Use of the MSG SEVIRI channels in a combined SSM/I, TRMM and geostationary IR method for rapid updates of rainfall

Bibcode
2000ESASP.452...63L
Levizzani, V.; Alberoni, P.P.; Bauer, P.; Bottai, L.; Buzzi, A.; Cattani, E.; Cerviño, M.; Ciotti, P.; Costa, M.J.; Dietrich, S.; Gozzini, B.; Khain, A.; Kidd, C.; Marzano, F.S.; Meneguzzo, F.; Migliorini, S.; Mugnai, A.; Porcu, F.; Prodi, F.; Rizzi, R.; Rosenfeld, D.; Schanz, L.; Smith, E.A.; Tampieri, F.; Torricella, F.; Turk, J.F.; Vicente, G.A.; Zipoli, G.
Referencia bibliográfica

First MSG RAO Workshop, held 17-19 May, 2000, at CNR, Bologna, Italy. Edited by R.A. Harris. European Space Agency ESASP-452, 2000., p.63

Fecha de publicación:
2000
Número de autores
28
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Not Available
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