MISMA inversion of HINODE SOT/SP and IBIS data: Preliminary Results

Bibcode
2008ESPM...12.2.33V
Viticchiè, B.; Berrilli, F.; Sánchez-Almeida, J.; Del Moro, D.
Referencia bibliográfica

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/, p.2.33"

Fecha de publicación:
9
2008
Número de autores
4
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
We present the preliminary results derived from the MISMA inversion of Stokes I and V profiles of FeI 630.1nm FeI 630.2nm lines observed with: 1. SOT/SP instrument aboard the HINODE satellite. 2. IBIS in spectropolarimetric mode imaging, supported by simultaneous white light and G-band images, for blind deconvolution reconstruction. The complete analysis has as a final goal the comparison of the results obtained from the analysis of the two datasets for a reliable statistical description of the quiet Sun through the definition of a probability density function.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    Estimation of the hydrostatic-to-lensing mass bias from resolved cluster masses
    We present a study on the bias of hydrostatic masses with respect to lensing mass estimates for a sample of 53 clusters in a redshift range between z = 0.05 and 1.07. The M 500 mass for each cluster was inferred from X-ray and lensing data, without using a priori observable-mass scaling relations. Cluster masses of our reference analysis were
    Muñoz-Echeverría, M. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300033M
    Número de citas
    0
  • Sin árbitro
    IRAM 30-meter millimeter follow-up of deep OSIRIS-GTC optical surveys
    It is broadly accepted that CO is a reliable tracer of H2 in massive IR (L IR ≳ 10 9 L ⊙) galaxies, and that there are clear correlations between L IR and L' CO that are qualitatively independent of environment and even redshift. We present two tales on the search for 12CO emission from dusty star-forming galaxies in both field (Lockman Hole, z < 0
    Sánchez-Portal, M. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300047S
    Número de citas
    0
  • Sin árbitro
    The NIKA2 Sunyaev-Zeldovich Large Program. Sample and upcoming product public release
    The NIKA2 camera operating at the IRAM 30-m telescope excels in high-angular resolution mapping of the thermal Sunyaev-Zel'dovich effect towards galaxy clusters at intermediate and high-redshift. As part of the NIKA2 guaranteed-time, the SZ Large Program (LPSZ) aims at tSZ-mapping a representative sample of SZ-selected galaxy clusters in the
    Perotto, L. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300040P
    Número de citas
    0