The Instrumentation of the Main Astronomical Observatory of the National Academy of Sciences of Ukraine

Bibcode
1997ASPC..118..372K
Kostik, R. I.; Shchukina, N. G.
Bibliographical reference

1st Advances in Solar Physics Euroconference. Advances in Physics of Sunspots, ASP Conf. Ser. Vol. 118., Eds.: B. Schmieder, J.C. del Toro Iniesta, & M. Vazquez, p. 372.

Advertised on:
0
1997
Number of authors
2
IAC number of authors
1
Citations
1
Refereed citations
0
Description
The instrumentation and observational programs of the Solar Physics Department of the Main Astronomical Observatory are described. The observatory has two solar horizontal telescopes. The first one is the 44 cm telescope located near Kyiv. This telescope has a spectrograph with a double pass system. It was designed for low scattered light and high spectral resolution. The second one is installed at Terskol High-Altitude Station in the Central Caucasus, at an altitude of 3100 m. This 65 cm telescope with its spectrograph is used for simultaneous photoelectric and photographic measurements of five solar spectral regions in the range from 3000 Angstroms to 12000 Angstroms. One of the scientific programs consists in the observation of solar irradiance fluctuations with the DIFOS photometer aboard the Ukraine-Russian satellite CORONAS-I, which was launched on March 2, 1994. These space observations will be continued during the new mission CORONAS-F.
Type
Non-refereed
Solar telescopes

It may interest you

  • Non-refereed
    Workshop summary: Kaons@CERN 2023

    Kaon physics is at a turning point - while the rare-kaon experiments NA62 and KOTO are in full swing, the end of their lifetime is approaching and the future experimental landscape needs to be defined. With HIKE, KOTO-II and LHCb-Phase-II on the table and under scrutiny, it is a very good moment in time to take stock and contemplate about the

    Anzivino, G. et al.

    Advertised on:

    4
    2024
    Bibcode
    2024EPJC...84..377A
    Citations
    0
  • Non-refereed
    Observational evidence of different formation mechanisms of Solar System-type architectures across spectral types

    Despite being the most abundant classes of known exoplanets, super-Earths and mini-Neptunes are absent in our Solar System, and the exact reason for this is still unknown. Some models suggest that cold-Jupiters play a major role in the formation of inner low-mass planets. This could explain the current architecture of our Solar System, and the

    Pinamonti, Matteo et al.

    Advertised on:

    4
    2024
    Bibcode
    2024ESS.....560801P
    Citations
    0
  • Non-refereed
    Measuring the Masses of the TOI-700 Planets with ESPRESSO

    Over the past three decades, astronomers have discovered that small, rocky planets in temperate orbits are common around our neighboring stars. Whether or not these planets can maintain atmospheres is an open question in the field. Recently, considerable attention in this search has been focused on M dwarfs stars, as their small sizes make it

    Gilbert, Emily et al.

    Advertised on:

    4
    2024
    Bibcode
    2024ESS.....560107G
    Citations
    0