Zobrazeno 1 - 10
of 65
pro vyhledávání: '"Nishtha Sachdeva"'
Autor:
Zhenguang Huang, Gábor Tóth, Jia Huang, Nishtha Sachdeva, Bart van der Holst, Ward B. Manchester
Publikováno v:
The Astrophysical Journal Letters, Vol 965, Iss 1, p L1 (2024)
A potential field solution is widely used to extrapolate the coronal magnetic field above the Sun’s surface to a certain height. This model applies the current-free approximation and assumes that the magnetic field is entirely radial beyond the sou
Externí odkaz:
https://doaj.org/article/2993caf8514e4097a4c5fc401384ab33
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 1, p 1 (2024)
In a previous study, Huang et al. used the Alfvén Wave Solar atmosphere Model, one of the widely used solar wind models in the community, driven by ADAPT-GONG magnetograms to simulate the solar wind in the last solar cycle and found that the optimal
Externí odkaz:
https://doaj.org/article/ded30c7149b54a379332c02a8069f457
Autor:
Zhenguang Huang, Gábor Tóth, Nishtha Sachdeva, Lulu Zhao, Bart van der Holst, Igor Sokolov, Ward B. Manchester, Tamas I. Gombosi
Publikováno v:
The Astrophysical Journal Letters, Vol 946, Iss 2, p L47 (2023)
We describe our first attempt to systematically simulate the solar wind during different phases of the last solar cycle with the Alfvén Wave Solar atmosphere Model (AWSoM) developed at the University of Michigan. Key to this study is the determinati
Externí odkaz:
https://doaj.org/article/228c07f75db94ba587e134ea45b61d1f
Autor:
Nishtha Sachdeva, Ward B. Manchester IV, Igor Sokolov, Zhenguang Huang, Alexander Pevtsov, Luca Bertello, Alexei A. Pevtsov, Gabor Toth, Bart van der Holst, Carl J. Henney
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 2, p 117 (2023)
We explore the performance of the Alfvén Wave Solar atmosphere Model with near-real-time (NRT) synoptic maps of the photospheric vector magnetic field. These maps, produced by assimilating data from the Helioseismic Magnetic Imager (HMI) on board th
Externí odkaz:
https://doaj.org/article/198741a2b9fe41459b4e2f374629199f
Autor:
Sarthak Tandon, Munish Gairola, Parveen Ahlawat, Sheh Rawat, Archana Aggarwal, Kanika Sharma, Sandeep Tiwari, Ahmad M. Karimi, Vinayakumar Muttagi, Nishtha Sachdeva, Manindra Bhushan
Publikováno v:
Journal of the Egyptian National Cancer Institute, Vol 30, Iss 3, Pp 107-115 (2018)
Objectives: Comparison of two fractionation schedules of intensity modulated radiotherapy (IMRT) for locally advanced head and neck cancer – simultaneous integrated boost (SIB-IMRT) and simultaneous modulated accelerated radiotherapy (SMART) boost
Externí odkaz:
https://doaj.org/article/64bb29104b8d437b9815fbd22ffd3f7b
Autor:
Nishtha Sachdeva, Gabor Toth, Ward Manchester, Bart van der Holst, Aniket Jivani, Hongfan Chen
Successful modeling of Coronal Mass Ejections (CMEs) is an important step towards accurately forecasting their space weather impact. Therefore, it is crucial to improve the various models, techniques and tools to reconstruct CMEs while validating sim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fd8cb1cd8bea4bd8e95005ca1e6fb765
https://doi.org/10.5194/egusphere-egu23-8641
https://doi.org/10.5194/egusphere-egu23-8641
Autor:
Aniket Jivani, Nishtha Sachdeva, Zhenguang Huang, Yang Chen, Bart van der Holst, Ward Manchester, Daniel Iong, Hongfan Chen, Shasha Zou, Xun Huan, Gabor Toth
Publikováno v:
Space Weather. 21
Autor:
Nishtha Sachdeva, Richard Frazin, Ward Manchester, Alessandro Bemporad, Federica Frassati, Federico Nuevo, Marco Romoli, Alberto Marcos Vasquez
Publikováno v:
Solar Physics. 297
Autor:
Alberto M. Vásquez, Federico A. Nuevo, Federica Frassati, Alessandro Bemporad, Richard A. Frazin, Marco Romoli, Nishtha Sachdeva, Ward B. Manchester IV
The Metis coronagraph of the Solar Orbiter (SolO) mission records full-Sun images of the solar corona in Lyman-α ultraviolet (UV) radiation and in visible light polarized brightness (pB). This work investigates the utility of a synoptic observationa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8fa8fb02015b2e754e0e9c052fee0c92
https://doi.org/10.21203/rs.3.rs-1631293/v1
https://doi.org/10.21203/rs.3.rs-1631293/v1
Autor:
Nishtha Sachdeva, Gabor Toth, Ward Manchester, Bart van der Holst, Zhenguang Huang, Carl Henney
The first step towards reliable prediction of the impact of solar transients that drive space weather is to accurately model the background solar wind into which these transients propagate. Uncertainties in the plasma environment into which CMEs prop
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7e7b00086ea7d885ba12547a1026ed08
https://doi.org/10.5194/egusphere-egu22-10472
https://doi.org/10.5194/egusphere-egu22-10472