Zobrazeno 1 - 10
of 74
pro vyhledávání: '"Tlatov Andrey G."'
Autor:
Erdélyi Robertus, Korsós Marianna B., Huang Xin, Yang Yong, Pizzey Danielle, Wrathmall Steven A., Hughes Ifan G., Dyer Martin J., Dhillon Vikram S., Belucz Bernadett, Brajša Roman, Chatterjee Piyali, Cheng Xuewu, Deng Yuanyong, Domínguez Santiago Vargas, Joya Raúl, Gömöry Peter, Gyenge Norbert G., Hanslmeier Arnold, Kucera Ales, Kuridze David, Li Faquan, Liu Zhong, Xu Long, Mathioudakis Mihalis, Matthews Sarah, McAteer James R.T., Pevtsov Alexei A., Pötzi Werner, Romano Paolo, Shen Jinhua, Temesváry János, Tlatov Andrey G., Triana Charles, Utz Dominik, Veronig Astrid M., Wang Yuming, Yan Yihua, Zaqarashvili Teimuraz, Zuccarello Francesca
Publikováno v:
Journal of Space Weather and Space Climate, Vol 12, p 2 (2022)
The Solar Activity Magnetic Monitor (SAMM) Network (SAMNet) is a future UK-led international network of ground-based solar telescope stations. SAMNet, at its full capacity, will continuously monitor the Sun’s intensity, magnetic, and Doppler veloci
Externí odkaz:
https://doaj.org/article/bb3757f31cdd4bd883696c991a0a4d01
Publikováno v:
Journal of Space Weather and Space Climate, Vol 11, p 4 (2021)
We briefly review the history of observations of magnetic fields on the Sun, and describe early magnetograps for full disk measurements. Changes in instruments and detectors, the cohort of observers, the knowledge base etc may result in non-uniformit
Externí odkaz:
https://doaj.org/article/79449ce11e894c7faf1328d6bc6e59f1
Autor:
Tlatov, Andrey G.
On modern satellite observations of the Sun in the continuum with high spatial resolution, as well as on high-quality ground observations, a large number of small dark areas can be observed. These regions have no penumbra, have a contrast of up to 20
Externí odkaz:
http://arxiv.org/abs/2205.13142
Autor:
Velasco Herrera, Victor Manuel, Soon, Willie, Babynets, Nelya, Muraközy, Judit, Tlatov, Andrey G., Nagovitsyn, Yury A., Qiu, Shican, Švanda, Michal, Velasco Herrera, Policarpo Arol
Publikováno v:
In Advances in Space Research 1 March 2024 73(5):2788-2815
Autor:
Chatzistergos, Theodosios, Ermolli, Ilaria, Krivova, Natalie A., Solanki, Sami K., Banerjee, Dipankar, Barata, Teresa, Belik, Marcel, Gafeira, Ricardo, Garcia, Adriana, Hanaoka, Yoichiro, Hegde, Manjunath, Klimeš, Jan, Korokhin, Viktor V., Lourenço, Ana, Malherbe, Jean-Marie, Marchenko, Gennady P., Peixinho, Nuno, Sakurai, Takashi, Tlatov, Andrey G.
Publikováno v:
A&A 639, A88 (2020)
We derive the plage area evolution over the last 12 solar cycles employing data from all Ca II K archives available publicly in digital form known to us, including several as yet unexplored Ca II K archives. We analyse more than 290,000 full-disc Ca
Externí odkaz:
http://arxiv.org/abs/2005.01435
Autor:
Pevtsov, Alexei A., Tlatova, Kseniya A., Pevtsov, Alexander A., Heikkinen, Elina, Virtanen, Ilpo, Karachik, Nina V., Bertello, Luca, Tlatov, Andrey G., Ulrich, Roger, Mursula, Kalevi
Publikováno v:
A&A 628, A103 (2019)
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:
http://arxiv.org/abs/1907.06492
We analyzed a small flux rope eruption converted into a helical blowout jet in a fan-spine configuration using multi-wavelength observations taken by SDO, which occurred near the limb on 2016 January 9. In our study, first, we estimated the fan-spine
Externí odkaz:
http://arxiv.org/abs/1802.01798
Autor:
Tlatov, Andrey G.1 (AUTHOR) tlatov@mail.ru
Publikováno v:
Solar Physics. Jul2023, Vol. 298 Issue 7, p1-11. 11p.
Autor:
Muñoz-Jaramillo, Andrés, Senkpeil, Ryan R., Longcope, Dana W., Tlatov, Andrey G., Pevtsov, Alexei A., Balmaceda, Laura A., DeLuca, Edward E., Martens, Petrus C. H.
Publikováno v:
The Astrophysical Journal, 804:68 (12pp), 2015 May 1
In this work we introduce a new way of binning sunspot group data with the purpose of better understanding the impact of the solar cycle on sunspot properties and how this defined the characteristics of the extended minimum of cycle 23. Our approach
Externí odkaz:
http://arxiv.org/abs/1508.01222
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