Zobrazeno 1 - 10
of 84
pro vyhledávání: '"SOLAR DIAMETER"'
Publikováno v:
Universe, Vol 10, Iss 2, p 90 (2024)
Solar and lunar eclipses are indeed the first astronomical phenomena which have been recorded since very early antiquity. Their periodicities gave birth to the first luni-solar calendars based on the Methonic cycle since the sixth century before Chri
Externí odkaz:
https://doaj.org/article/dac872e2e4914cd89e474437aff3cb6f
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Alasta, Amro F., Algamudi, Abdulrazag, Qahwaji, Rami S.R., Ipson, Stanley S., Hauchecorne, A., Meftah, M
Yes
PICARD is a space-based observatory hosting the Solar Diameter Imager and Surface Mapper (SODISM) telescope, which has continuously observed the Sun from July 2010 and up to March 2014. In order to study the fine structure of the solar surfa
PICARD is a space-based observatory hosting the Solar Diameter Imager and Surface Mapper (SODISM) telescope, which has continuously observed the Sun from July 2010 and up to March 2014. In order to study the fine structure of the solar surfa
Externí odkaz:
http://hdl.handle.net/10454/16611
Yes
This paper presents a new method that provides the means to detect sunspots on full-disk solar images recorded by the Solar Diameter Imager and Surface Mapper (SODISM) on the PICARD satellite. The method is a totally automated detection proc
This paper presents a new method that provides the means to detect sunspots on full-disk solar images recorded by the Solar Diameter Imager and Surface Mapper (SODISM) on the PICARD satellite. The method is a totally automated detection proc
Externí odkaz:
http://hdl.handle.net/10454/16608
Autor:
Alasta, Amro F., Algamudi, Abdulrazag, Qahwaji, Rami S.R., Ipson, Stanley S., Nagem, Tarek A.
Yes
The surface of the sun often shows visible sunspots which are located in magnetically active regions of the Sun, and whose number is an indicator of the Sun’s magnetic activity. The detection and classification of sunspots are useful techn
The surface of the sun often shows visible sunspots which are located in magnetically active regions of the Sun, and whose number is an indicator of the Sun’s magnetic activity. The detection and classification of sunspots are useful techn
Externí odkaz:
http://hdl.handle.net/10454/16609
Autor:
Erdélyi, Robertus, Damé, Luc, Fludra, Andrzej, Mathioudakis, Mihalis, Amari, T., Belucz, B., Berrilli, F., Bogachev, S., Bolsée, D., Bothmer, V., Brun, S., Dewitte, S., de Wit, T. Dudok, Faurobert, M., Gizon, L., Gyenge, N., Korsós, M. B., Labrosse, Nicolas, Matthews, S., Meftah, M., Morgan, H., Pallé, P., Rochus, P., Rozanov, E., Schmieder, B., Tsinganos, K., Verwichte, E., Zharkov, S., Zuccarello, F., Wimmer-Schweingruber, R.
Publikováno v:
Experimental Astronomy
Erdélyi, R, Damé, L, Fludra, A, Mathioudakis, M, Amari, T, Belucz, B, Berrilli, F, Bogachev, S, Bolsée, D, Bothmer, V, Brun, S, Dewitte, S, de Wit, T D, Faurobert, M, Gizon, L, Gyenge, N, Korsós, M B, Labrosse, N, Matthews, S, Meftah, M, Morgan, H, Pallé, P, Rochus, P, Rozanov, E, Schmieder, B, Tsinganos, K, Verwichte, E, Zharkov, S, Zuccarello, F & Wimmer-Schweingruber, R 2022, ' HiRISE-High-Resolution Imaging and Spectroscopy Explorer-Ultrahigh resolution, interferometric and external occulting coronagraphic science ', Experimental Astronomy, vol. 54, pp. 227–256 . https://doi.org/10.1007/s10686-022-09831-2
Experimental Astronomy, 2022, 54, pp.227-256. ⟨10.1007/s10686-022-09831-2⟩
Experimental Astronomy, 2022, (in press). ⟨10.1007/s10686-022-09831-2⟩
Erdélyi, R, Damé, L, Fludra, A, Mathioudakis, M, Amari, T, Belucz, B, Berrilli, F, Bogachev, S, Bolsée, D, Bothmer, V, Brun, S, Dewitte, S, de Wit, T D, Faurobert, M, Gizon, L, Gyenge, N, Korsós, M B, Labrosse, N, Matthews, S, Meftah, M, Morgan, H, Pallé, P, Rochus, P, Rozanov, E, Schmieder, B, Tsinganos, K, Verwichte, E, Zharkov, S, Zuccarello, F & Wimmer-Schweingruber, R 2022, ' HiRISE-High-Resolution Imaging and Spectroscopy Explorer-Ultrahigh resolution, interferometric and external occulting coronagraphic science ', Experimental Astronomy, vol. 54, pp. 227–256 . https://doi.org/10.1007/s10686-022-09831-2
Experimental Astronomy, 2022, 54, pp.227-256. ⟨10.1007/s10686-022-09831-2⟩
Experimental Astronomy, 2022, (in press). ⟨10.1007/s10686-022-09831-2⟩
Recent solar physics missions have shown the definite role of waves and magnetic fields deep in the inner corona, at the chromosphere-corona interface, where dramatic and physically dominant changes occur. HiRISE (High Resolution Imaging and Spectros
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ef8c2faccd06253b1a95ded90c83f77
Publikováno v:
Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1990 Apr . 330(1615), 487-497.
Externí odkaz:
https://www.jstor.org/stable/53598
Autor:
Becker, L.
Publikováno v:
Philosophical Transactions of the Royal Society of London. Series A, Containing Papers of a Mathematical or Physical Character, 1908 Jan 01. 207, 307-339.
Externí odkaz:
https://www.jstor.org/stable/90962
Autor:
Pettit, Edison
Publikováno v:
The Scientific Monthly, 1938 Nov 01. 47(5), 421-428.
Externí odkaz:
https://www.jstor.org/stable/16864
Autor:
Algamudi, Abdulrazag A.M.
Life on Earth is strongly related to the Sun, which makes it a vital star to study and understand. To improve our knowledge of the way the Sun works, many satellites have been launched into space to monitor the Sun‟s activities where the one of mai
Externí odkaz:
http://hdl.handle.net/10454/19216