Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
Department of Physics, University of New Hampshire, Durham, NH 03824
Atmospheric and Environmental Research, Inc., 131 Hartwell Avenue, Lexington, MA 02421, USA
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138
Institute of Geophysics and Planetary Physics, University of California Riverside, 900 University Avenue, Room 1432 Geology Building, Riverside, CA 92521, USA of Geophysics and Planetary Physics, University of California, Riverside, Riverside, CA 92521 and Environmental Research Inc., 131 Hartwell Ave., Lexington, MA 02421, USA
Space Science Center, University of New Hampshire, Durham, NH 03824, USA
Institute of Geophysics and Planetary Physics, University of California Riverside, 900 University Ave., Room 1432, Geology Bldg., Riverside, CA 92521, USA of Geophysics and Planetary Physics, University of California, Riverside, CA 92521, USA of Geophysics and Planetary Physics, University of California Riverside, Geology Bldg., Rm. 1432, Riverside, CA 92521, USA of Geophysics and Planetary Physics, University of California, Riverside, Riverside, CA 92521, USA of New Hampshire, Space Science Center University of New Hampshire, Durham, NH 08324, USA
Space Science Center, University of New Hampshire, Morse Hall, Durham, NH 03824
Space Science Center, University of New Hampshire, Durham, NH 03824
Space Science Center, University of New Hampshire, Morse Hall, Durham, NH 03824, USA
Institute of Geophysics and Planetary Physics, University of California, Riverside, CA 92521
Institute of Geophysics and Planetary Physics, University of California, Riverside, CA 92521; Space Scien
Alfvén Waves in Shear Flows Revisited
Compound and Perpendicular Diffusion of Cosmic Rays
Compound and Perpendicular Diffusion of Cosmic Rays and Random Walk of the Field Lines. I. Parallel Particle Transport Models
Compound and Perpendicular Diffusion of Solar Energetic Particles and Field Line Random Walk
Compound and perpendicular diffusive transport of cosmic rays
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