Prognoz 7 Non-refereed Publications


  1. Solar wind helium observations on the Prognoz 7 satellite
    Yermolaev, Y, Solar Wind Eight, 73 (1995)
  2. Large-scale structure of solar wind as observed on the Prognoz 7 satellite
    Yermolaev, Y, Solar Wind Eight, 89 (1995)
  3. Influence of large-scale solar wind disturbances on dynamics of outer radiation belt relativistic electrons
    Bezrodnykh, I, Morozova, Y & Shafer, Y, RpScT, 1, 39 (1987)
  4. Investigations of solar activity and the Prognoz space system
    Sagdeev, R, isap book (1984)
  5. Investigation of the electron component of the solar wind.
    Romanov, S et al., Investigations of Solar Activity and the Prognoz Space System, 67 (1984)
  6. Heavy ion streams in the solar wind and their use for solar corona diagnostics.
    Vaisberg, O et al., Investigations of Solar Activity and the Prognoz Space System, 73 (1984)
  7. Propagation of charged particles in the solar corona
    Pisarenko, N et al., Investigations of Solar Activity and the Prognoz Space System, 131 (1984)
  8. Correlation of X-ray and microwave emission from solar flares according to observations during March-April 1979
    Kocharov, G et al., Prediction of Solar Flares and their Consequences, 45 (1984)
  9. Identification of the coordinates of a transient gamma-ray source with star-catalog coordinates
    Bisnovatyi-Kogan, G et al., Investigation of Gamma-Ray Transients by Means of Unmanned Spacecraft, 62 (1983)
  10. Investigation of gamma-ray transients on Venera 11 and 12 and Prognoz 7
    Vedrenne, G et al., Investigation of Gamma-Ray Transients by Means of Unmanned Spacecraft, 137 (1983)
  11. Peculiarities of propagation of charged particles in the solar corona.
    Klimenko, V et al., IzSSR, 46, 1702 (1982)
  12. Catalogue of Gamma-Bursts Detected by the Soviet-French Experiment Signe 2m VENERA-11 VENERA-12 and PROGNOZ-7
    Diyachkov, A et al., grap, symp, 211 (1982)
  13. Gamma ray burst observations by the 3 Satellite Signe network
    Chambon, G et al., nsgr, symp, 141 (1980)

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