(4):2242-2246
    [154]McComas D J,Allegrini F,Pollock C J,et al.Ultrathin(10 nm)carbon foils in space instrumentation[J].Rev.Sci.Instrum.,2004,75(ll):4863-4870
    [155]Drake V A,Sandel B R,Jenkins D G,Hsieh K C.H Lyαtransmittance of thin foils of C,Si/C,and Al/C for keV particle detectors[J].SPIE Techn.Conf.,1992,1744:148-160
    [156]Funsten H O,McComas,D J,Gruntman M A.Neutral atom imaging:UV rejection techniques[M]//Measurement Techniques for Space Plasma:Fields and Particles.Washington D C:American Geophysical Union,1998:251-256
    [157]Gruntman M A,Kozochkina A A,Leonas V B.Multielectron secondary emission of thin foils bombarded by accelerated atomic beam[J].JETP Letters,1990,51(10):22-25
    [158]Shaw A,Hsieh K C,Hilchenbach M,et al.Energetic neutral helium of heliospheric origin at 1AU[M]//COSPAR Colloquia Series-The Outer Heliosphere:The New Frontiers.Amsterdam:Pergamon,2001:219-222
    [159]Funsten H O,Allegrini F,Bochsler P,et al.The Interstellar Boundary Explorer High Energy(IBEX-Hi)neutral atom imager[J].Space Sci.Rev.,2009,146:75-103
    [160]Fuselier S A,Bochsler P.Chornay D,Clark G,Crew G B,Dunn G,et al.The IBEX-Lo sensor[J].Space Sci.Rev.,2009,146:117-147
    [161]McComas D J,Allegrini F,Bochsler P,et al.IBEXinterstellar boundary explorer[J].Space Sci.Rev.,2009,146:11-33
    [162]Witte M,Rosenbauer H,Keppler E,et al.The interstellar neutral-gas experiment on ULYSSES[J].Astron.Astrophys.Suppl.Ser.,1992,92:333-348
    [163]Witte M,Bleszynski S,Banaszkiewicz M,Rosenbauer M.Sputtering efficiency of LiF surfaces on impact of low energy neutral helium 20~80eV:Calibration of the interstellar neutral helium instrument on ULYSSES[J].Rev.Sci.Instrum.,1999,70:4404-4411
    [164]Wurz P,Schletti R,Aellig M R.Hydrogen and oxygen negative ion production by surface ionization using diamond surfaces[J].Surf.Sci.,1997,373:56-66
    [165]Aellig M R,Wurz P,Schletti R,et al.Surface ionization with cesiated converters for space application[M]//Measurement Techniques in Space Plasma Fields.Washington D C:American Geophysical Union,1998:289-296
    [166]Wieser M,Wurz P.Production of a 10~1000 eV neutral particle beam using surface neutralization[J].Meas.Sci.Tech.,2005,16(12):2511-2516
    [167]Mobius E,Kistler L M,Popecki M,Crocker K,Granoff M,Jiang Y,et al.The 3-D plasma distribution function analyzers with time-of-flight mass discrimination for CLUSTER,FAST and Equator-S,measurement techniques in space plasmas[M]//Measurement Techniques in Space Plasma Fields.Washington D C:American Geophysical Union,1998:243-248
    [168]Wieser M,Wurz P,Mobius E,et al.The ion-optical propotype of the low energy neutral atoms sensor of the Interstellar Boundary Explorer Mission(IBEX)[J].Rev.Sci.Instr.,2007,78:124 502-124 516
    [169]Orsini S,Livi S,Torkar K,et al.SERENA:A suite of four instruments(ELENA,STROFIO,PICAM and MIPA)on board BepiColombo-MPO for particle detection in the Hermean environment[J].Planet.Space Sci.,2010,58:166181
    [170]Milillo A,Orsini S,Hsieh K C,et al.Observing planets and small bodies in sputtered high-energy atom(SHEA)fluxes[J].J.Geophys.Res,2011,116:A07229,doi:10.1029/2011JA016530
    [171]Orsini S,Selci S,Di Lellis A M,et al.The BepiColombo Senrean/ELENA instrument:Performance and testing[C]//European Geosciences Union General Assembly.Vienna,Austria:European Geosciences Union,2013
    [172]Milillo A,Orsini S,Plainaki C,et al.Energetic neutral particles detection in the environment of Jupiter's icy moons:Ganymede's and Europa's neutral imaging experiment(GENIE)[J].Planet.Space Sci.,2013,88:53-63
    [173]Hsieh K C,Zurbuchen T H,Orr J,et al.A collimator design for monitoring heliospheric energetic neutral atoms at 1AU[J].Adv,Space Res.,2004,34:213-218
    [174]Lu Li,S McKenna-Lawlor,J Balaz,et al.Technical configuration and simulation of NAIS-H for the MIT mission[J].Chin.J.Space Sci,2014,34(3):341-351.In Chinese(ISA,McKenna-Lawlor S,Balaz J,等.中性原子成像探测的物理设计与仿真[J].空间科学学报,2014,34(3):341-351)
    [175]McKenna-Lawlor S,Balaz J,Strharsky I,et al.An overview of the scientific objectives and technical configuration of the Neutral Atom Detector Unit(NUADU)for the Chinese Double Star Mission[J].Planet.Space Sci.,2005,53(1-3):335-348
    [176]Mewaldt R A,Leske R A,Stone E C,et al.STEREO observations of energetic neutral hydrogen atoms during the 2006 December 5 solar flare[J].Astrophys.J.Lett,2009,693:L11-L15
    [177]Mewaldt R A,Cohen C M S,Cook R W,et al.The LowEnergy Telescope(LET)and SEP central electronics for the STEREO mission[J].Space Sci.Rev.,2008,136:285-362
    [178]Hsieh K C,Shih K L,McComas D J,et al.Forecasting the arrival of fast coronal mass ejecta at Earth by the detection of 2~20 keV neutral atoms[C]//Proceeding SPIE International Symposium on Optical Applied Science and Engineering.San Diego:SPIE,1992:72-78
    [179]Gruntman M A,Hsieh K C.Neutral solar wind properties:Advance warning of major geomagnetic storms[J].J.Geophys.Res.,1994,99(A10):19213-19227
    [180]Hsieh K C,Frisch P C,Giacalone J,et al.A re-interpretation of the STEREO/STE observations and its consequences[J].Astrophys.J.Lett,2009,694:L79-L82
    [181]Collier M R,Moore T M,Simpson D,et al.An unexplained 10~40°shift in the location of some diverse neutral atom data at 1AU[J].Adv.Space Sci.,2004,34:199-171
    [182]Galli A,Wurz P,Barabash S,et al.Direct measurement of energetic neutral hydrogen in the interplanetary medium[J].Astrophys.J.,2006,644(2):1317-1325
    [183]Brandt J C,Hunten D M.One ejection of neutral hydrogen from the Sun and the terrestrial consequences[J].Planet.Space Sci.,1966,14:95-105
    http://www.ifsi-roma.inaf.it/serena/index.php?categoryid=1

© 2004-2018 中国地质图书馆版权所有 京ICP备05064691号 京公网安备11010802017129号

地址:北京市海淀区学院路29号 邮编:100083

电话:办公室:(+86 10)66554848;文献借阅、咨询服务、科技查新:66554700