Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Alexander Pevtsov"'
Autor:
Azim Ahmadzadeh, Rohan Adhyapak, Kartik Chaurasiya, Laxmi Alekhya Nagubandi, V. Aparna, Petrus C. Martens, Alexei Pevtsov, Luca Bertello, Alexander Pevtsov, Naomi Douglas, Samuel McDonald, Apaar Bawa, Eugene Kang, Riley Wu, Dustin J. Kempton, Aya Abdelkarem, Patrick M. Copeland, Sri Harsha Seelamneni
Publikováno v:
Scientific Data, Vol 11, Iss 1, Pp 1-15 (2024)
Abstract We present the Manually Annotated GONG Filaments in H-alpha Observations (MAGFiLO v1.0) dataset. This dataset contains 10,244 annotated filaments from 1,593 observations captured by the Global Oscillation Network Group (GONG), spanning the y
Externí odkaz:
https://doaj.org/article/13a69e292c4f40f0b27193c2e121b83f
Autor:
Tong Shi, Ward Manchester IV, Enrico Landi, Bart van der Holst, Judit Szente, Yuxi Chen, Gábor Tóth, Luca Bertello, Alexander Pevtsov
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 1, p 60 (2024)
The coronal heating problem has been a major challenge in solar physics, and a tremendous amount of effort has been made over the past several decades to solve it. In this paper, we aim at answering how the physical processes behind the Alfvén wave
Externí odkaz:
https://doaj.org/article/6a53fc6e31e94624bce5a9817af1bf63
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:
Nishtha Sachdeva, Ward B Manchester, Igor Sokolov, Zhenguang Huang, Alexander Pevtsov, Luca Bertello, Alexei A Pevtsov, Gabor Toth, Bart Van Der Holst
We explore model performance for the Alfvén Wave Solar atmosphere Model (AWSoM) with near-9 real-time (NRT) synoptic maps of the photospheric vector magnetic field. These maps, produced by 10 assimilating data from the Helioseismic Magnetic Imager (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1acc61569e7c851f364a56d9fe6e3306
Autor:
Ward Manchester, Tong Shi, Enrico Landi, Bart Van Der Holst, Judit Szente, Yuxi Chen, Gábor Tóth, Luca Bertello, Alexander Pevtsov
5 For the first time, we simulate the detailed spectral line emission from a solar active 6 region (AR) with the Alfven Wave Solar Model (AWSoM). We select an AR appearing 7 near disk center...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3dcd9062e0c28137d580e65d9185534b
https://doi.org/10.1002/essoar.10508137.1
https://doi.org/10.1002/essoar.10508137.1
Autor:
Tong Shi, Ward Manchester IV, Enrico Landi, Bart van der Holst, Judit Szente, Yuxi Chen, Gábor Tóth, Luca Bertello, Alexander Pevtsov
Publikováno v:
The Astrophysical Journal. 928:34
For the first time, we simulate the detailed spectral line emission from a solar active region (AR) with the Alfvén Wave Solar Model (AWSoM). We select an AR appearing near disk center on 2018 July 13 and use the National Solar Observatory’s Helio
Autor:
Nina V. Karachik, Roger K. Ulrich, Kalevi Mursula, Alexei A. Pevtsov, Alexander Pevtsov, Elina Heikkinen, Luca Bertello, Ilpo Virtanen, Kseniya A. Tlatova, Andrey Tlatov
Context. Systematic observations of magnetic field strength and polarity in sunspots began at Mount Wilson Observatory (MWO), USA in early 1917. Except for a few brief interruptions, this historical dataset continues till present. Aims. The sunspot f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d4224f5e9de2309f183c160e1f77de5
http://arxiv.org/abs/1907.06492
http://arxiv.org/abs/1907.06492
Autor:
Nina V. Karachik, Kalevi Mursula, K. A. Tlatova, Valeria V. Vasil’eva, Alexei A. Pevtsov, Andrey Tlatov, Alexander Pevtsov, Elina Heikkinen, Luca Bertello, Ilpo Virtanen
We use recently digitized sunspot drawings from Mount Wilson Observatory to investigate the latitudinal dependence of tilt angles of active regions and its change with solar cycle. The drawings cover the period from 1917 to present and contain inform
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e327c8a18104842ba315027b5a93389d
http://arxiv.org/abs/1807.07913
http://arxiv.org/abs/1807.07913