Selected Publications

From Space Science Theory Group

Contents

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Naoki Bessho

  • Electron Acceleration and Trapping by an Oblique Shock Wave, N. Bessho and Y. Ohsawa, Phys. Plasmas 9, 979 (2002).
  • Energies of Ultrarelativistic Electrons Produced by an Oblique Shock Wave, N. Bessho and Y. Ohsawa, Phys. Plasmas 7, 4004 (2000).
  • Electron Acceleration to Ultrarelativistic Energies in a Collisionless Oblique Shock Wave, N. Bessho and Y. Ohsawa, Phys. Plasmas 6, 3076 (1999).
  • Production of Ultrarelativistic Electrons by Oblique Magnetosonic Shock Waves, N. Bessho, K. Maruyama, and Y. Ohsawa, J. Phys. Soc. Jpn. 68, 1 (1999).
  • Acceleration of Energetic Ions by Nonlinear Magnetosonic Waves, K. Maruyama, N. Bessho, and Y. Ohsawa, Phys. Plasmas 5, 3257 (1998).


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Terry G. Forbes

  • Prominence eruptions and coronal mass ejections triggered by newly emerging flux, Lin, J., T.G. Forbes, and P.A. Isenberg, J. Geophys. Res., 106 , 25053-25073, 2001.
  • The magnetic nature of solar flares, Priest, E.R. and T.G. Forbes, Astron. Astrophys. Revs., 10 , 313-377, 2002.
  • Models of three-dimensional flux ropes, Birn, J., T.G. Forbes, and K. Schindler, Astrophys. J ., 588, 578-585, 2003.
  • A three-dimensional flux rope model for coronal mass ejections based on a loss of equilibrium, Roussev, I.I., T.G. Forbes, T.I. Gombosi, I.V. Sokolov, D.L De Zeeuw, and J. Birn, Astrophys. J., 588 , L45-48, 2003.
  • Observational evidence of new current sheets trailing coronal mass ejections, Webb, D.F., J. Burkepile, T.G. Forbes, and P. Riley, J. Geophys. Res ., 108(A12), 1440, doi: 10.1029/2003JA009923, 2003.


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Joseph Hollweg

  • 2004: Intermittent heating of the solar corona by heat flux-generated ion cyclotron waves, Markovskii, S.A., and J.V. Hollweg, Astrophys. J., 609, 1112.
  • 2004: Cross-field energy transfer of a body Alfvén wave propagating along and across a pressure-balanced structure, Vasquez, B.J., and J.V. Hollweg, Geophys. Res. Lett., in press.
  • 2004, Deceleration of relative streaming between proton components among nonlinear low-frequency Alfvén waves, Kaghashvili, E., B.J. Vasquez, G.P. Zank, and J.V. Hollweg, J. Geophys. Res., submitted.
  • Coronal loop oscillations: Calculation of resonantly damped MHD quasi-mode kink oscillations of longitudinally stratified loops, Andries, J., M. Goossens, J.V. Hollweg, I. Arregui, and T. Van Doorsselaere, Astron. Astrophys., submitted, 2005.
  • 2005, The solar wind then and now, Hollweg, J.V., Phil. Trans. Royal Society, submitted.


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Philip Isenberg

  • Heating of coronal holes and generation of the solar wind by ion-cyclotron resonance, Isenberg, P.A., Space Sci. Rev., 95, 119, 2001.
  • Generation of the fast solar wind: A review with emphasis on the resonant cyclotron interaction, Hollweg, J.V., and P.A. Isenberg, J. Geophys. Res., 107(A7), 1147, doi:10.1029/2001JA000270, 2002.
  • Turbulent heating of the distant solar wind by interstellar pickup protons, Isenberg, P.A., C.W. Smith, and W.H. Matthaeus, Astrophys. J., 592, 564, 2003.
  • The kinetic shell model of coronal heating and acceleration by ion cyclotron waves. 3. The proton halo and dispersive waves, Isenberg, P.A., J. Geophys. Res., 109(A3), 3101, doi: 10.1029/2002JA009449, 2004.
  • Turbulence-driven solar wind heating and energization of pickup protons in the outer heliosphere, Isenberg, P. A., Astrophys. J., 623, 502, 2005.
  • Preferential perpendicular heating of coronal hole minor ions by the Fermi mechanism, Isenberg, P. A., and B. J. Vasquez, Astrophys. J., in press, 2007.


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Martin A. Lee

  • On the effect of directional medium scale interplanetary variations on the diffusion of galactic cosmic rays and their solar cycle variation, Morfill, G.E., H.J. Völk, and M.A. Lee, J. Geophys. Res., 81 , 5841, 1976.
  • Modulation of solar flare particles and track density profiles in gas-rich meteorite grains, Lee, M.A., J. Geophys. Res., 81 , 3207, 1976.
  • Simple analytic solutions appropriate for galactic cosmic ray modulation, Cowsik, R., and M.A. Lee, Astrophys. J., 216 , 635, 1977.
  • Simple analytical solutions for spherically-symmetric production and modulation of energetic solar particles, Gross, M., M.A. Lee, and I. Lerche, Astrophys. J ., 218 , 552, 1977.
  • Simple analytic solutions appropriate for galactic cosmic ray modulation, Cowsik, R., and M.A. Lee, Proc. 15th Inter. Conf. Cosmic Rays , 3 , 18, 1977.


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Yuri Litvinenko

  • Relativistic Acceleration of Protons in Reconnecting Current Sheets of Solar Flares,Y. E. Litvinenko, and B. V. Somov, Solar Physics, 158 (2), 317, 1995.
  • Particle Acceleration in Reconnecting Current Sheets with a Nonzero Magnetic Field, Y. E. Litvinenko, Astrophysical Journal, 462 (2), 997, 1996.
  • Photospheric Magnetic Reconnection and Canceling Magnetic Features on the Sun, Y. E. Litvinenko, Astrophysical Journal, 515 (1), 435, 1999.
  • Flare Energy Release by Flux Pile-Up Magnetic Reconnection in a Turbulent Current Sheet, Y. E. Litvinenko, and I. J. D. Craig, Astrophysical Journal, 544 (2), 1101, 2000.
  • Energy Balance in the Corona Over the 22-Year Solar Cycle, Y. E. Litvinenko, and M. S. Wheatland, Solar Physics, 219 (2), 265, 2004.


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Chung Sang Ng

  • 2004 Complete Spectrum of Kinetic Eigenmodes for Plasma Oscillations in a Weakly Collisional Plasma, C. S. Ng, A. Bhattacharjee, and F. Skiff, Phys. Rev. Lett,92, 065 002, 2004.
  • 2003 Anisotropic Fluid Turbulence in the Interstellar Medium and the Solar Wind, C. S. Ng, A. Bhattacharjee, K. Germaschewski, and S. Galtier, Phys. Plasma, 10, 1954, 2003.
  • 1999 Kinetic Eigenmodes and Discrete Spectrum of Plasma Oscillations in a Weakly Collisional Plasma, C. S. Ng, A. Bhattacharjee, and F. Skiff, Phys. Rev. Lett., 83, 1974, 1999.
  • 1999 Ginzburg-Landau Model and Single-Mode Operation of a Free-Electron Laser Oscillator, C. S. Ng and A. Bhattacharjee, Phys. Rev. Lett., 82, 2665, 1999.
  • 1998 Non-Equilibrium and Current Sheet Formation in Line-Tied magnetic Fields, C. S. Ng and A. Bhattacharjee, Phys. Plasma, 5, 4028, 1998.


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John Podesta

  • Relationship between the shell-averaged energy spectrum and the frequency spectrum measured by a single spacecraft in the solar wind, Podesta, J. J., Astrophys. J., (submitted) 2008.
  • Laws for third-order moments in homogeneous, anisotropic, incompressible magnetohydrodynamic turbulence, Podesta, J. J., J. Fluid Mech., (submitted) 2007.
  • Anisotropic form of third-order moments and relationship to the cascade rate in axisymmetric magnetohydrodynamic turbulence, Podesta, J. J., M. A. Forman, C. W. Smith, Phys. of Plasmas, (in press) 2007.
  • Angle between velocity and magnetic field fluctuations in solar wind turbulence, Podesta, J. J., D. A. Roberts, M. L. Goldstein, B. Chandran, and A. Bhattacharjee, J. Geophys. Res., (submitted) 2007.
  • Spectral Exponents of Kinetic and Magnetic Energy Spectra in Solar Wind Turbulence, Podesta, J. J., D. A. Roberts, and M. L. Goldstein, Astrophys. J., 664, 543-548, 2007.
  • Mode decomposition scheme for ideal magnetohydrodynamic planewaves in space-time coordinates, Podesta, J. J., M. L. Goldstein, and D. A. Roberts, J. Geophys. Res., 112, A06103, doi:10.1029/2006JA012097, 2007.
  • Self-similar stochastic processes in solar wind turbulence, Adv. Space Res., Podesta, J. J., to appear: Proceedings 2006 COSPAR Assembly, Beijing, 2006.
  • Self-similar scaling of kinetic energy density in the inertial range of solar wind turbulence, Podesta, J. J., J. Geophys. Res., (in press) 2007.
  • Self-similar scaling of magnetic energy in the inertial range of solar wind turbulence, Podesta, J. J., D. A. Roberts, and M. L. Goldstein, J. Geophys. Res., 111, A09105, doi:10.1029/2006JA011766, 2006.
  • Power spectrum of small-scale turbulent velocity fluctuations in the solar wind, Podesta, J. J., D. A. Roberts, and M. L. Goldstein, J. Geophys. Res., 111, A10109, doi:10.1029/2006JA011834, 2006.
  • Empirical analysis of the radial momentum balance of the solar wind in the ecliptic plane between 0.3 and 1 AU, Podesta, J. J., J. Geophys. Res. (in preparation), 2008.
  • Radial decay law for large-scale velocity and magnetic field fluctuations in the solar wind, Podesta, J. J., J. Geophys. Res., 111, A08103, doi:10.1029/2005JA011528, 2006.


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Jimmy Raeder


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Brian Sullivan

  • Extension of the electron dissipation region in collisionless Hall MHD Reconnection, B. P. Sullivan, and A. Bhattacharjee, submitted to Phys. Plas., May 2009.

† © 2008 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.These articles appeared in Physics of Plasmas and may be found at: Physics of Plasmas


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Bernard Vasquez

  • A wave-model interpretation of the evolution of rotational discontinuities, Vasquez, B. J., and P. J. Cargill, J. Geophys. Res., 98, 1277, 1993.
  • Simulation study of the role of ion kinetics in low-frequency wave train evolution, Vasquez, B. J., J. Geophys. Res., 100, 1779, 1995.
  • Formation of arc-shaped Alfv´en waves from oblique linearly polarized wave trains, Vasquez, B. J., and J. V. Hollweg, J. Geophys. Res., 101, 13,527, 1996.
  • Nonlinear evolution of Alfvén waves and RDs-Hybrid simulations, Vasquez, B. J., and J. V. Hollweg, Solar Wind Nine, edited by Shadia Habbal et al., AIP Conf. Proc., 167, 1999.
  • Cross-Field Energy Transfer of a Body Alfv´en Wave Propagating Along and Across a Pressure-Balanced Structure, Vasquez, B. J., and J. V. Hollweg, Geophys. Res. Lett., 31, doi:10.1029/2004GL019746, 2004.
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