A set of satellite experiments for studying the magnetosphere-ionosphere communications

Magnetospheric substorms are one of the basic problems in the physics of near earth space. They appear as magnetic and ionospheric perturbations, disturbances in radio communication, polar auroras and electromagnetic radiation in different frequency ranges. These phenomena were studied from single satellites. However, it is impossible to study these phenomena adequately without simultaneous measurements from at least two different positions with identical instruments. A suitable program can be developed based on the Interkosmos work using new achievements in electronics

Variations of solar wind's ion fluxes during the increase of solar activity level according to the measurement data of ''Venera-2'' and ''Venera-4''

Results of observation of solar wind fluxes near earth obtained by Venera 2 and Venera 4 satellite

The outermost belt of charged particles

Outer radiation belt of low energy charged particle

Method of Determination of Ion Temperature by the Variations of Satellite Induced Ion Trap Currents and Estimate of the Upper Limit of Ion Temperature at Altitudes of 10,000 Kilometers and Higher According to Data of AES Electron-2

Ion temperature determination by variations of satellite induced ion trap currents - Electron 2 satellite measurements of ion temperatures in ionospher

Comparison of Certain Results of Simultaneous Measurements of Solar Wind Characteristics on Spacecrafts ''Venera-3'' and ''Pioneer-6''

Ion concentration, ion velocity, and other solar wind characteristics measured simultaneously aboard spacecraf

Plasma measurements conducted in the vincinity of Venus on the spacecraft VENERA-4

Plasma flux measurements in vicinity of Venus by charged particle traps on Venera-4 spacecraf

The magnetic field of Mars estimated from the data of plasma measurements by Soviet artificial satellites of Mars

The dimensions of the obstacle forming the shock wave of Mars are estimated by use of electron trap data from Mars 2, 3, and 5. The mean altitude of the obstacle at the subsolar point can be convincingly explained if the obstacle is the magnetosphere of Mars. On the assumption that Mars has its own dipole magnetic field, the magnetic moment of Mars is estimated, Mm approximately equal to 2 x 10 to the twenty second power gs x cubic cu

Once More About the Possibility of Determining the Local Electron Concentration by the Dispersion Method with the Help of AES and on New Ionization Maxima in the Ionosphere

Reliability of ionospheric density measurements by satellites using dispersion metho

Estimates of the Upper Limit of Ion Temperature in the 7000-30,000 Km Altitude Range According to Measurements Aboard AES ''elektron-2''

Elektron-2 measurements of upper limits of ion temperatures between 7000 and 30,000 k

Results of experiments for the detection of lunar ionosphere carried out on the first moon's artificial satellite /Luna-10/

Lunik X experiments to detect lunar ionospher