Zobrazeno 1 - 10
of 2 028
pro vyhledávání: '"Bhatia, A. S."'
Autor:
Smitha, H. N., Shapiro, Alexander I., Witzke, Veronika, Kostogryz, Nadiia M., Unruh, Yvonne C., Bhatia, Tanayveer S., Cameron, Robert, Seager, Sara, Solanki, Sami K.
Accurate calculations of starspot spectra are essential for multiple applications in astronomy. The current standard is to represent starspot spectra by spectra of stars that are cooler than the quiet star regions. This implies approximating a starsp
Externí odkaz:
http://arxiv.org/abs/2411.14056
Publikováno v:
A&A 681, A32 (2023)
Some of the quiet solar magnetic flux could be attributed to a small-scale dynamo (SSD) operating in the convection zone. An SSD operating in cool main-sequence stars is expected to affect the atmospheric structure, in particular the convection, and
Externí odkaz:
http://arxiv.org/abs/2311.02286
Autor:
Witzke, Veronika, Shapiro, Alexander I., Kostogryz, Nadiia M., Mauviard, Lucien, Bhatia, Tanayveer S., Cameron, Robert, Gizon, Laurent, Przybylski, Damien, Solanki, Sami K., Unruh, Yvonne C., Yue, Li
Publikováno v:
A&A 681, A81 (2024)
Three-dimensional (3D) radiative magnetohydrodynamics (MHD) simulations are the only way to model stellar atmospheres without any ad hoc parameterisations. Several 3D radiative MHD codes have achieved good quantitative agreement with observables for
Externí odkaz:
http://arxiv.org/abs/2310.05652
Autor:
Witzke, V., Duehnen, H. B., Shapiro, A. I., Przybylski, D., Bhatia, T. S., Cameron, R., Solanki, S. K.
Publikováno v:
A&A 669, A157 (2023)
All cool main sequence stars including our Sun are thought to have magnetic fields. Observations of the Sun revealed that even in quiet regions small-scale turbulent magnetic fields are present. Simulations further showed that such magnetic fields af
Externí odkaz:
http://arxiv.org/abs/2211.02722
Autor:
Bhatia, Tanayveer S., Cameron, Robert H., Solanki, Sami K., Peter, Hardi, Przybylski, Damien, Witzke, Veronika, Shapiro, Alexander
Publikováno v:
A&A 663, A166 (2022)
Some of the small-scale solar magnetic flux can be attributed to a small-scale dynamo (SSD) operating in the near-surface convection. The SSD fields have consequences for solar granular convection, basal flux, as well as chromospheric heating. A simi
Externí odkaz:
http://arxiv.org/abs/2206.00064
Autor:
Bhatia, Harpreet S., Dweck, Marc R., Craig, Neil, Capoulade, Romain, Pibarot, Philippe, Trainor, Patrick J., Whelton, Seamus P., Rikhi, Rishi, Lidani, Karita C.F., Post, Wendy S., Tsai, Michael Y., Criqui, Michael H., Shapiro, Michael D., Budoff, Matthew J., DeFilippis, Andrew P., Thanassoulis, George, Tsimikas, Sotirios
Publikováno v:
In Journal of the American College of Cardiology 17-24 December 2024 84(25):2430-2441
Autor:
Nomura, Sarah O., Bhatia, Harpreet S., Garg, Parveen K., Karger, Amy B., Guan, Weihua, Cao, Jing, Shapiro, Michael D., Tsai, Michael Y.
Publikováno v:
In American Journal of Preventive Cardiology March 2025 21
Autor:
Nargund, Raghavendra1 (AUTHOR) raghavendra.nargund@icar.gov.in, Bhatia, Virender S.1 (AUTHOR) bhatia_virender_singh@hotmail.com, Sinha, Nishant K.2 (AUTHOR) nishant.sinha@icar.gov.in, Mohanty, Monoranjan2 (AUTHOR), Jayaraman, Somasundaram3 (AUTHOR) somajayaraman@gmail.com, Dang, Yash P.4 (AUTHOR) nishant.sinha@icar.gov.in, Nataraj, Vennampally1 (AUTHOR) vennampally.nataraj@icar.gov.in, Drewry, Darren5 (AUTHOR) drewry.19@osu.edu, Dalal, Ram C.4 (AUTHOR)
Publikováno v:
Agronomy. Sep2024, Vol. 14 Issue 9, p1929. 20p.
Autor:
Lidani, Karita Claudia Freitas, Trainor, Patrick James, Bhatia, Harpreet S., Nasir, Khurram, Blaha, Michael J., Tsai, Michael Y., Gottesman, Rebecca F., Post, Wendy S., Thanassoulis, George, Tsimikas, Sotirios, Heckbert, Susan R., DeFilippis, Andrew Paul
Publikováno v:
In Atherosclerosis March 2024 390
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