Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Íñigo Arregui"'
Autor:
Andrés Asensio Ramos, Íñigo Arregui
Bayesian methods are being increasingly employed in many different areas of research in the physical sciences. In astrophysics, models are used to make predictions to be compared to observations. These observations offer information that is incomplet
Publikováno v:
International Journal of Computer Mathematics. :1-21
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b080d3405f79585a3c02a5df411b9988
https://doi.org/10.1080/00207160.2023.2172322
https://doi.org/10.1080/00207160.2023.2172322
Magnetohydrodynamic Processes in The Solar Plasma provides comprehensive and up-to-date theory and practice of the fundamentals of heliospheric research and the Sun's basic plasma processes, covering the dynamics of the solar interior to its exterior
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 1, p 68 (2024)
Magnetohydrodynamic kink waves naturally form as a consequence of perturbations to a structured medium, for example, transverse oscillations of coronal loops. Linear theory has provided many insights into the evolution of linear oscillations, and res
Externí odkaz:
https://doaj.org/article/6ae569744f2248a3947a78213b0d9419
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 1, p 69 (2024)
Estimating the magnetic field strength in the solar corona is crucial for understanding different physical processes happening over diverse spatiotemporal scales. However, the high temperatures and low density of the solar corona make this task chall
Externí odkaz:
https://doaj.org/article/6109fc63ce5a46cb9b2a8549cfca22d5
Autor:
Iñigo Arregui
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
Solar coronal seismology is based on the remote diagnostics of physical conditions in the corona of the Sun by comparison between model predictions and observations of magnetohydrodynamic wave activity. Our lack of direct access to the physical syste
Externí odkaz:
https://doaj.org/article/22defd879a6d46e8bd583f7b79459134
Publikováno v:
Living Reviews in Solar Physics, Vol 15, Iss 1, Pp 1-154 (2018)
Abstract Prominences are intriguing, but poorly understood, magnetic structures of the solar corona. The dynamics of solar prominences has been the subject of a large number of studies, and of particular interest is the study of prominence oscillatio
Externí odkaz:
https://doaj.org/article/1df2970dbe4a4db0b580bbf41fab44e2
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 6 (2019)
This paper investigates the mixed properties of MHD waves in a non-uniform plasma. It starts with a short revision of MHD waves in a uniform plasma of infinite extent. In that case the MHD waves do not have mixed properties. They can be separated in
Externí odkaz:
https://doaj.org/article/fc7f5df7037c44eda1488a93892f907d
Publikováno v:
Living Reviews in Solar Physics, Vol 9, p 2 (2012)
Prominences are intriguing, but poorly understood, magnetic structures of the solar corona. The dynamics of solar prominences has been the subject of a large number of studies, and of particular interest is the study of prominence oscillations. Groun
Externí odkaz:
https://doaj.org/article/7573d614555b4db394c2f5f41270ba63