Radiative Relaxation in Small Scale Structures

Bibcode
1987rfsm.conf..281T
Trujillo-Bueno, J.; Kneer, F.
Bibliographical reference

The Role of Fine-Scale Magnetic Fields on the Structure of the Solar Atmosphere, Proceedings of the Inaugural workshop and round table discussion for the D-E-S Telescope installations on the Canary Islands, La Laguna, Tenerife, Spain, 6-12 October 1986. Edited by E.-H. Schröter, M. Vázquez, and A.A. Wyller. Cambridge: Cambridge University Press, 1987., p.281

Advertised on:
0
1987
Number of authors
2
IAC number of authors
0
Citations
1
Refereed citations
1
Description
The authors discuss the effects of multidimensional radiative transfer on the energy exchange by radiation in small-scale structures.
Type
Non-refereed

It may interest you

  • Non-refereed
    EST preliminary design, status and future steps
    The European Solar Telescope (EST) aims to significantly improve our capabilities to observe the solar chromosphere and understanding the solar chromosphere represents one of the most challenging tasks in solar physics. EST incorporates the most innovative technology, with a simple and efficient design, and the most advanced instrumentation to
    Barreto, Mary et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..695B
    Citations
    0
  • Non-refereed
    The Galactic underdogs: characterizing a population of metal-poor stars with disc kinematics in the Milky Way
    To deepen our knowledge of the early history of the Milky Way, it is of particular interest to investigate the orbital and chemical properties of the most metal-poor stars, which are commonly associated with the oldest stars in our Universe. With the advent of astrometric (Gaia), spectroscopic (APOGEE, GALAH, LAMOST, Gaia-RVS), and photometric
    Gonzalez Rivera, Isaure et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..624G
    Citations
    0
  • Non-refereed
    Inferring stellar population properties from HST+JWST photometry using Normalizing Flows
    Spectral energy distributions (SEDs) encode information about the stellar populations within galaxies. By investigating the properties of these stars, such as their ages, masses, and metallicities, we can gain insights into the underlying physical processes that drive the growth and transformation of galaxies over cosmic time. For this purpose, we
    Iglesias Navarro, Patricia et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..225I
    Citations
    0