activity
20082025
most citedSolar X-ray Monitor On Board the Chandrayaan-2 Orbiter: In-flight Performance and Science Prospects

40 citations · 246 across the 24 of their papers we have counts for

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Showing astro-ph.SRShow all

18 papers · 1 filter

astro-ph.SR2025★ 3 cited

Evidence for in situ particle energization during the May-2024 event based on ASPEX instrument on board Aditya-L1

Shivam Parashar, Dibyendu Chakrabarty, Prashant Kumar +26

The interaction between interplanetary Coronal Mass Ejection (ICME) structures can alter the geo-effectiveness of the ICME events in myriad ways. Many aspects of these interaction…

astro-ph.SR2025

One year of ASPEX-SWIS operation -- Characteristic features, observations and science potential

Abhishek Kumar, Shivam Parashar, Prashant Kumar +26

The Aditya-L1 mission, India's first dedicated solar observatory positioned at the first Lagrange point (L1) of the Sun-Earth system, carries the Solar Wind Ion Spectrometer (SWIS)…

astro-ph.SR2025

Wave Particle Interaction in the Upstream of ICME Shocks

Shanwlee Sow Mondal, Aveek Sarkar, Sofiane Bourouaine

Shocks associated with Interplanetary Coronal Mass Ejections are known to energize charged particles and give rise to Solar Energetic Particles. Many of these energetic particles m…

astro-ph.SR2023

Suprathermal population associated with stream interaction regions observed by STEREO-A: New insights

Bijoy Dalal, Dibyendu Chakrabarty, Nandita Srivastava +1

Stream interaction regions (SIRs) are often thought to be responsible for the generation of suprathermal population in the interplanetary medium. Despite the source being same, wid…

astro-ph.SR2023★ 14 cited

Role of small-scale impulsive events in heating the X-ray bright points of the quiet Sun

Biswajit Mondal, James A Klimchuk, Santosh V. Vadawale +6

Small-scale impulsive events, known as nanoflares, are thought to be one of the prime candidates that can keep the solar corona hot at its multi-million Kelvin temperature. Individ…

astro-ph.SR2023

Evolution of elemental abundances in hot active region cores from Chandrayaan-2 XSM observations

Biswajit Mondal, Santosh V. Vadawale, Giulio Del Zanna +5

The First Ionization Potential (FIP) bias, whereby elemental abundances for low FIP elements in different coronal structures vary from their photospheric values and may also vary w…