collaborators

6 papers

astro-ph.SR2026

Intermittent turbulent fluctuations in solar coronal mass ejections

Apurva Bhagat, Sumit Tambe, Debesh Bhattacharjee +1

Localised regions of high intensity fluctuations are known to be signatures of intermittency in fluid and plasma turbulence. We investigate such turbulent spots using near-Earth {\…

gr-qc2026

Open Data from LIGO, Virgo, and KAGRA through the Second Part of the Fourth Observing Run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1809

LIGO, Virgo, KAGRA, and GEO 600 form a network of gravitational-wave observatories. Data and analysis results from this network are made publicly available through the Gravitationa…

astro-ph.SR2025

Energy-Containing Electrons in Solar Flares: Improving Hard X-Ray and EUV Diagnostics

Yingjie Luo, Eduard P. Kontar, Debesh Bhattacharjee

Solar flares effectively accelerate particles to non-thermal energies. These accelerated electrons are responsible for energy transport and subsequent emissions in HXR, radio, and…

astro-ph.SR2025

Total Power and Low-energy Cut-off Time Evolution of Solar Flare Accelerated Electrons Using X-Ray Observations and Warm-Target Model

Debesh Bhattacharjee, Eduard P. Kontar, Yingjie Luo

A primary characteristic of solar flares is the efficient acceleration of electrons to nonthermal deka-keV energies. While hard X-Ray (HXR) observation of bremsstrahlung emission s…

astro-ph.SR2025

Proton heating estimates from near-Earth observations of coronal mass ejections in solar cycle 24

Debesh Bhattacharjee, Prasad Subramanian, Saikat majumder +1

As solar coronal mass ejections (CMEs) propagate through the heliosphere, they expend energy in heating protons to compensate for the cooling that occurs due to expansion. CME prop…

astro-ph.HE2025

Spectroscopy of Supernova Remnants and Candidates in M31

Nelson Caldwell, John C. Raymond, Knox S. Long +1

With a star formation rate of order 0.4 M yr, M31 should have significant population of supernova remnants (SNRs), and, in fact, 156 SNR and SNR candidates have bee…