activity
20152025
most citedKinematics of Interacting CMEs of September 25 and 28, 2012

32 citations · 224 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2025

Pivot of the Emerging Bipolar Magnetic Region in the Birth of Sigmoidal Solar Active Regions

Ronald L. Moore, Sanjiv K. Tiwari, V. Aparna +3

We present an augmentation to longstanding evidence from observations and MHD modeling that (1) every solar emerging bipolar magnetic region (BMR) is made by an emerging omega-loop…

astro-ph.SR2025

Magnetohydrodynamic Simulation of a Coronal Mass Ejection Observed During the Near-radial Alignment of Solar Orbiter and Earth

Talwinder Singh, Dinesha V. Hegde, Tae K. Kim +1

Interplanetary Coronal Mass Ejections (ICMEs) are the primary sources of geomagnetic storms at Earth. Negative out-of-ecliptic component (Bz) of magnetic field in the ICME or its a…

astro-ph.SR2023★ 2 cited

CME Propagation Through the Heliosphere: Status and Future of Observations and Model Development

M. Temmer, C. Scolini, I. G. Richardson +31

The ISWAT clusters H1+H2 have a focus on interplanetary space and its characteristics, especially on the large-scale co-rotating and transient structures impacting Earth. SIRs, gen…

physics.space-ph2023★ 15 cited

Improving the Arrival Time Estimates of Coronal Mass Ejections by Using Magnetohydrodynamic Ensemble Modeling, Heliospheric Imager data, and Machine Learning

Talwinder Singh, Bernard Benson, Syed A. Z. Raza +4

The arrival time prediction of Coronal mass ejections (CMEs) is an area of active research. Many methods with varying levels of complexity have been developed to predict CME arriva…

physics.space-ph2022★ 22 cited

Ensemble simulations of the 12 July 2012 Coronal Mass Ejection with the Constant Turn Flux Rope Model

Talwinder Singh, Tae K. Kim, Nikolai V. Pogorelov +1

Flux-rope-based magnetohydrodynamic modeling of coronal mass ejections (CMEs) is a promising tool for the prediction of the CME arrival time and magnetic field at Earth. In this wo…

astro-ph.SR2020★ 6 cited

The Missing Cool Corona in the Flat Magnetic Field around Solar Active Regions

Talwinder Singh, Alphonse C. Sterling, Ronald L. Moore

SDO/AIA images the full solar disk in several EUV bands that are each sensitive to coronal plasma emissions of one or more specific temperatures. We observe that when isolated acti…