97 citations · 900 across the 40 of their papers we have counts for
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Observation of Inertial-range Energy Cascade within a Reconnection Jet in Earth's Magnetotail
Riddhi Bandyopadhyay, Alexandros Chasapis, D. J. Gershman +6
Earth's magnetotail region provides a unique environment to study plasma turbulence. We investigate the turbulence developed in an exhaust produced by magnetic reconnection at the…
Direct Measurement of the Solar-Wind Taylor Microscale using MMS Turbulence Campaign Data
Riddhi Bandyopadhyay, William H. Matthaeus, Alexandros Chasapis +7
Using the novel Magnetospheric Multiscale (MMS) mission data accumulated during the 2019 MMS Solar Wind Turbulence Campaign, we calculate the Taylor microscale o…
Interplay of Turbulence and Proton-Microinstability Growth in Space Plasmas
Riddhi Bandyopadhyay, Ramiz A. Qudsi, William H. Matthaeus +13
Numerous prior studies have shown that as proton beta increases, a narrower range of proton temperature anisotropy values is observed. This effect has often been ascribed to the ac…
The Temperature Anisotropy and Helium Abundance Features of Alfvénic Slow Solar Wind Observed by Parker Solar Probe, Helios, and Wind Missions
Jia Huang, Davin E. Larson, Tamar Ervin +20
Slow solar wind is typically characterized as having low Alfvénicity, but the occasional occurrence of highly Alfvénic slow solar wind (HASSW) raises questions about its source reg…
Intermittency and Ion Temperature-Anisotropy Instabilities: Simulation and Magnetosheath Observation
Ramiz A. Qudsi, Riddhi Bandyopadhyay, Bennett A. Maruca +11
Weakly collisional space plasmas are rarely in local thermal equilibrium and often exhibit non-Maxwellian electron and ion velocity distributions that lead to the growth of microin…
Inner-Heliosphere Signatures of Ion-Scale Dissipation and Nonlinear Interaction
Trevor A. Bowen, Alfred Mallet, Stuart D. Bale +19
We perform a statistical study of the turbulent power spectrum at inertial and kinetic scales observed during the first perihelion encounter of Parker Solar Probe. We find that oft…