MMS observation of inverse energy dispersion in shock drift accelerated ions
暂无分享,去创建一个
R. Gold | B. Mauk | G. Ho | I. Cohen | R. Torbert | D. Sibeck | J. Burch | Y. Wang | K. Hwang | C. Russell | G. Mason | B. Giles | H. Wei | S. Lee | C. Chu | M. D. Silveira
[1] M. Lester,et al. Inverse energy dispersion of energetic ions observed in the magnetosheath , 2016 .
[2] D. Baker,et al. Observations of energetic particle escape at the magnetopause: Early results from the MMS Energetic Ion Spectrometer (EIS) , 2016 .
[3] U. Gliese,et al. Fast Plasma Investigation for Magnetospheric Multiscale , 2016 .
[4] Thomas E. Moore,et al. Magnetospheric Multiscale Overview and Science Objectives , 2016 .
[5] Wolfgang Baumjohann,et al. The Magnetospheric Multiscale Magnetometers , 2016 .
[6] M. R. Stokes,et al. The Energetic Particle Detector (EPD) Investigation and the Energetic Ion Spectrometer (EIS) for the Magnetospheric Multiscale (MMS) Mission , 2016 .
[7] Wolfgang Baumjohann,et al. The FIELDS Instrument Suite on MMS: Scientific Objectives, Measurements, and Data Products , 2016 .
[8] E. Möbius,et al. The free escape continuum of diffuse ions upstream of the Earth's quasi‐parallel bow shock , 2013 .
[9] A. Spitkovsky,et al. ION ACCELERATION IN NON-RELATIVISTIC ASTROPHYSICAL SHOCKS , 2011, 1107.0762.
[10] R. Yamazaki,et al. RELATIVISTIC ELECTRON SHOCK DRIFT ACCELERATION IN LOW MACH NUMBER GALAXY CLUSTER SHOCKS , 2011, 1109.0070.
[11] B. Klecker,et al. Multipoint observations of ions in the 30–160 keV energy range upstream of the Earth's bow shock , 2009 .
[12] I. Dandouras,et al. On the edge of the foreshock: model-data comparisons , 2008 .
[13] J. Slavin,et al. Three‐dimensional position and shape of the bow shock and their variation with upstream Mach numbers and interplanetary magnetic field orientation , 2005 .
[14] E. Möbius,et al. Multi‐spacecraft observations of diffuse ions upstream of Earth's bow shock , 2004 .
[15] M. Pastoriza,et al. Sample of minor merger of galaxies : optical CCD surface photometry and HII region properties , 2004, astro-ph/0409150.
[16] J. Giacalone. Large-Scale Hybrid Simulations of Particle Acceleration at a Parallel Shock , 2004 .
[17] P. Louarn,et al. Observation of energy-time dispersed ion structures in the magnetosheath by CLUSTER: possible signatures of transient acceleration processes at shock , 2003 .
[18] N. Hasebe,et al. Ring current oxygen ions escaping into the magnetosheath , 2001 .
[19] A. Szabo,et al. Solar wind preconditioning in the flank foreshock: IMP 8 observations , 2001 .
[20] N. Paschalidis,et al. Energy time dispersion of a new class of magnetospheric ion events observed near the Earth’s bow shock , 2000 .
[21] Louis J. Lanzerotti,et al. Electron, Proton, and Alpha Monitor on the Advanced Composition Explorer spacecraft , 1998 .
[22] S. M. Krimigis,et al. The Ultra-Low-Energy Isotope Spectrometer (ULEIS) for the ACE spacecraft , 1998 .
[23] S. Krimigis,et al. Characteristics of upstream energetic (E≥50 keV) ion events during intense geomagnetic activity , 1998 .
[24] G. Le,et al. ULF waves in the foreshock , 1995 .
[25] M. Hilchenbach,et al. Statistical analysis of diffuse ion events upstream of the Earth's bow shock , 1994 .
[26] S. Kahler. Injection profiles of solar energetic particles as functions of coronal mass ejection heights , 1994 .
[27] J. Meyer,et al. Energetic-particle abundances in impulsive solar flare events , 1994 .
[28] R. Decker. Shock Drift Acceleration , 1992 .
[29] H. Kucharek,et al. Ion injection and Fermi acceleration at Earth's bow shock : the 1984 September 12 event revisited , 1992 .
[30] Wolfgang Baumjohann,et al. Upstream pressure variations associated with the bow shock and their effects on the magnetosphere , 1990 .
[31] Wolfgang Baumjohann,et al. The Magnetospheric Response to 8-Minute Period Strong-Amplitude Upstream Pressure Variations , 1989 .
[32] D. Baker,et al. The magnetosphere as a sufficient source for upstream ions on November 1, 1984 , 1988 .
[33] R. Decker,et al. Computer modeling of test particle acceleration at oblique shocks , 1988 .
[34] S. Krimigis,et al. Simultaneous measurements of energetic ion (≥50 keV) and electron (≥220 keV) activity upstream of Earth's bow shock and inside the plasma sheet: Magnetospheric source for the November 3 and December 3, 1977 upstream events , 1987 .
[35] S. Krimigis,et al. Energetic magnetospheric ions at the dayside magnetopause: Leakage or merging? , 1987 .
[36] D. Ellison,et al. Diffusive shock acceleration - comparison of a unified shock model to bow shock observations , 1987 .
[37] D. Burgess. Shock drift acceleration at low energies , 1987 .
[38] David G. Sibeck,et al. Magnetospheric particle injection and the upstream ion event of September 5, 1984 , 1986 .
[39] S. Krimigis,et al. Magnetospheric origin of energetic (E ≥ 50 keV) ions upstream of the bow shock: The October 31, 1977, event , 1986 .
[40] Reuven Ramaty,et al. Shock acceleration of electrons and ions in solar flares , 1985 .
[41] D. Ellison. Shock acceleration of diffuse ions at the Earth's bow shock: Acceleration efficiency and A/Z enhancement , 1985 .
[42] C. Russell,et al. Patterns of potential magnetic field merging sites on the dayside magnetopause , 1984 .
[43] R. Decker. Formation of shock‐spike events at quasi‐perpendicular shocks , 1983 .
[44] E. Sarris,et al. Dominant acceleration processes of ambient energetic protons (E ⩾ 50 keV) at the Bow Shock: Conditions and limitations , 1983 .
[45] Martin A. Lee. Coupled hydromagnetic wave excitation and ion acceleration upstream of the earth's bow shock , 1982 .
[46] E. Stone,et al. Energetic electrons in the magnetosheath and upstream of the bow shock , 1982 .
[47] G. Gloeckler,et al. Temporal development of composition, spectra, and anisotropies during upstream particle events , 1981 .
[48] N. Sckopke,et al. Characteristics of reflected and diffuse ions upstream from the earth's bow shock , 1981 .
[49] A. Galvin,et al. A Statistical survey of Ions Observed Upstream of the Earth's Bow Shock' , 1981 .
[50] D. Eichler. Energetic particle spectra in finite shocks: the earth's bow shock , 1981 .
[51] G. Gloeckler,et al. Conditions for acceleration of energetic ions ≳30 keV associated with the Earth's bow shock , 1980 .
[52] I. Papamastorakis,et al. Plasma acceleration at the Earth's magnetopause: evidence for reconnection , 1979, Nature.
[53] G. Parks,et al. Thin sheets of energetic electrons upstream from the earth's bow shock , 1979 .
[54] T. Terasawa. Origin of 30 ∼ 100 kev protons observed in the upstream region of the Earth's bow shock , 1979 .
[55] N. Sckopke,et al. Observations of two distinct populations of bow shock ions in the upstream solar wind , 1978 .
[56] S. Krimigis,et al. Simultaneous measurements of energetic protons and electrons in the distant magnetosheath, magnetotail, and upstream in the solar wind , 1978 .
[57] T. Armstrong,et al. Location of the source of magnetospheric energetic particle bursts by multispacecraft observations , 1976 .
[58] C. Meng,et al. 30- to 100-keV protons upstream from the earth's bow shock , 1974 .
[59] J. Asbridge,et al. Outward flow of protons from the Earth's bow shock , 1968 .