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Spectral observations of solar active features and dynamic processes in the solar atmosphere.|Sayan_Solar_Observatory}} | Spectral observations of solar active features and dynamic processes in the solar atmosphere.|Sayan_Solar_Observatory}} | ||
- | {{text_box|[[ | + | {{text_box|[[The_Radio-Astrophysical_Observatory|The Radio-Astrophysical Observatory]]|[[Image:Ssrt1.jpg|left|130px]]The Radio-Astrophysical Observatory (RAO) is in the Tunka Valley that separates two ranges of the East Sayan, 220 km from Irkutsk (51°45′33″ N, 102°13′08″ E). The Observatory site survey (https://goo.gl/maps/895pyjucMxabSPKw9) was determined by minimizing technogenous noise. At the moment, the main instruments are a radioheliograph and a suite of integral flux spectro-polarimeters. The RAO staff equals about 40, the operation time being 00–10 UT.|The Siberian Solar Radio Telescope}} |
{{text_box|[[Integrated Magnetic-Ionospheric Observatory]]|[[Image:Magnit1.jpg|left|130px]] General Purposes: | {{text_box|[[Integrated Magnetic-Ionospheric Observatory]]|[[Image:Magnit1.jpg|left|130px]] General Purposes: |
ObservatoriesThe Baikal Astrophysical Observatory (BAO)The Baikal Astrophysical Observatory (BAO) is located in the outskirts of the settlement of Listvyanka on the south shore of Lake Baikal, 70 km far from Irkutsk.
BAO is noted for its remarkable astroclimatic regime due to an antihunt action of big water area and local anticyclon upon air environment. General Purposes: Observations of a thin structure of active solar formations; Registration of solar flares and other non-stationary phenomena in solar atmosphere. More..The Sayan Solar ObservatoryThe observatory is located in the mountains at 2000m altitude.
This is due to the specific character of the observatory's main objectives which require very good seeing for polarization observations and solar corona observations. Main objectives: Measurements of solar magnetic fields; Spectral observations of solar active features and dynamic processes in the solar atmosphere. More..The Radio-Astrophysical ObservatoryThe Radio-Astrophysical Observatory (RAO) is in the Tunka Valley that separates two ranges of the East Sayan, 220 km from Irkutsk (51°45′33″ N, 102°13′08″ E). The Observatory site survey (https://goo.gl/maps/895pyjucMxabSPKw9) was determined by minimizing technogenous noise. At the moment, the main instruments are a radioheliograph and a suite of integral flux spectro-polarimeters. The RAO staff equals about 40, the operation time being 00–10 UT. More.. Integrated Magnetic-Ionospheric Observatory General Purposes:
An origin and diagnostics of geoeffective formations in a solar wind; Modelling of magnetospheric disturbances; Electromagnetic waves in the magnetosphere. A magnetic observatory was established at Irkutsk in 1886 by the Department of National Education. More..Norilsk Integrated Magnetic-Ionospheric Station Data base of Norilsk Neutron Monitor Database contents of Norilsk neutron monitor data starting from 1971 (18NM64): up from January 1971-1981 and from 2000.
The interval of accumulation: hourly from 1971; 1-minute since August 2000. Database updating goes in real time. An interactive access is possible to this database and FTP as well. More..Geophysical Observatory Is located in Tory, 150 km away from Irkutsk.
The major task is monitoring structure and dynamics of the upper and middle atmosphere by passive radiophysical and optical methods. More.. Atmosphere Radio Diagnostics Observatory Observatory is located in the Irkutsk region, 125 km away from Irkutsk. The Irkutsk Radar of Incoherent Scatter (IRIS) that was created on the base of the radar installation “Dnepr” received within the conversion programme of the Soviet Armed Forces. The IISR has a whole set of process equipment, buildings and communication systems and represents a complicated technical complex. Modernization of the system of control, registration and signal processing permits efficient usage of the radar for research into the upper atmosphere with the incoherent scatter technique.
Transmitting complex of the LFM ionosonde of the ionosphere vertical, oblique and oblique back scatter sounding within the frequency range of 1-30 MHz. This complex is the main component of the ISTP SB RAS multiposition LFM ionosonde with remote transmitters in Magadan and Norilsk and a receiver in Tory (the Buryat republic). More.. |
General InformationInstitute of Solar-Terrestrial Physics was founded in 1960 on the basis of the Siberia's oldest geomagnetic observatory formed in 1886. Today it's a big scientific institute. Director - Corresponding member of RAS A.V. Medvedev. Total staff: 507, including 140 researchers, 36 Doctors of Science, 76 Candidates of Science. More.. Major research areas According to the Charter of the Institute, the main fields of research are fundamental, exploratory and applied research studies in the following main research areas: solar physics. near-Earth space physics, problems of asteroid and comet impact hazards and space ecology, analysis and forecast of state of the Earth's climate system.
Space weather monitoring and forecast in an effort to solve a number of applied problems; | |
News[edit] 15:52, 3 May 2023: 14th-Russian-Mongolian-Workshop 2023 First Announcement[edit] FIRST ANNOUNCEMENTThe Institute of the Earth’s Crust of the Siberian Branch RAS, in cooperation with the Institute of Solar-Terrestrial Physics of the Siberian Branch RAS, Siberian Branch RAS and Mongolia Research Center for Astronomy and Geophysics will hold the XIV Russian-Mongolian International Conference on Astronomy and Geophysics in Irkutsk on September 15–20, 2023. More...[edit] 14:00, 29 August 2018: ISW2018[edit] The International Workshop
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