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.
Bibliographical reference

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

Advertised on:
0
1991
Journal
Advances in Space Research
Number of authors
21
IAC number of authors
2
Citations
0
Refereed citations
0
Description
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.
Type
Refereed

It may interest you

  • Refereed
    Copacabana: a probabilistic membership assignment method for galaxy clusters
    Cosmological analyses using galaxy clusters in optical/near-infrared photometric surveys require robust characterization of their galaxy content. Precisely determining which galaxies belong to a cluster is crucial. In this paper, we present the COlor Probabilistic Assignment of Clusters And BAyesiaNAnalysis (Copacabana) algorithm. Copacabana
    Esteves, J. H. et al.

    Advertised on:

    1
    2025
    Bibcode
    2025MNRAS.536..931E
    Citations
    1
  • Refereed
    Constraints on compact objects from the Dark Energy Survey 5-yr supernova sample
    Gravitational lensing magnification of Type Ia supernovae (SNe Ia) allows information to be obtained about the distribution of matter on small scales. In this paper, we derive limits on the fraction $\alpha$ of the total matter density in compact objects (which comprise stars, stellar remnants, small stellar groupings, and primordial black holes)
    Shah, P. et al.

    Advertised on:

    1
    2025
    Bibcode
    2025MNRAS.536..946S
    Citations
    0
  • Refereed
    Multiband Optical Variability of the Blazar 3C 454.3 on Diverse Timescales
    Due to its peculiar and highly variable nature, the blazar 3C 454.3 has been extensively monitored by the WEBT team. Here, we present for the first time these long-term optical flux and color variability results using data acquired in B, V, R, and I bands over a time span of about two decades. We include data from WEBT collaborators and public
    Dogra, Karan et al.

    Advertised on:

    1
    2025
    Bibcode
    2025ApJS..276....1D
    Citations
    0