Zobrazeno 1 - 10
of 20
pro vyhledávání: '"V. Sarp"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Advances in Astronomy, Vol 2021 (2021)
In this study, we used the flare index (FI) data taken from Kandilli Observatory for the period of 2009–2020. The data sets are analyzed in three categories as Northern Hemisphere, Southern Hemisphere, and total FI data sets. Total FI data set is o
Publikováno v:
Solar Physics. 295
The aim of this study is revisit the physical parameters of umbral dots (UDs) with the latest high resolution observations and contribute to the scientific understanding of their formation and evolution. In this study, we applied a particle tracking
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 481:2981-2985
Autor:
Vasyl Yurchyshyn, Ali Kilcik, Seray Sahin, Atila Özgüç, V. Sarp, Jean-Pierre Rozelot, V. N. Obridko
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 477:293-297
Autor:
Burcin Donmez, Atila Özgüç, Ali Kilcik, Jean-Pierre Rozelot, Vasyl Yurchyshyn, Partha Chowdhury, V. Sarp
In this study we compared the temporal and periodic variations of the Maximum CME Speed Index (MCMESI) and the number of different class (C, M, and X) solar X-Ray flares for the last two solar cycles (Cycle 23 and 24). To obtain the correlation betwe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f3bbe72b4f0e6b9c44a21750d8ac9ab3
Publikováno v:
The Astrophysical Journal. 891:151
The Kodaikanal Archive Program (India) is now available to the scientific community in digital form as daily digitized solar white light pictures, from 1923 to 2011. We present here the solar radius data, obtained after a painstaking effort to remove
Autor:
V. Sarp, Ali Kilcik
Publikováno v:
Volume: 42, Issue: 3 283-292
Turkish Journal of Physics
Turkish Journal of Physics
Two x-ray solar flare parameters (number of flares and peak flux) are compared to geomagnetic and space weather activity indices. The first solar flare parameter, X-ray solar flare number (SFN), is the total number of solar flares observed in a given
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10ea18a64cdf3666938893c86afd543e
https://dergipark.org.tr/tr/pub/tbtkphysics/issue/40696/490312
https://dergipark.org.tr/tr/pub/tbtkphysics/issue/40696/490312
Autor:
V. Sarp, Ali Kilcik
Publikováno v:
Proceedings of the International Astronomical Union. 13:321-322
Solar activity is a chaotic process and there are various approximations to forecast its long term and short term variations. But there is no prediction method that predicts the solar activity exactly. In this study, a nonlinear prediction approach w
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.