Publications of Talwinder Singh ordered by citations


A list of publications authored or co-authored by Talwinder Singh, derived from the SAO/NASA Astrophysics Data System (ADS) and ordered by the numbers of citations.

Orcid ID: 0000-0002-0213-6038

Number of papers: 17
No. of citations: 224

35 A Data-constrained Model for Coronal Mass Ejections Using the Graduated Cylindrical Shell Method
Singh, T., Yalim, M. S. & Pogorelov, N. V., 2018, ApJ, 864, 18
27 Kinematics of interacting CMEs of 25 and 28 September 2012
Mishra, Wageesh, Srivastava, Nandita & Singh, Talwinder, 2015, Journal of Geophysical Research (Space Physics), 120, 10,221
24 Ensemble Simulations of the 2012 July 12 Coronal Mass Ejection with the Constant-turn Flux Rope Model
Singh, Talwinder, Kim, Tae K., Pogorelov, Nikolai V. & Arge, Charles N., 2022, ApJ, 933, 123
24 Active Longitude and Coronal Mass Ejection Occurrences
Gyenge, N., Singh, T., Kiss, T. S., Srivastava, A. K. & Erdélyi, R., 2017, ApJ, 838, 18
24 Evolution of Magnetic Rayleigh-Taylor Instability into the Outer Solar Corona and Low Interplanetary Space
Mishra, Sudheer K., Singh, Talwinder, Kayshap, P. & Srivastava, A. K., 2018, ApJ, 856, 86
22 A Modified Spheromak Model Suitable for Coronal Mass Ejection Simulations
Singh, Talwinder, Yalim, Mehmet S., Pogorelov, Nikolai V. & Gopalswamy, Nat, 2020, ApJ, 894, 49
17 Application of a Modified Spheromak Model to Simulations of Coronal Mass Ejection in the Inner Heliosphere
Singh, Talwinder, Kim, Tae K., Pogorelov, Nikolai V. & Arge, Charles N., 2020, Space Weather, 18, e02405
15 Simulating Solar Coronal Mass Ejections Constrained by Observations of Their Speed and Poloidal Flux
Singh, T., Yalim, M. S., Pogorelov, N. V. & Gopalswamy, N., 2019, ApJ, 875, L17
14 Improving the Arrival Time Estimates of Coronal Mass Ejections by Using Magnetohydrodynamic Ensemble Modeling, Heliospheric Imager Data, and Machine Learning
Singh, Talwinder, Benson, Bernard, Raza, Syed A. Z., Kim, Tae K., Pogorelov, Nikolai V., Smith, William P. & Arge, Charles N., 2023, ApJ, 948, 78
7 Inference of magnetic field in the coronal streamer invoking kink wave motions generated by multiple EUV waves
Srivastava, A. K., Singh, Talwinder, Ofman, Leon & Dwivedi, Bhola N., 2016, MNRAS, 463, 1409
5 The Missing Cool Corona in the Flat Magnetic Field around Solar Active Regions
Singh, Talwinder, Sterling, Alphonse C. & Moore, Ronald L., 2021, ApJ, 909, 57
5 GPS as a solar observational instrument: Real-time estimation of EUV photons flux rate during strong, medium, and weak solar flares
Singh, Talwinder, Hernandez-Pajares, Manuel, Monte, Enric, Garcia-Rigo, Alberto & Olivares-Pulido, Germán., 2015, Journal of Geophysical Research (Space Physics), 120, 10,840
2 Propagation of MRT Unstable Plasma Spikes in the Inter-planetary Space
Mishra, Sudheer K., Singh, Talwinder, Kayshap, P. & Srivastava, A. K., 2018, Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles (Editors: Banerjee, D., Jiang, J., Kusano, K. & Solanki, S.), IAU Symposium, 340, p. 237
2 Magnetohydrodynamic Simulation of a Coronal Mass Ejection Observed during the Near-radial Alignment of Solar Orbiter and Earth
Singh, Talwinder, Hegde, Dinesha V., Kim, Tae K. & Pogorelov, Nikolai V., 2025, ApJ, 981, 53
1 Pivot of the Emerging Bipolar Magnetic Region in the Birth of Sigmoidal Solar Active Regions
Moore, Ronald L., Tiwari, Sanjiv K., Aparna, V., Panesar, Navdeep K., Sterling, Alphonse C. & Singh, Talwinder, 2025, ApJ, 989, L54
0 Solar Flare Forecasting Using Machine Learning and SDO/HMI Data: A Multiple Machine Learning Model and Data Curation Technique Comparison Study
Newman, Timothy S., Hall, Christian W., Farris, Luke, Singh, Talwinder, Pogorelov, Nikolai, Benson, Bernard, Raza, Syed & Trital, Prajun, 2025, ApJS, 280, 54
0 Combining local and global magnetohydrodynamic simulation frameworks to understand the evolution of coronal mass ejections
Singh, Talwinder, Sankar Maity, Samriddhi, Chatterjee, Piyali & Pogorelov, Nikolai, 2025, Journal of Astrophysics and Astronomy, 46, 87


Created on Wed Apr 8 04:29:10 2026.