A solar interferometric mission for ultrahigh resolution imaging and spectroscopy: SIMURIS

Bibcode
1991AdSpR..11..383D
DOI
10.1016/0273-1177(91)90135-7
Damé, L.; Acton, L.; Bruner, M.; Connes, P.; Cornwell, T.; Foing, B. H.; Heyvaerts, J.; Lemaire, P.; Martić, M.; Muller, R.; Porteneuve, J.; Roca-Cortés, T.; Riehl, J.; Rutten, R.; Séchaud, M.; Smith, P.; Thorne, A. P.; Title, A. M.; Vial, J.-C.; Visser, H.; Weigelt, G.
Referencia bibliográfica

Advances in Space Research, Volume 11, Issue 1, p. 383-386.

Fecha de publicación:
0
1991
Revista
Advances in Space Research
Número de autores
21
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
SIMURIS is an interferometric investigation of the very fine structure of the solar atmosphere from the photosphere to the corona. It was proposed to ESA /1/, November 30 1989, for the Next Medium Size Mission - M2, and accepted in February 1990 for an Assessment Study in the context of the Space Station. The main scientific objectives will be outlined, and the ambitious model payload featuring the Solar Ultraviolet Network (SUN), a 2 m long monolithic array of 4 telescopes of Ø20 cm, and the Imaging Fourier Transform Spectrometer (IFTS), an UV and Visible Imaging Fourier Transform Spectrometer coupled to a Ø40 cm Gregory, described.
Tipo
Con árbitro

Te puede interesar

  • Con árbitro
    Calibrating the Clock of JWST
    JWST, despite not being designed to observe astrophysical phenomena that vary on rapid timescales, can be an unparalleled tool for such studies. If timing systematics can be controlled, JWST will be able to open up the subsecond infrared timescale regime. Rapid time-domain studies, such as lag measurements in accreting compact objects and solar
    Dhillon, V. S. et al.

    Fecha de publicación:

    1
    2025
    Bibcode
    2025AJ....169...21S
    Número de citas
    0
  • Con árbitro
    Comparing metallicity correlations in nearby non-AGN and AGN-host galaxies
    The gas-phase metallicity distribution within galaxies records critical information about galactic evolution. In this work, we investigate how active galactic nuclei (AGNs) influence this distribution by measuring the two-point correlation functions of gas-phase metallicity in 95 non-AGN and 37 AGN-host galaxies from the Calar Alto Legacy Integral
    Li, Song-Lin et al.

    Fecha de publicación:

    1
    2025
    Bibcode
    2025MNRAS.536..430L
    Número de citas
    1
  • Con árbitro
    Why do some ultra diffuse Galaxies have rich globular cluster systems?
    Some ultra diffuse galaxies (UDGs) reveal many more globular clusters (GCs) than classical dwarf galaxies of the same stellar mass. These UDGs, with a mass in their GC system ( $M_{\rm GC}$) approaching 10 per cent of their host galaxy stellar mass ( $M_{\ast }$), are also inferred to have high halo mass to stellar mass ratios ( $M_{\rm halo}/M_{
    Forbes, Duncan A. et al.

    Fecha de publicación:

    1
    2025
    Bibcode
    2025MNRAS.536.1217F
    Número de citas
    0