Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Space Science Center, Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, New Hampshire, USA
Physics Department and Space Science Center, Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, NH 03824, USA
Delaware University
Physics Department, Space Science Center, University of New Hampshire, Durham, NH, USA
Space Science Center, Morse Hall, University of New Hampshire, Durham, New Hampshire, USA
Space Science Center, University of New Hampshire, Durham, New Hampshire, USA
Bartol Research Institute, Newark, DE
Institute of Earth, Oceans and Space, University of New Hampshire, Durham, New Hampshire, USA
Delaware Univ., Newark.
University of Delaware, Newark, DE, US
Southwest Research Institute, San Antonio, TX, US
Delaware, Univ., Newark
Physics Department, Space Science Center, Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, NH 03824
Space Science Center, University of New Hampshire, Durham, NH 03824 for Earth, Oceans and Space, University of New Hampshire, Durham, NH 03824
Bartol Research Institute, University of Delaware, Newark
Bartol Research Institute, University of Delaware, Newark, Delaware, USA
Space Science Center, University of New Hampshire, Durham, NH 03824 Research Institute, University of Delaware, Newark, Delaware
Physics Department, Space Science Center, Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, NH 03824, USA
Physics Department and Space Science Center Institute for the Study of Earth, Oceans, and Space University of New Hampshire Durham, New Hampshire, USA
Physics Department and Space Science Center, U
A slow mode transition region adjoining the front boundary of a magnetic cloud as a relic of a convected solar wind feature: Observations and MHD simulation
A Two-component Transport Model for Solar Wind Fluctuations: Waves plus Quasi-2D Turbulence
Anisotropies and helicities in the solar wind inertial and dissipation ranges at 1 AU
Anisotropy of shock-accelerated ion distributions in interplanetary space
Considerations limiting cyclotron-resonant damping of cascading interplanetary turbulence and why the `slab' approximation fails
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