Member Since 2017
Riddhi Bandyopadhyay
Associate Research Scholar, Princeton University
AGU Research
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Characterizing Turbulence in the Inner Solar Corona, Transition Region, and Chromosphere From Total Solar Eclipse Observations
SOLAR ECLIPSE SCIENCE: WHAT WE LEARNED FROM THE GREAT AMERICAN ECLIPSES AND WHAT IS NEXT I POSTER
spa-solar and heliospheric physics | 13 december 2024
Zac Bailey, Shadia R. Habbal, Riddhi Bandyopadhyay...
Spectroscopic imaging of the corona during total solar eclipses in 1860s revealed the presence of unknown elements, associating them almost 70 years l...
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Pressure-Strain Interaction in a Magnetotail Reconnection Region
MAGNETIC RECONNECTION: CONNECTING IDEAS FROM OBSERVATIONS, EXPERIMENTS, MODELS, AND THEORY II ORAL
spa-magnetospheric physics | 13 december 2024
James L. Burch, Kevin J. Genestreti, Steven V. Heu...
The NASA Magnetospheric Multiscale (MMS) mission explores the boundary regions of the Earth's magnetosphere with high-accuracy measurements of charged...
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Unravelling the link between turbulence, intermittency, and dissipation in the terrestrial magnetosheath
MULTISCALE DYNAMICS IN MAGNETIZED TURBULENCE II ORAL
spa-solar and heliospheric physics | 13 december 2024
Alexandros Chasapis, Yi Qi, NEHA PATHAK, Narges Ah...
Turbulence is an inherently multiscale phenomenon. It is characterized by cross-scale energy transfer, along with the formation of intermittent struct...
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Chaotic fluctuations in Turbulent Plasma
GEOPHYSICAL FLUID DYNAMICS I ORAL
nonlinear geophysics | 12 december 2024
Riddhi Bandyopadhyay, Nicholas V. Sarlis, James M....
Most space and astrophysical plasmas are considered to be in turbulent state, often characterized by stochastic fluctuations. Many laboratory experime...
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Correlation between the Upstream Diffusion Coefficient and a Shock’s Peak Energetic Particle Intensity
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA VI POSTER
spa-solar and heliospheric physics | 11 december 2024
Manuel E. Cuesta, Riddhi Bandyopadhyay, Federico F...
There is an abundance of studies that investigate the spatial diffusion coefficient (κ) via simulations and in-situ solar wind observations. However, ...
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Asymmetric Tangential Velocity inside Switchbacks
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA V POSTER
spa-solar and heliospheric physics | 11 december 2024
Juston Ward, Riddhi Bandyopadhyay, David J. McComa...
The Parker Solar Probe (PSP) has provided observations of magnetic switchbacks over progressively closer perihelia, since its launch in 2018. These sw...
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The Alfven transition zone observed by the Parker Solar Probe in young solar wind – global properties and model comparisons
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA V POSTER
spa-solar and heliospheric physics | 11 december 2024
Rohit Chhiber, Francesco Pecora, Arcadi V. Usmanov...
The transition from subAlfvénic to superAlfvénic flow in the solar atmosphere is examined by means of Parker Solar Probe (PSP) measurements during sol...
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Observed Fluctuation Enhancement and Departure from WKB Theory in Sub-Alfv\'enic Solar Wind
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA V POSTER
spa-solar and heliospheric physics | 11 december 2024
William H. Matthaeus, David J. Ruffolo, Panisara T...
We examine fluctuation amplitudes throughout the critical region where the solar wind flow speed approaches and then exceeds the Alfv\'en wave speed u...
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