Observations of Jupiter around 80 microns at high spectral resolution

Bibcode
1978A&A....64...61B
Baluteau, J. P.; Marten, A.; Bussoletti, E.; Anderegg, M.; Moorwood, A. F. M.; Beckman, J. E.; Coron, N.
Referencia bibliográfica

Astronomy and Astrophysics, vol. 64, no. 1-2, Mar. 1978, p. 61-65.

Fecha de publicación:
3
1978
Revista
Astronomy and Astrophysics
Número de autores
7
Número de autores del IAC
0
Número de citas
15
Número de citas referidas
14
Descripción
High-resolution (up to 0.02 kayser) airborne spectral observations of Jupiter in the range from 105 to 140 kaysers are presented. The procedures used to remove the effects of telluric opacity and for the brightness-temperature calibration are described. The resulting spectrum is compared with recent calculations for different Jovian models. Some constraints on the NH3 column density above the temperature-inversion level are derived.
Tipo
Con árbitro
Atmósferas planetarias
Temperatura de brillo
Júpiter
Espectroscopia

Te puede interesar

  • Con árbitro
    An ultra-short-period super-Earth with an extremely high density and an outer companion
    We present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC 201595106). K2-360 was first identified in K2 photometry as the host of an ultra-short-period (USP) planet candidate with a period of 0.88 d. We obtained follow-up transit photometry, confirming the star as the host of the signal
    Livingston, John H. et al.

    Fecha de publicación:

    11
    2024
    Bibcode
    2024NatSR..1427219L
    Número de citas
    0
  • Con árbitro
    Neural calibration of imaging Stokes polarimeters
    Current polarimetric calibration techniques derive the instrument modulation matrix by numerically fitting an instrumental model to measurements of a set of calibration Stokes vectors. These techniques are typically limited to an error on the retrieved normalized Stokes Q, U and V parameters, in the $1\times10^{-2}$ to $1\times10^{-3}$ range. This
    Iglesias, F. A. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024BAAA...65..281I
    Número de citas
    0
  • Con árbitro
    Model-based identification of solar coronal mass ejections using deep neural networks
    Coronal mass ejections (CMEs) are a major driver of space weather and thus can have important negative technological and social impacts. To assess their geoeffectiveness once they are ejected, it is crucial their prompt identification in coronagraph images. In the last decade, deep neural networks (DNN) have experienced enormous improvements in
    Iglesias, F. A. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024BAAA...65...17I
    Número de citas
    0