Zobrazeno 1 - 5
of 5
pro vyhledávání: '"J. I. Campos-Rozo"'
Publikováno v:
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Context. The Sun features on its surface typical flow patterns called the granulation, mesogranulation, and supergranulation. These patterns arise due to convective flows transporting energy from the interior of the Sun to its surface. The other well
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9657fb538b8c9635add1cd0be7608914
Publikováno v:
Proceedings of the International Astronomical Union. 12:86-93
Small-scale kG strong magnetic field elements in the solar photosphere are often identified as so-called magnetic bright points (MBPs). In principle these MBPs represent the cross-section of a vertical, strong, magnetic flux tube which is expanding w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a8fc402faeaff9fbbc41c5e75d86c15d
https://doi.org/10.1017/s174392131700401x
https://doi.org/10.1017/s174392131700401x
Autor:
J. I. Campos-Rozo, S. Vargas Domínguez
Publikováno v:
Proceedings of the International Astronomical Union. 12:25-27
Python is considered to be a mature programming language, besides of being widely accepted as an engaging option for scientific analysis in multiple areas, as will be presented in this work for the particular case of solar physics research. SunPy is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4b9071ff72d979d0c513c299f1ae3ebf
https://doi.org/10.1017/s1743921317003568
https://doi.org/10.1017/s1743921317003568
Publikováno v:
Central European Astrophysical Bulletin
Volume 38
Issue 1
Volume 38
Issue 1
Python programming language has experienced a great progress and growing use in the scientific community in the last years as well as a direct impact on solar physics. Python is a very mature language and almost any fundamental feature you might want
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______951::6fb1c655ce1698875d7e9650d0a15002
https://hrcak.srce.hr/143691
https://hrcak.srce.hr/143691
Autor:
S. J. González Manrique, Christoph Kuckein, S. Vargas Domínguez, D. Utz, P. Zelina, G. Berrios Saavedra, P. Gömöry, J. I. Campos Rozo, H. Balthasar
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Context. High-resolution observations of the solar photosphere reveal the presence of fine structures, in particular the so-called Magnetic Bright Points (MBPs), which are small-scale features associated with strong magnetic field regions of the orde
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3e2e0a731712da43205e21db2d8fbf6f