The successful completion of the first development phase, which confirmed the good prospects of remote sensing techniques for solving scientific and application problems, made it necessary to expand the field of research and design work. OKB-586 established a special division incorporating design-theoretical departments, but the range of problems was so extensive that a single company was not capable to deal with them properly. Therefore, it was decided to transfer several projects to other space enterprises.
To reduce time and cost of spacecraft development and manufacture, it was decided to create the world’s first series of satellite buses comprised of the DS-U1, non-oriented with storage batteries; DS-U2, non-oriented with solar panels; and the Sun-oriented DS-U3.
Forty-nine spacecraft were developed, manufactured, and delivered into orbit in 1963-1976.
The small unified satellite buses became the instrumental basis for establishment of international cooperation in space under the Interkosmos program.
Results of scientific studies into problems of space physics, obtained using the small unified spacecraft, received wide international acclaim.
DS-U1 based spacecraft
The first spacecraft designed by OKB-586 to lay the foundation for further development of spacecraft design field.

DS-U1-G geophysical
|
Mass, kg |
291 |
| Active life, days | 24 |
| Launch vehicle | 11К63 |
| Main experimental results | Valuable information on correlation between solar activity and condition of the atmosphere. A middle-atmosphere model was built. |
| Orbited on |
12 February 1966 |

DS-U1-A astronomical
|
Mass, kg |
302 |
| Active life, days | 30 |
| Launch vehicle | 11К63 |
| Main experimental results | Valuable information on energy distribution in spectra of various stars. Photometric studies of stellar radiation in ultraviolet and X-ray spectral regions. |
| Orbited on |
19 April 1968 |
4.png)
DS-U1-Ya nuclear
|
Mass, kg |
316 |
| Active life, days | 14 |
| Launch vehicle | 11К63 |
| Main experimental results | Valuable information on the level of natural radiation background and radiations in a wide range of energies and intensities in near-Earth space. |
| Orbited on |
12 June 1968 |
DS-U1-P
|
Mass, kg |
315 |
| Active life, days | 30 |
| Launch vehicle | 11К63 |
| Main experimental results | Data on discrete X-radiation sources, on energy distribution in spectra of various stars, and on isotropic X-ray background. |
| Orbited on |
24 April 1970 |
4.png)
DS-U1-IK-1
|
Mass, kg |
288 |
| Active life, days | 30 |
| Launch vehicle | 11К63 |
| Main experimental results |
Data on global distribution of electron temperature and ion concentration. A night equatorial ionospheric anomaly was discovered at an altitude of 1000 km. |
| Orbited on |
25 December 1969 |
DS-U1-IK-2
|
Mass, kg |
287 |
| Active life, days | 30 |
| Launch vehicle | 11К63 |
| Main experimental results |
Data on subauroral ionosphere of the northern and southern hemispheres; on ionospheric electron concentration and temperature and ion concentration; on mechanism of the predawn effect. |
| Orbited on |
14 October 1970 |
DS-U2 based spacecraft
The satellite instrumentation helped to discover and determine a range of large-scale heterogeneous formations in the ionosphere; radio refraction angles were determined.

DS-U2-V vibration
|
Mass, kg |
240 |
| Active life, days | 20 |
| Launch vehicle | 11К63 |
| Main experimental results |
Electron concentration in the vicinity of the spacecraft was defined, as well as properties of the ionosphere in the path of coherent-wave propagation from the spacecraft to an observation point. |
| Orbited on |
19 October 1965 |
6.png)
DS-U2-М molecular
|
Mass, kg |
230 |
| Active life, days | 90 |
| Launch vehicle | 11К63 |
| Main experimental results |
Spacecraft missions experimentally confirmed that quantum frequency standards can work in vacuum, zero gravity, and other space flight environments. The data allowed continuing engineering development of onboard molecular oscillators in order to produce generic designs. |
| Orbited on |
26 November 1965 |
5.png)
DS-U2-I ionospheric
|
Mass, kg |
286 |
| Active life, days | 90 |
| Launch vehicle | 11К63 |
| Main experimental results |
The desired signal was received at all working frequencies: for the first time ever, the passage of 31.8 kHz and 44.9 kHz radio-waves through the ionosphere was confirmed. The hypothesis of the ultralow frequency electromagnetic waves passage through the ionosphere was confirmed. The data allowed estimating charged-particle concentration in lower ionosphere versus time and other factors. |
| Orbited on |
24 May 1966 |
5.png)
DS-U2-D dosimetric
|
Mass, kg |
237 |
| Active life, days | 70 |
| Launch vehicle | 11К63 |
| Main experimental results |
Data on charged particles in Earth natural and artificial radiation belts; data on primary cosmic rays |
| Orbited on |
21 December 1966
|
3.png)
DS-U2-MP meteorite
|
Mass, kg |
280 |
| Active life, days | 90 |
| Launch vehicle | 11К63 |
| Main experimental results |
Data did not confirm a dust belt around Earth and allowed determining the nature of trace elements in a majority of principal meteor showers. A nuclear explosion in China was recorded. |
| Orbited on |
12 December 1966 |
3.png)
DS-U2-GK geophysical integrated
|
Mass, kg |
335 |
| Active life, days | 40 |
| Launch vehicle | 11К63 |
| Main experimental results |
Data on ionospheric plasma motion |
| Orbited on |
20 December 1968 |
2.png)
DS-U2-GF heliophysical
|
Mass, kg |
283 |
| Active life, days | 90 |
| Launch vehicle | 11К63 |
| Main experimental results |
This spacecraft was a small optical observatory with instrumentation for simultaneous recording of solar, stellar, nebula, and Earth upper atmosphere radiation. Instrumentation recordings enabled tracing radiation bursts and decays due to active processes in outer sheaths of the Sun (solar flares). |
| Orbited on |
26 December 1968 |
2.png)
DS-U2-MG magnetic
|
Mass, kg |
265 |
| Active life, days | 40 |
| Launch vehicle | 11К63 |
| Main experimental results |
Data on Earth’s magnetic field behavior. The equatorial electrojet effect was measured for the first time. These data are used for studying the globe conductivity. Experiments in space allowed determining the degree of conformity of a true picture with theoretical models created on the basis of observations conducted for centuries from the Earth surface. |
| Orbited on |
20 January 1970 |
1.png)
DS-U2-IP ionospheric
|
Mass, kg |
281 |
| Active life, days | 90 |
| Launch vehicle | 11K65М |
| Main experimental results |
The spacecraft studied ion and electron concentrations, ion chemical composition, and absorption of solar ultraviolet radiation in the atmosphere. Energetic-particle fluxes, related to the outer radiation belt and the “soft”-electron flow, were measured. |
| Orbited on |
17 November 1970 |
1.png)
DS-U2-K geophysical
|
Mass, kg |
298 |
| Active life, days | 90 |
| Launch vehicle | 11K65М |
| Main experimental results |
Regular observations of geoactive corpuscles and survey of anisotropic distribution of Earth’s magnetic field were carried out; upper atmosphere structure parameters were measured; global distribution of corpuscular fluxes was studied, and a relationship between the corpuscular flux intensity and the aurora luminosity was established. |
| Orbited on |
4 June 1971 |
1.png)
DS-U2-MT meteorite
|
Mass, kg |
330 |
| Active life, days | 40 |
| Launch vehicle | 11K63 |
| Main experimental results |
Low-energy and high-energy component intensity variations of charged-particle flows were measured; radiation intensity and spectral composition were studied over a wide range, from X-ray to hard gamma radiation; radiation variations and a correlation with the activity of principal meteor showers was studied. |
| Orbited on |
2 December 1971 |
.png)
DS-U2-GKA Aureole
|
Mass, kg |
348 |
| Active life, days | 40 |
| Launch vehicle |
11K65М |
| Main experimental results |
New data were obtained about a particular phenomenon, which is hardly visible to the human eye but very important for researchers: the hydrogenous aurora caused by precipitation of energetic protons into the atmosphere. Some characteristics of the precipitation, in particular on the dayside auroral oval, were studied. |
| Orbited on |
27 December 1971 |
.png)
DS-U2-IK-1
|
Mass, kg |
222 |
| Active life, days | 60 |
| Launch vehicle |
11K63 |
| Main experimental results |
Research into natural low-frequency radio waves was conducted. Many and various signals generated by lightning discharges were recorded during the experiment. The interaction of radio waves and ionospheric plasma, which was the source of peculiar space "noises", was observed. The ionospheric plasma "self-excitation" effect was also observed; it was manifested by the plasma emitting natural noise waves of higher intensity. |
| Orbited on |
7 August 1970 |
.png)
DS-U2-IK-2
|
Mass, kg |
296 |
| Active life, days | 60 |
| Launch vehicle |
11K63 |
| Main experimental results |
Studying of charged-particle flows gave additional data on the structure of radiation belts in geomagnetic calm; allowed monitoring the charged particle dynamics under magnetic agitation, and, with data on low frequency electromagnetic radiation, allowed proposing possible mechanisms of charged-particle loss in radiation belts. It was found experimentally that electrons leave ionosphere as a result of cyclotron resonance of particles and low-frequency noise. |
| Orbited on |
2 December 1971 |
.png)
DS-U2-IK-3
|
Mass, kg |
329 |
| Active life, days | 60 |
| Launch vehicle |
11K65M |
| Main experimental results |
The experimental gear gave simultaneous information on ionospheric, magnetic, and electrical field parameter values; on electromagnetic low-frequency radiations and charged-particle flows. Data on electrical field oscillations and low-frequency radiation spectrum, on electron temperature and concentration in ionospheric plasma |
| Orbited on |
30 October 1973 |
.png)
DS-U2-IK-4
|
Mass, kg |
317 |
| Active life, days | 60 |
| Launch vehicle |
11K65M |
| Main experimental results |
Data on electron and positive-ion density, electron temperature and ionic composition of Earth’s ionosphere; on space density, energy characteristics, spectra, mass and destructive effects of sporadic meteoric particles of meteor showers |
| Orbited on |
31 October 1974 |
.png)
DS-U2-IK-5
|
Mass, kg |
320 |
| Active life, days | 60 |
| Launch vehicle |
11K65M |
| Main experimental results |
Data on interaction between charged particles and low-frequency electromagnetic radiation in Earth’s magnetosphere |
| Orbited on |
12 March 1975 |
.png)
DS-U2-IK-6
|
Mass, kg |
312 |
| Active life, days | 60 |
| Launch vehicle |
11K65M |
| Main experimental results |
Data on electrical and magnetic components of low-frequency electromagnetic radiation; allocation of charged-particle concentration and temperature distribution; integrated electron content in ionospheric plasma |
| Orbited on |
11 December 1975 |
.png)
DS-U2-IK-8 Interkosmos-Kopernik-500
|
Mass, kg |
256 |
| Active life, days | 60 |
| Launch vehicle |
11K63 |
| Main experimental results |
Data on sporadic solar radio emission. Irregularity was detected in the structure of solar radio bursts in the 3 to 6 MHz frequency range. Measurement data helped discover a new type of radio noise in ionosphere: Bernstein waves that occur spontaneously in high-temperature magnetic plasma. The most interesting solar observation was the discovery of significant polarization of type III bursts in the 2 to 4 MHz frequency range. |
| Orbited on |
19 April 1973 |
DS-U3 based spacecraft
The DS-U3 spacecraft family specialized in research into short-wave solar radiation that can be observed only above the atmosphere. Solar observations using space technologies allow gaining new knowledge about physical processes inside the Sun.
.png)
DS-U3-S
|
Mass, kg |
285 |
| Active life, days | 75 |
| Launch vehicle |
11K63 |
| Main experimental results |
Data on the hottest areas of the solar corona in X-ray and ultra-violet spectral regions were used to assess the quantity of short-wave solar radiation absorbed by Earth's atmosphere. |
| Orbited on |
16 June 1967 |
.png)
DS-U3-IK-1 (the first spacecraft built with direct participation of scientists and experts from socialist countries under the Interkosmos program)
|
Mass, kg |
303 |
| Active life, days | 60 |
| Launch vehicle |
11K63 |
| Main experimental results |
Discovery of X-ray polarization during solar flares. When the spacecraft was in eclipse, optical and Lyman-alpha photometers determined a "reserve" of molecular oxygen and aerosols in upper atmosphere. |
| Orbited on |
14 October 1969 |
DS-U3-IK-2
|
Mass, kg |
303 |
| Active life, days | 60 |
| Launch vehicle |
11K63 |
| Main experimental results |
A vast store of data on physical processes on the Sun; research into fine X-ray spectra of ions in solar flares. |
| Orbited on |
14 October 1970 |
DS-U3-IK-3
|
Mass, kg |
301 |
| Active life, days | 60 |
| Launch vehicle |
11K63 |
| Main experimental results |
Data on dynamics and X-ray spectrum of energetic proton flares; one-dimensional monochrome X-ray patterns; research into absorption of visible solar radiation by the high-altitude aerosol. Studies of soft and hard solar X-rays. |
| Orbited on |
30 June 1972 |
DS-U3-IK-4
|
Mass, kg |
335 |
| Active life, days | 60 |
| Launch vehicle |
11K65М |
| Main experimental results |
Study of general properties of quiet Sun X-rays. Measurement of absolute radiant flux and its variations in various levels of solar activity; definition of radiation spectral composition; location of active X-ray regions in the solar corona. |
| Orbited on |
17 May 1974 |
DS-U3-IK-5
|
Mass, kg |
305 |
| Active life, days | 60 |
| Launch vehicle |
11K65М |
| Main experimental results |
Data on X-ray and ultraviolet spectra in solar minimum periods. The data are very valuable for studying the mechanism of solar-terrestrial relationship and developing new methods of diagnostics of hot astrophysical and laboratory plasma. |
| Orbited on |
27 July 1976 |

back in history


















