Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Laboratory for Solar and Space Physics, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
NASA Goddard Space Flight Center, Laboratory for Solar and Space Physics Code 612.2, Greenbelt, MD 20771, USA
ISR Division, Los Alamos National Laboratory, Los Alamos, NM, USA;
Courant Institute of Mathematical Sciences, New York University
Los Alamos National Laboratory, Los Alamos, NM, 87545, USA
Los Alamos National Laboratory, Los Alamos, New Mexico, USA
NASA Goddard Space Flight Center, Laboratory for Solar and Space Physics, Code 612.2, Greenbelt, MD 20771, USA
Los Alamos National Laboratory, Los Alamos, NM 87545, USA
NASA Goddard Space Flight Center, Laboratory for Solar and Space Physics, Code 612.2, Greenbelt, MD 20771, USA Goddard Space Flight Center, Laboratory for Geospace Physics, Heliosphysics Science Division, Greenbelt, MD 20771
Los Alamos National Laboratory Space Science and Applications Los Alamos, New Mexico, 87545, USA
University of New Hampshire, Physics Department, EOS / SSC, Durham, NH 03824, USA Science Center, University of New Hampshire, Durham, NH 03824, USA
Space Science Center, University of New Hampshire, Durham, New Hampshire, USA
Center for Integrated Computation and Analysis of Reconnection and Turbulence, University of New Hampshire, Durham, NH 03824, USA Alamos National Laboratory, Los Alamos, New Mexico, 87545
Los Alamos National Laboratory, Los Alamos, New Mexico, 87544
Courant Institute of MathematiSciences, New York University, New York, NY 10012, USA Alamos National Laboratory, Los Alamos, NM, USA
NASA Goddard Space Flight Center, Laboratory for Solar and Space Physics Code 61
A Kinetic Alfven wave cascade subject to collisionless damping cannot reach electron scales in the solar wind at 1 AU
Accurate estimation of third-order moments from turbulence measurements
Aspects of the theory of incompressible MHD turbulence with cross-helicity and applications to the solar wind
Boundary Conditions for Alfven Waves in the Solar Corona
Comment on ``Turbulent Cascade at 1 AU in High Cross-Helicity Flows''
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