First Steps Towards the Electronic Inversion of the Radiative Transfer Equation

Bibcode
2006ASPC..358..177C
Castillo Lorenzo, J. L.; Orozco Suárez, D.; Bellot Rubio, L. R.; Jiménez, L.; Del Toro Iniesta, J. C.
Referencia bibliográfica

Solar Polarization 4, ASP Conference Series, Vol. 358, Proceedings of the conference held 19-23 September, 2005, in Boulder, Colorado, USA. Edited by R. Casini and B. W. Lites, p.177

Fecha de publicación:
12
2006
Número de autores
5
Número de autores del IAC
0
Número de citas
2
Número de citas referidas
1
Descripción
The radiative transfer equation (RTE) gives us information about how the light streams through the medium. It must be inverted in order to obtain the properties of the medium that generated the observation. While there are a number of well discussed methods to approach the solution of the inversion, none of them is suitable for the real-time analysis of high-resolution images due to their computational requirements. This document introduces an electronic inverter for the RTE, suitable for real-time inversion and mainly intended for space missions and on-line ground-based observations.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    RAD@home Citizen Scientists Uncover Emerging Jet-Galaxy Interactions
    The RAD12 object's recent investigation (Hota et al. 2022), via the RAD@home Astronomy Collaboratory, has provided a streamlined and focused perspective on the complex subject of jet-galaxy interactions, which has always posed a significant challenge for observational confirmation. This emerging field holds increasing significance, providing a
    Hota, Ananda et al.

    Fecha de publicación:

    1
    2024
    Bibcode
    2024asi..confP..76H
    Número de citas
    0
  • Sin árbitro
    A Disc Wind Where You Least Expect It: The Outflow in the Short-period X-ray Binary UW CrB
    Studying outflows of low mass X-ray binaries (LMXBs) is important for understanding the physics of accretion, the evolution of compact binaries, and dynamics of the local interstellar medium. One significant source of these outflows is the accretion disc wind, which can blow away vast amounts of material from the disc before it can be accreted on
    Fijma, Stefanie et al.

    Fecha de publicación:

    5
    2024
    Bibcode
    2024HEAD...2150106F
    Número de citas
    0
  • Sin árbitro
    Constraining the core-rotation rate along the red-giant evolution
    The evolution of the core rotation rate of red giant stars is a key parameter in understanding the stellar behavior in the late phases of stellar evolution. Thanks to the mixed-dipole modes, we can constrain the core rotation and internal rotational gradient as a star advances through the red-giant phase. This master thesis presents a pipeline
    Muntean, N. et al.

    Fecha de publicación:

    3
    2024
    Bibcode
    2024aecc.conf...34M
    Número de citas
    0