Publications in Refereed Journals
Khuntia, S., and Mishra, W. (2025), Thermal properties of interplanetary coronal mass ejections at 1 AU and their connection to geoeffectiveness across solar cycles 23-25, accepted in MNRAS (ArXiv: 2512.15155)
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, 46, 70 (DOI: 10.1007/s12036-025-10085-5)
(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: Solar blasts that lit up Ladakh Skies May last year uncoded
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
4. DST article: Estimations of the heat budget of Solar Coronal Mass Ejections can pave the way for space weather forecasting
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