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
    The variability patterns of the TeV blazar PG 1553 + 113 from a decade of MAGIC and multiband observations

    PG 1553 + 113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray band. The source is also a very high energy (VHE; >100 GeV) gamma-ray emitter. To better understand its properties and identify the underlying physical processes driving its variability, the MAGIC Collaboration initiated a multiyear, multiwavelength

    Abe, H. et al.

    Fecha de publicación:

    4
    2024
    Bibcode
    2024MNRAS.529.3894A
    Número de citas
    0
  • Con árbitro
    First characterization of the emission behavior of Mrk 421 from radio to very high-energy gamma rays with simultaneous X-ray polarization measurements

    Aims: We have performed the first broadband study of Mrk 421 from radio to TeV gamma rays with simultaneous measurements of the X-ray polarization from IXPE. Methods: The data were collected as part of an extensive multiwavelength campaign carried out between May and June 2022 using MAGIC, Fermi-LAT, NuSTAR, XMM-Newton, Swift, and several optical

    Abe, S. et al.

    Fecha de publicación:

    4
    2024
    Bibcode
    2024A&A...684A.127A
    Número de citas
    0
  • Con árbitro
    Effects of density and temperature variations on the metallicity of Mrk 71

    In a very recent work, [1] claim that the scenario of temperature inhomogeneities proposed by [2] ($t2$ > 0) is not able to explain the O$^{2+}$/H$^{+}$ abundance discrepancy observed between the calculations based on the optical [OIII] collisional excited lines (CELs) and the OII recombination lines (RLs) in the star forming galaxy Mrk71. In this

    Méndez-Delgado, J. Eduardo et al.

    Fecha de publicación:

    3
    2024
    Bibcode
    2024NatAs...8..275M
    Número de citas
    2