Kosmos 122
Kosmos 122, launched on 25 June 1966, Meteor No.5L, and was one of eleven weather satellites put into orbit between 1964 and 1969.
This launch was dubbed a Kosmos satellite mission because that was the designation given to prototype satellites by the Soviet Union. Kosmos 122 was the first announced Russian meteorological satellite and the last in a series of prototype meteorological satellites that included Kosmos 44, Kosmos 58, Kosmos 100, and Kosmos 118. It was the last meteorological satellite launched from the Baikonur site with a Vostok-2M launch vehicle at an orbital inclination of 65.0°, and it provided a transition from the prototype series to the Kosmos "Meteor" experimental weather satellite system. The deployment of two other satellites, Kosmos 144 and Kosmos 156, helped create the first Soviet weather forecasting network. Kosmos 122 and the other satellites had two cameras on board, one high resolution and one infrared in order to see the weather day or night. The Kosmos 122 was a successful mission and this specific satellite was used for four months. These satellites were used until 1969 when they were replaced with an upgraded model officially called Meteor.
Spacecraft
The satellite was in the form of a large cylindrical capsule, long and in diameter. Two large solar cell panels of three segments each were deployed from opposite sides of the cylinder after satellite separation from the launch vehicle. The solar panels were rotated to constantly face the Sun during satellite daytime by means of a Sun sensor-controlled drive mechanism fitted in the top end of the center body.The meteorological instruments were housed in a hermetically sealed compartment located in the lower part of the capsule, while the basic satellite servicing systems were contained in a special hermetically sealed compartment in the upper part of the capsule. Data were transmitted to Earth at a frequency of 90 MHz by means of a steerable high-gain parabolic antenna that was attached to the center section of the satellite body by a long arm. The satellite was triaxially stabilized by a series of inertial flywheels, driven by electric motors, whose kinetic energy was dampened by torques produced by electromagnets interacting with the Earth's magnetic field.
Kosmos 122 was oriented by Earth sensors with one of its axes directed Earthward along the local vertical, a second oriented along the orbital velocity vector, and a third oriented perpendicular to the orbital plane. This orientation ensured that the optical axes of the instruments were constantly directed Earthward.
Instruments
The instrumentation consisted of two vidicon cameras for daytime cloud cover pictures, a high-resolution scanning infrared radiometer for nighttime and daytime imaging of the Earth and clouds, and an array of narrow-angle and wide-angle radiometers for measuring the intensity of radiation reflected from the clouds and oceans, the surface temperatures of the Earth and cloud tops, and the total flux of thermal energy from the Earth-atmosphere system into space, respectively. The experiment terminated operations in October 1966.| Instrument | Number of spectral bands | Band wavelengths | Ground swath | Ground resolution |
| TV optical instrument MR-600 | 1 | 0.5–0.7 | 1000 | 1.25 x 1.25 |
| TV infrared instrument Lastocha | 1 | 8–12 | 1100 | 15 x 15 |
| Actinometric instrument | 3 | 0.3–12 | 2500 | 50 x 50 |
Dual vidicon cameras
The Kosmos 122 dual vidicon camera experiment was designed to test the capability of Russian weather satellites to provide daytime pictures of the Earth's cloud cover distribution, local storms, and global weather systems for use by the Soviet Hydrometeorological Service. The instrumentation consisted of two identical vidicon cameras that were mounted in the satellite base and were directed toward the Earth. Each camera viewed a by area – one to the left and the other to the right of nadir – with a resolution of at nadir from a satellite altitude of to. The cameras took a one-frame image of the Earth's cloud cover with slight overlapping of successive frames to provide continuous coverage. The cameras switched on automatically any time the sun was more than 5° above the horizon. Because the Earth illumination varied so much, automatic sensors adjusted the camera apertures to produce high-quality pictures under a variety of illumination conditions. The image formed by each vidicon tube either was transmitted directly to the ground if the satellite was in radio contact with one of two ground stations or was recorded on magnetic tape for later transmission if the satellite was beyond the zone of radio communication.The TV images received by these ground stations were processed and transmitted to the Hydrometeorological Center in Moscow, where they were analyzed and used in various forecast and analysis products. The pictures were archived at the Hydrometeorological Center. The Kosmos 122 cameras, although having 2.5 times the resolution of those carried on the ESSA satellites, could not provide continuous overlapping global coverage as do the ESSA cameras owing to the lower orbit of the Kosmos 122 satellite. Thus, to close the gaps in coverage, at least two satellites were required in the weather satellite system. In addition, cloud cover mosaics were produced from 10 or more individual cloud cover pictures at the Hydrometeorological Center to provide a more comprehensive view of global weather systems.
Some of the individual pictures and the cloud mosaics were transmitted to various foreign meteorological centers as part of an international meteorological data exchange program. The United States received some of these pictures at the National Environmental Satellite Service in Suitland, Maryland, via the "cold line" facsimile link with Moscow. Pictures were transmitted to NESS from September 11, 1966, through October 26, 1966. These pictures were archived at NESS for 1 yr and then, unless of unusual interest, were discarded.
Scanning high-resolution infrared radiometer
The high-resolution scanning infrared radiometer was designed to make measurements of cloud distribution and snow and ice cover on the dayside and nightside of the Earth. The radiometer measured the outgoing radiation from the Earth-atmosphere system in the 8 to 12 μm atmospheric window. Measurements made in this spectral region permitted the construction of brightness patterns of the thermal relief and determination of equivalent radiation temperatures of the Earth's surface and cloud tops. The instrument was a narrow-angle scanning radiometer with an instantaneous viewing angle of 1.5 x 1.5°. It was mounted in the base of the satellite in a sealed instrument compartment with its optical axis directed along the local vertical and toward nadir. The radiometer measured the intensity of the outgoing radiation by comparing the Earth's radiation flux with the radiation flux from space. Each type of radiation entered the radiometer through separate windows, which were oriented in mutually perpendicular directions. The radiation from the Earth-atmosphere system fell on a plane scanning mirror that was mounted at an angle of 45° to the satellite velocity vector and scanned through an angle of ± 50° from nadir.The radiation was reflected from the scanning mirror through a stationary modulating disk and filter window onto a parabolic mirror that focused the parallel beam through a movable modulating disk onto a thermistor bolometer. The stationary and movable modulating disks provided the channel switching, sending first the Earth-atmosphere radiation and then the space radiation to the parabolic mirror and finally to the bolometer. The bolometer converted the radiant flux into variable electric voltages whose frequency was equal to the modulator frequency and whose magnitudes were proportional to the differences in the radiant flux intensities between Earth and space developed at the bolometer output. During the movement of the scanning mirror through a ± 40° sector, line scanning of the target area was accomplished in a plane normal to the orbital plane using a forward and back path, while scanning along the flight path was provided by the relative motion of the satellite with respect to the Earth. In each scan, with the indicated viewing and scanning angles from the satellite's orbital altitude, the radiometer recorded the mean radiation intensities from a band about wide with a resolution of about at nadir to about to at the edges. The radiometer was capable of measuring radiation temperatures within 2 to 3° for temperatures above 273 K and within 7 to 8° for temperatures below 273 K.
The video signals were amplified and sent either to the satellite memory unit for later transmission or to the radiotelemetry unit for direct transmission to Earth, depending on whether the satellite was beyond or within the zone of radio communication with a ground receiving station, respectively. The ground receivers recorded the transmitted data in digital form on magnetic tape and simultaneously on 80-mm photographic film in the form of a brightness image of the thermal relief of the Earth-atmosphere system. The data on magnetic tape was processed by computer at the Soviet Hydrometeorological Center and was used to produce a digital map of the equivalent radiation temperature field with a superposed geographic grid. The photographic film was developed and processed into an IR picture also with a superposed grid. The pictures were archived at the Hydrometeorological Center. Some of these pictures were transmitted to various foreign meteorological centers as part of an international meteorological data exchange program. The United States received these pictures at the National Environmental Satellite Service, Suitland, Maryland, via the "cold line" facsimile link with Moscow. Pictures were transmitted to NESS from mid-September until late October 1966. These IR pictures were kept at NESS for 1 yr and then, unless of unusual interest, were discarded.