Publications in Refereed Journals
Khuntia, S., and Mishra, W. (2025). Statistical properties of ICMEs at 1AU (coming soon)
Khuntia, S., and Mishra, W. (2025). Thermal and Turbulence Characteristics of Fast and Slow Coronal Mass Ejections at 1 AU, Journal of Astrophysics and Astronomy (ArXiv: 2505.18296)
Khuntia, S., Mishra, W., and Agarwal, A. (2025). Evolution of interacting coronal mass ejections that drove the great geomagnetic storm of 10 May 2024, Astronomy & Astrophysics, 698, A79, 14 (DOI: 10.1051/0004-6361/202452866) (ArXiv: 2504.03335)
Khuntia, S., Mishra, W., Wang, Y., Mishra, S. K., Nieves-Chinchilla Teresa, and Lyu, S. (2024). Deciphering the Evolution of Thermodynamic Properties and their Connection to the Global Kinematics of High-Speed Coronal Mass Ejections Using FRIS Model, Monthly Notices of the Royal Astronomical Society (MNRAS), stae2523. DOI: 10.1093/mnras/stae2523
Mishra, W., Sahani. P. S., Khuntia, S., and Chakrabarty, D. (2024). " Distribution and recovery phase of geomagnetic storms during solar cycles 23 and 24," Monthly Notices of the Royal Astronomical Society, stae1045. DOI: 10.1093/mnras/stae1045
Khuntia, S., Mishra, W., Mishra, S. K., Wang, Y., Zhang. J., and Lyu, S. (2023). "Unraveling the Thermodynamic Enigma between Fast and Slow Coronal Mass Ejections," The Astrophysical Journal, 958, 92. DOI: 10.3847/1538-4357/ad00ba
Mishra, W., Wang, Y., Lyu, S., and Khuntia, S. (2023). "Erratum: Modeling the Thermodynamic Evolution of Coronal Mass Ejections Using Their Kinematics," The Astrophysical Journal, 952, 173, DOI:10.3847/1538-4357/ace691
Media Articles
1. DST article: Estimations of the heat budget of Solar Coronal Mass Ejections can pave the way for space weather forecasting
2. INDUS seminar: Heating Versus Cooling in CMEs: The Thermal History of Fast and Slow Events Across the Solar Distances
3. DOOT Magazine: Sizzling Roads, Soaring Rockets: A Journey to Witness Aditya L1’s Majestic Lift-Of, Page 7-10
Derived electron and proton polytropic indices at 1 AU, as a proxy to understand the thermal state of magnetic ejecta and surrounding solar wind regions.
FRIS model-derived polytropic index and temperature profile each CMEs near the Sun.
Solar Cycle 23
Solar Cycle 24
SC23: The correlation between the recovery phase duration of single peak (left) and multi-peak (right) storms and storm characteristics
SC24: The correlation between the recovery phase duration of single peak (left) and multi-peak (right) storms and storm characteristics