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Sandeep Kumar

4 papers hereh-index 318 citations10 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.EP1
same name
  • Sandeep Kumar — 8 papers, h 2
  • Sandeep Kumar — 4 papers, h 2
  • Sandeep Kumar — 3 papers, h 0
  • Sandeep Kumar — 3 papers, h 5
  • Sandeep Kumar — 3 papers, h 1
  • Sandeep Kumar — 2 papers, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20242026
collaborators

4 papers

astro-ph.SR2026

Source Surface Height Optimisation for Improved Solar Wind Velocity Forecasting Across Solar Cycles 23, 24 and 25

Sandeep Kumar, Nandita Srivastava, Dana-Camelia Talpeanu

The potential field source surface (PFSS) model is a cornerstone of many state-of-the-art space weather forecasting frameworks. It includes a single physical free parameter, the so…

astro-ph.SR2026

Propagation Characteristics of the April 21, 2023 CME

Sandeep Kumar, Nandita Srivastava, Parthib Banerjee +1

Accurate estimation of propagation characteristics of coronal mass ejections (CMEs) is crucial for predicting their geoeffectiveness. Stereoscopic techniques to study the kinematic…

astro-ph.EP2025

Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution

Daniele Viganò, Soumya Sengupta, Clà udia Soriano-Guerrero +4

The inflated radii observed in hundreds of hot Jupiters (HJ) represent a long-standing open issue. In this study, we quantitatively investigate this phenomenon within the framework…

astro-ph.SR2024

On The Influence Of The Solar Wind On The Propagation Of Earth-impacting Coronal Mass Ejections

Sandeep Kumar, Nandita Srivastava, Nat Gopalswamy +1

Coronal Mass Ejections (CMEs) are subject to changes in their direction of propagation, tilt, and other properties as they interact with the variable solar wind. We investigated th…

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