activity
20172023
most citedModeling Shocks Detected by Voyager 1 in the Local Interstellar Medium

56 citations · 226 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2023★ 44 cited

Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R

Samuel T. Badman, Pete Riley, Shaela I. Jones +11

Drawing connections between heliospheric spacecraft and solar wind sources is a vital step in understanding the evolution of the solar corona into the solar wind and contextualizin…

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★ 43 cited

Turbulence in the outer heliosphere

Federico Fraternale, Laxman Adhikari, Horst Fichtner +9

The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their interaction is governed by complex physical processes and creates heliospheric regions with sign…

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…

physics.space-ph2020★ 23 cited

Application of a Modified Spheromak Model to Simulations of Coronal Mass Ejection in the Inner Heliosphere

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

The magnetic fields of interplanetary coronal mass ejections (ICMEs), which originate close to the Sun in the form of a flux rope, determine their geoeffectiveness. Therefore, robu…

physics.space-ph2019★ 23 cited

Predicting the Solar Wind at Parker Solar Probe Using an Empirically Driven MHD Model

T. K. Kim, N. V. Pogorelov, C. N. Arge +20

Since the launch on 2018/08/12, Parker Solar Probe (PSP) has completed its first and second orbits around the Sun, having reached down to 35.7 solar radii at each perihelion. In an…

physics.space-ph2017★ 56 cited

Modeling Shocks Detected by Voyager 1 in the Local Interstellar Medium

Tae K. Kim, Nikolai V. Pogorelov, Leonard F. Burlaga

The magnetometer (MAG) on Voyager 1 (V1) has been sampling the interstellar magnetic field (ISMF) since August 2012. The V1 MAG observations have shown draped ISMF in the very loca…