The Radio-Astrophysical Observatory

From ISTP SB RAS

(Difference between revisions)
Revision as of 08:27, 17 June 2021 (edit)
Admin (Talk | contribs)

← Previous diff
Revision as of 08:30, 17 June 2021 (edit) (undo)
Admin (Talk | contribs)

Next diff →
Line 1: Line 1:
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>
{| {|
|- |-
-|[[Image:Ssrt2.jpg|left]]+|[[Image: Ssrt2.jpg|left]]
|<b>Mission:</b> |<b>Mission:</b>
* studying solar corona heating, * studying solar corona heating,
Line 15: Line 15:
* 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.
|- |-
-|[[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]);

Revision as of 08:30, 17 June 2021

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.

Image: Ssrt1.jpg
Mission:
  • studying solar corona heating,
  • investigating solar flares,
  • measuring coronal magnetic fields,
  • monitoring coronal mass ejections,
  • all-weather multiwave monitoring of solar activity,
  • multiwave mapping of the Sun in the microwave range,
  • monitoring the solar integral flux at a high spectral and temporal resolutions within a wide frequency range.
Instruments:
Log in / create account