Studies of intensity and spectral composition of lunar gamma-radiation on the automatic station Luna-10
Lunik X scintillation spectrometer studies of lunar gamma radiation intensity and spectral composition
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Lunik X scintillation spectrometer studies of lunar gamma radiation intensity and spectral composition
Interplanetary scintillation observations from solar wind inhomogeneities
Charge and energy spectra of primary cosmic rays made with large area Cerenkov scintillation counter on baloon flights - heavier than iron nuclei
Upper limit on quiet time solar neutron flux at energies above 60 MeV determined by using balloon flights with Cerenkov scintillation counters
Scintillation counters for measuring gamma radiation of tracers in nuclear reactor shielding studies
Gamma scintillation spectrometer design based on electron-positron pair formation
Lithium drifted germanium and silicon semiconducting detectors compared with thallium activated sodium iodide crystal scintillation counter for gamma spectrometry
Spectra of outgoing protons for various targets using scintillation counter, interpreting data by means of impulse-approximation calculation
Measurement of half-life of 14.4 kev level of 57 Fe with scintillation detectors and digital timer
Circuit for discriminating neutrons, gammas and charged particles from each other in phoswich scintillator
Directional neutron spectrometer for events in which neutron is scattered by first scintillator into second
Directional neutron detector using liquid scintillator for low mev energy range for rocket and satellite experiments
Upper limits to hard X-ray flux from quiet sun analyzed by balloon-borne scintillation detector measuring celestial sources
Atmospheric electron energy spectrum in range 70-2000 mev measured, using scintillation telescope with gas Cerenkov detector and lead glass total energy spectrometer
Energetic protons from March 24, 1966 solar flare observed with OGO 1 satellite scintillation counter
Pionic and muonic K-series X-rays studied by liquid He scintillation counter, obtaining separation peaks
We shall perform a series of active satellite tracking experiments to develop atmospheric scintillation mitigation strategies.
The detection of coronal streamers in Doppler scintillation measurements revealed for the first time that variations in radio occultation measurements near the Sun could be caused by quasi-stationary raylike structures.