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Pawan Kumar
Pawan Kumar
Senior Research Fellow, IIT (BHU) Varanasi
在 itbhu.ac.in 的电子邮件经过验证
标题
引用次数
引用次数
年份
The polar precursor method for solar cycle prediction: comparison of predictors and their temporal range
P Kumar, M Nagy, A Lemerle, BB Karak, K Petrovay
The Astrophysical Journal 909 (1), 87, 2021
372021
Physical link of the polar field buildup with the Waldmeier effect broadens the scope of early solar cycle prediction: Cycle 25 is likely to be slightly stronger than Cycle 24
P Kumar, A Biswas, BB Karak
Monthly Notices of the Royal Astronomical Society: Letters 513 (1), L112-L116, 2022
242022
Evolution of the Sun’s activity and the poleward transport of remnant magnetic flux in Cycles 21–24
AV Mordvinov, BB Karak, D Banerjee, EM Golubeva, AI Khlystova, ...
Monthly Notices of the Royal Astronomical Society 510 (1), 1331-1339, 2022
242022
Supercriticality of the dynamo limits the memory of the polar field to one cycle
P Kumar, BB Karak, V Vashishth
The Astrophysical Journal 913 (1), 65, 2021
142021
Exploring the reliability of polar field rise rate as a precursor for an early prediction of solar cycle
A Biswas, BB Karak, P Kumar
Monthly Notices of the Royal Astronomical Society 526 (3), 3994-4003, 2023
112023
Probing the variations in the timing of the Sun’s polar magnetic field reversals through observations and surface flux transport simulations
EM Golubeva, A Biswas, AI Khlystova, P Kumar, BB Karak
Monthly Notices of the Royal Astronomical Society 525 (2), 1758-1768, 2023
92023
Characterizing the solar cycle variability using nonlinear time series analysis at different amounts of dynamo supercriticality: Solar dynamo is not highly supercritical
A Ghosh, P Kumar, A Prasad, BB Karak
The Astronomical Journal 167 (5), 209, 2024
22024
Variabilities in the polar field and solar cycle due to irregular properties of bipolar magnetic suregions
P Kumar, BB Karak, A Sreedevi
Monthly Notices of the Royal Astronomical Society 530 (3), 2895-2905, 2024
2024
Solar cycle variability induced by stochastic fluctuations of BMR properties and at different amounts of dynamo supercriticality
P Kumar
arXiv preprint arXiv:2401.11159, 2024
2024
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