Magnetic flux emergence into the atmosphere

Bibcode
2006IAUS..233...33M
DOI
10.1017/S1743921306001359
Moreno-Insertis, F.
Bibliographical reference

Solar Activity and its Magnetic Origin, Proceedings of the 233rd Symposium of the International Astronomical Union held in Cairo, Egypt, March 31 - April 4, 2006, Edited by Volker Bothmer; Ahmed Abdel Hady. Cambridge: Cambridge University Press, 2006., pp.33-40

Advertised on:
0
2006
Number of authors
1
IAC number of authors
0
Citations
1
Refereed citations
1
Description
Understanding the mechanism that causes the emergence of magnetic flux from the solar interior to the atmosphere, the drastic changes in the properties of the matter and magnetic fields along the rise and the interplay of dynamic and resistive phenomena that shape the emerged regions is one of the major open tasks in solar physics. Important advances are being made both in the theoretical modelling and in the observation of the emergence events. This review concentrates on recent advances through 3D numerical experiments carried out with massively parallel MHD and radiative transfer codes.
Type
Non-refereed

It may interest you

  • Non-refereed
    The luminosity functions of an homogeneous sample of 50 young nearby open clusters
    Open clusters are groups of coeval stars sharing properties such as distance and metallicity, and they are key to understanding stellar evolution. We shed light on the evolution of open clusters with a special focus on the universality of the luminosity function. We applied an upgraded version of the convergent point technique on about 50 open
    Lodieu, Nicolas et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..512L
    Citations
    0
  • Non-refereed
    Gas Flows in the Central Regions of NGC 4593 with Muse
    Gas flows into the centres of galaxies form an important ingredient to the formation, growth and evolution of galaxies. The process of gas falling into the central supermassive black hole (SMBH) can lead to high levels of non-stellar emission which results in an active galactic nucleus (AGN). However, the details of how such gas flows reach the
    Mulumba, Dorcus et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..479M
    Citations
    0
  • Non-refereed
    The effect of local and large scale environment on star formation histories in galaxies
    The environment of galaxies plays a key role in their evolution. The availability of large extragalactic surveys makes it possible to place a galaxy not only in its immediate environment, but also in its position within the large-scale structure of the universe. Within this context, we investigate how the local environment influences the star
    Torres-Ríos, Gloria et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1965T
    Citations
    0