With the MKF-6, terrain sections of around length and width, at a flight altitude of and a resolution of about were recorded. wide un-perforated films with a length of per lens were used, which provided individual images with a Negative format of. An overlay of 20 to 80% of the images was possible for serial recordings. The total weight of the camera including all its control units doesn't exceed. The MKF-6 is equipped with six high-resolutionPinatar 4.5 / 125 mm lenses and a rotary shutter, capable to simultaneously take six photos in six different spectral ranges at an exposure time between and seconds. The color channels range within the wavelengths of 460–500 nm, 520–560 nm, 580–620 nm, 640-680 nm, 700-740 nm and 780–860 nm. Films and filters can be variously combined. Nevertheless, all photos of all lenses have to be free of optical distortions and require an identical image scale regardless of their spectral range. In order to acquire the desired quality, the developers of Carl Zeiss Jena created a completely new lens type. Moreover, the camera moves in the flight's direction during exposure to compensate for the carrier satellite's or spacecraft's orbital movement and speed of approximately, which otherwise causes smearing and blurry images. Manufacture of the lenses was also very complex. Each of the lenses was framed separately and then clamped in a purpose-built lathe. The mounted lenses were centered in such a way that the axis of rotation of the machine and the optical axis of the lenses matched exactly. Thus, the lens frames could be reworked with highest accuracy and then arranged in tubes of precise interior diameter. Parallel to the MKF-6, a multispectral projector, the MSP-4 was developed. With it, several spectral images, on top of each other and under various filters can be projected on a screen or photographic film. The PKA precision copying machine was designed for image reproduction.
Operation
The geoscientificflight test program, developed by the Central Institute for Earth Physics took place aboard Soviet military aircraft. The MKF-6 was first used in September 1976 on board of Soyuz 22. The spacecraft was modified and equipped with a module that accommodated the camera. A completely revised version of the device, the MKF-6M, that could be remotely operated from the ground was introduced in 1978 and deployed at the Salyut programme of Salyut 6 and 7 and the MIR space station. A total of eleven MKF-6 cameras was produced. Beginning in September 1979 it was also installed in utility/agricultural aircraft, such as the Antonov An-2 for terrestrial surveys and recordings.
National significance
For the various research institutes of East Germany, the MKF-6 project represented the first steps towards advanced scientific orbital and airborne remote sensing of the earth's surface, the assessment of water and soil quality, military reconnaissance, environmental and meteorological research, among many other fields. Eventually, as a division of the Interkosmos program of the socialist Comecon countries a department for Remote terrestrial sensing was established. Considered to be the best spectral camera of its time, the development and construction costs of the MKF-6 camera amounted to 82 million East German marks. The MKF-6 is still occasionally being used. Cooperation between the Soviet Union and Carl-Zeiss-Jena for the equipment of satellites and earth terminals began in the mid-1970s. Altogether around 100 devices, developed and produced in East Germany were utilized in space missions of the Interkosmos program and about 150 devices for ground stations.
Advanced scientific research
Achievements and experiences with the MKF-6 were applied to research and data analysis for further missions and the development of new devices. Fourier-transform infrared spectroscopy was developed and used to study the atmosphere of Venus. Device development and research participation in the 1986 Vega program, in which all image data of Halley's Comet was recorded, processed and interpreted. Contributions to the planetary mission Mars 96, with the development of the Wide-Angle Optoelectronic Stereo Scanner. Participation in the 1988/89 Mars lunar Phobos program, which greatly exceeded GDR involvement in the Vega missions. The Central Institute for Cybernetics and Information Processes played a major role in the development of the Fregat Camera Complex. The Phobos mission failed due to premature probe failure as only very little data and images could be acquired, which, however were thoroughly studied and evaluated.