22 citations · 25 across the 9 of their papers we have counts for
10 papers
Elemental Composition Evolution during the 2024 September 30 Solar Eruption: A Comparison of Hot and Cool Plasma Components with Solar Orbiter/SPICE, Hinode/EIS, and Chandrayaan-2/XSM
Momchil Molnar, Joseph Plowman, Amir Caspi +7
Solar plasma composition differs between the photosphere and corona over a range of timescales, with preferential enhancement of elements with low first ionization potential (FIP).…
Neural Enhancement of the Traditional Wang-Sheeley-Arge Solar Wind Relation
Prateek Mayank, Enrico Camporeale, Arpit K. Shrivastav +2
The Wang-Sheeley-Arge (WSA) model has been the cornerstone of operational solar wind forecasting for nearly two decades, owing to its simplicity and physics-based formalism. Howeve…
Co-existence of longitudinal and transverse oscillations in polar plumes observed with Solar Orbiter/EUI
Upasna Baweja, Vaibhav Pant, S. Krishna Prasad +6
Magnetohydrodynamic (MHD) waves play a key role in heating the solar corona and driving the solar wind. Recent observations have shown the presence of slow magneto-acoustic and Alf…
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…
On the Existence of Long-Period Decayless Oscillations in Short Active Region Loops
Arpit Kumar Shrivastav, Vaibhav Pant, Rohan Kumar +5
Decayless kink oscillations, characterized by their lack of decay in amplitude, have been detected in coronal loops of varying scales in active regions, quiet Sun and coronal holes…
Exploring the magnetic and thermal evolution of a coronal jet
Sushree S Nayak, Samrat Sen, Arpit Kumar Shrivastav +2
Coronal jets are the captivating eruptions which are often found in the solar atmosphere, and primarily formed due to magnetic reconnection. Despite their short-lived nature and lo…
On the Effect of Coronal Rain on Decayless Kink Oscillations of Coronal Loops
Arpit Kumar Shrivastav, Vaibhav Pant, Patrick Antolin
Decayless kink oscillations are ubiquitously observed in active region coronal loops with an almost constant amplitude for several cycles. Decayless kink oscillations of coronal lo…
SITCoM: SiRGraF Integrated Tool for Coronal dynaMics
Purvi Udhwani, Arpit Kumar Shrivastav, Ritesh Patel
SiRGraF Integrated Tool for Coronal dynaMics (SITCoM) is based on Simple Radial Gradient Filter (SiRGraF) used to filter the radial gradient in the white-light coronagraph images a…
A Statistical Investigation of Decayless Oscillations in Small-scale Coronal Loops Observed by Solar Orbiter/EUI
Arpit Kumar Shrivastav, Vaibhav Pant, David Berghmans +6
Decayless kink oscillations are omnipresent in the solar atmosphere and a viable candidate for coronal heating. Though there have been extensive studies of decayless oscillations i…
Characterizing Spectral Channels of Visible Emission Line Coronagraph of Aditya-L1
Ritesh Patel, Megha A., Arpit Kumar Shrivastav +4
Aditya-L1 is India's first solar mission with Visible Emission Line Coronagraph (VELC) consisting of three spectral channels taking high-resolution spectroscopic observations of th…