activity
20222026
most citedSWASTi-SW: Space Weather Adaptive SimulaTion framework for Solar Wind and its relevance to ADITYA-L1 mission

26 citations · 28 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2026

Fast and Differentiable MHD Surrogate for Solar Wind using Neural Operator

Prateek Mayank, Enrico Camporeale, Thomas E. Berger +2

Global magnetohydrodynamic (MHD) simulations provide the complete plasma state of the heliosphere, but their computational cost limits applications requiring repeated model evaluat…

astro-ph.SR2026

Finding Novel Precursors for Solar Wind Stream Interaction Regions with Interpretable Deep Learning

Prateek Mayank, Yogesh, Enrico Camporeale +4

Solar wind stream interaction regions (SIRs) drive recurrent geomagnetic storms, yet most existing catalogs rely on expert inspection and simple thresholds that are subjective and…

astro-ph.SR2025

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…

physics.space-ph2024

Simulating the Arrival of Multiple Coronal Mass Ejections that Triggered the Gannon Superstorm on May 10, 2024

Smitha V. Thampi, Ankush Bhaskar, Prateek Mayank +2

The May 10, 2024 space weather event stands out as the most powerful storm recorded during the current solar cycle. This study employs a numerical framework utilizing a semi-empiri…

astro-ph.SR2024

Study of Evolution and Geo-effectiveness of CME-CME Interactions using MHD Simulations with SWASTi framework

Prateek Mayank, Stefan Lotz, Bhargav Vaidya +2

The geo-effectiveness of Coronal Mass Ejections (CMEs) is a critical area of study in space weather, particularly in the lesser-explored domain of CME-CME interactions and their ge…

astro-ph.SR2024★ 2 cited

Using sunRunner3D to interpret the global structure of the heliosphere from in situ measurements

José Juan González-Avilés, Pete Riley, Michal Ben-Nun +2

Understanding the large-scale three-dimensional structure of the inner heliosphere, while important in its own right, is crucial for space weather applications, such as forecasting…

astro-ph.SR2023

Solar Flare Prediction and Feature Selection using Light Gradient Boosting Machine Algorithm

Vysakh P. A., Prateek Mayank

Solar flares are among the most severe space weather phenomena, and they have the capacity to generate radiation storms and radio disruptions on Earth. The accurate prediction of s…

astro-ph.SR2023

SWASTi-CME: A physics-based model to study CME evolution and its interaction with Solar Wind

Prateek Mayank, Bhargav Vaidya, Wageesh Mishra +1

Coronal mass ejections (CMEs) are primary drivers of space weather and studying their evolution in the inner heliosphere is vital to prepare for a timely response. Solar wind strea…

astro-ph.SR2022★ 26 cited

SWASTi-SW: Space Weather Adaptive SimulaTion framework for Solar Wind and its relevance to ADITYA-L1 mission

Prateek Mayank, Bhargav Vaidya, D. Chakrabarty

Solar wind streams, acting as background, govern the propagation of space weather drivers in the heliosphere, which induce geomagnetic storm activities. Therefore, predictions of t…