THE SERIES OF ULTRA-LOW-NOISE RECEIVERS AND RADIOMETERS ON BASED OF COOLING TRANSISTOR'S AMPLIFIERS.
      Joint-Stock Company "Saturn" has developed the series of
ultra-low-noise receivers and radiometers, cooling to cryogenic temperatures and operating
in frequency range from 1.0 up to 43 GHz with 5-45 K noise temperature.
      It is possible to use a cooled mixer at the device input.
In this case the operating frequency range can be widened up to 300 GHz.
      Ultra-low-noise receivers are executed on base of cooled up to 12-15K
of the transistor amplifiers, in which are installed the high electron mobility transistors
(HEMT).
      The cooling of transistor amplifier and input path is provided by
microcryogenic closed-type system of hydrogen level.
      The radiotelescopes RT-22, RT-70 (Ukraine), RATAN-600, RT-64,
RTF-32 (Russia), and also the radiotelescopes with dish 25-m diameter in Shanghai and Urumgi
(China) are equipped with the radiometers developed in "Saturn".
      Input microwave channels of the devices in 1.5-2.3GHz range are
performed on the base of 7/3 mm coaxial line; in other ranges - on the base of standard
rectangular waveguides. The output microwave channels in 1-18 GHz frequency range are
performed on the base of 3.5/1.5 mm coaxial line; in other ranges - on base of standard
waveguides.
      The ultra-low-noise receiving SYSTEMS are not serial products, and
its are manufactured according to individual order under particular tasks. The estimated
cost of such system from $80.000 up to $320.000, depending on reguired kits and ordered
frequency range.

THE MAIN PARAMETERS OF RECEIVERS
| Fo, GHz | F, % | Noise temperature, K | Gain, dB | VSWR in/out | Quantity of case. |
| 1,5 | 15 | 6 | 35 | 1.3/1.5 | 2 |
| 2,3 | 15 | 7 | 35 | 1.3/1.5 | 2 |
| 3,7 | 15 | 6 | 30 | 1.3/1.5 | 2 |
| 4,8 | 15 | 7 | 30 | 1.3/1.5 | 2 |
| 7,5 | 15 | 9 | 30 | 1.3/1.5 | 3 |
| 8,5 | 15 | 10 | 30 | 1.3/1.5 | 3 |
| 11,2 | 15 | 12 | 30 | 1.3/1.5 | 3 |
| 22,0 | 15 | 20 | 30 | 1.3/1.5 | 3 |
| 30,0 | 15 | 25 | 28 | 1.3/1.5 | 3 |
| 37,0 | 15 | 30 | 30 | 1.3/1.5 | 4 |
| 43,0 | 15 | 35 | 28 | 1.3/1.5 | 4 |
THE MAIN PARAMETERS OF RADIOMETERS
| Designation | Frequency range, GHz | IF range, MHz | Noise temperature, K | Gain, dB |
| CS 022101 | 1,38 - 1,72 | 100 - 440 | 6 | 55 |
| CS 022102 | 2,15 - 2,50 | 100 - 450 | 7 | 55 |
| CS 022103 | 4,60 - 5,10 | 100 - 600 | 7 | 55 |
| CS 022104 | 8,18 - 8,68 | 100 - 600 | 12 | 55 |
| CS 022105 | 22,0 - 22,5 | 100 - 600 | 25 | 55 |
ULTRA-LOW-NOISE CRYOGENICALY COOLED AMPLIFIERS

CONSTITUTIVE PROPERTIES
| Fo,GHz | 1,5 | 2,3 | 3,9 | 4,8 | 5,9 | 7,5 | 8,5 | 11,2 | 22,0 | 30,0 | 37,0 | 43,0 |
Noise temperature, K (in frequency band 20%) | 6 | 7 | 7 | 8 | 9 | 10 | 12 | 15 | 25 | 30 | 35 | 40 |
THE BLOCK DIAGRAM OF ULTRA-LOW-NOISE RADIOMETER

      1,2. Directional couplers.
      3. Calibration noise generator.
      4. Communication unit.
      5. Cooled transistor amplifier.
      6. Noise generator of compensation.
      7. Thermostabilization device.
      8. Modulator.
      9. Microcryogenic system.
      10. Amplifier.
      11. Supply unit.
      12. RF filter.
      13. Mixer.
      14. IF amplifier.
      15. IF filter.
      16. Device of thermostabilization.
      17. Block of remote control and diagnostics.
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