Solar Luminosity Oscillation Telescope (SLOT)

Bibcode
1988ESASP.286..175A
Andersen, Bo Nyborg; Domingo, V.; Jones, A. R.; Korzennik, Sylvain G.; Jimenez, A.; Palle, Pere L.; Regulo, C.; Roca Cortés, Teodoro
Referencia bibliográfica

In its Seismology of the Sun and Sun-Like Stars p 175-176 (SEE N89-25819 19-92)

Fecha de publicación:
12
1988
Número de autores
8
Número de autores del IAC
0
Número de citas
6
Número de citas referidas
6
Descripción
Low degree l=0-2 solar p-modes were detected with the SLOT instruments at Izana and Baja California. The main source of noise for these ground based observations is in the terrestrial atmosphere. However, the data acquisition system still has to have very low intrinsic noise. It is shown how this is achieved in the SLOT instruments. Design and operating principles of the photometers and data acquisition system are outlined.
Tipo
Sin árbitro
Observatorios solares
Oscilaciones solares
Radiación solar
Telescopios

Te puede interesar

  • Sin árbitro
    Massive characterisation of subgiants and red giants with TESS (Kepler and Gaia)
    TESS serves as a formidable tool for investigating stellar variability. Nonetheless, the adaptation of methodologies employed in other space missions, such as Kepler, to deduce long stellar rotation periods or solar-like stellar pulsations has been a challenge. The advent of multiple sectors of data for most stars every two years with the extended
    García, Rafael A. et al.

    Fecha de publicación:

    9
    2024
    Bibcode
    2024tkas.confE.123G
    Número de citas
    0
  • Sin árbitro
    a Study of Post-Agb Stars in the Light of GAIA DR3 Data
    Low and intermediate-mass stars evolve through the Post Asymptotic Giant Branch (post-AGB) phase before they reach the Planetary Nebulae stage. After leaving the Main Sequence, they undergo intense episodes of mass loss when in the Giant Branch and, then, they enter the post-AGB stage which is a rather puzzling stellar evolutionary phase . Also, it
    Manteiga, Minia et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024IAUGA..32P1413M
    Número de citas
    0
  • Sin árbitro
    Unsupervised classification of RR Lyrae stars
    Big datasets are becoming increasingly important in astrophysics due to new surveys continuously observing our night sky. A prominent example of an observatory that will produce a large data stream is Vera C. Rubin LSST, designed to simultaneously monitor the southern night sky in six colors. Unsupervised machine learning (ML), a method of learning
    Steinwender, Lukas et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024tkas.confE...2S
    Número de citas
    0