activity
20242026
collaborators

8 papers

astro-ph.SR2026

Energy and mass transport associated with impulsive spicular flows in solar coronal holes

Lei Ni, Jun Lin, Tanmoy Samanta +3

How the solar atmosphere is heated from a temperature of about \,K in the lower atmosphere to about \,MK in the corona has challenged the astrophysical community…

astro-ph.SR2026

On the Origin of Coronal Picoflare Jets

Annu Bura, Daniel Nóbrega-Siverio, Tanmoy Samanta +1

Small-scale jet-like eruptions, such as picoflare jets and jetlets, are recognized as potential contributors to coronal heating and solar wind acceleration, yet their physical orig…

astro-ph.SR2026

Probing the CME Core--Prominence Relation Using Inner Coronal Observations

Sunit Sundar Pradhan, Jayant Joshi, Tanmoy Samanta

Coronal mass ejections (CMEs) often exhibit a three-part structure consisting of a bright inner core, an outer leading edge, and an intervening dark cavity. While the core has trad…

astro-ph.SR2025

Dynamics of Reconnection Nanojets in Eruptive and Confined Solar Flares

Annu Bura, Arpit Kumar Shrivastav, Ritesh Patel +6

Recent observations reveal small-scale reconnection-driven plasma ejections, often termed nanojets, triggered by magnetic field interactions at slight misalignment angles. These fa…

astro-ph.SR2025

Formation of chromospheric fan-shaped jets through magnetic reconnection

Annu Bura, Tanmoy Samanta, Avijeet Prasad +4

Recurrent chromospheric fan-shaped jets highlight the highly dynamic nature of the solar atmosphere. They have been named as ''light walls'' or ''peacock jets'' in high-resolution…

astro-ph.SR2025

The Detectability of Coronal Mass Ejections in the Low Corona Using Multi-slit Extreme-ultraviolet Spectroscopy

Lami Chan, Xianyong Bai, Hui Tian +6

The spectra of coronal mass ejections (CMEs) in the low corona play a crucial role in understanding their origins and physical mechanism, and enhancing space weather forecasting. H…