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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 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 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 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. | ||
- | <center>[[Image:Ssrt1.jpg]]</center> | + | <center>[[Image: Ssrt1.jpg]]</center> |
{| | {| | ||
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- | |[[Image:Ssrt2.jpg|left]] | + | |[[Image: Ssrt2.jpg|left]] |
|<b>Mission:</b> | |<b>Mission:</b> | ||
* studying solar corona heating, | * studying solar corona heating, | ||
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* monitoring the solar integral flux at a high spectral and temporal resolutions within a wide frequency range. | * monitoring the solar integral flux at a high spectral and temporal resolutions within a wide frequency range. | ||
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- | |[[Image:Ssrt3.jpg|left]] | + | |[[Image: Ssrt3.jpg|left]] |
|<b>Instruments:</b> | |<b>Instruments:</b> | ||
* Siberian Solar Radio Telescope (SSRT) ([https://badary.iszf.irk.ru/ssrt.php https://badary.iszf.irk.ru/ssrt.php]); | * Siberian Solar Radio Telescope (SSRT) ([https://badary.iszf.irk.ru/ssrt.php https://badary.iszf.irk.ru/ssrt.php]); |
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.
Mission:
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Instruments:
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