Cosmic ray electrons from 0.2 to 8 MeV - Pioneer 8 and 9 measurements of their spectrum, time variations, and interplanetary radial gradient.
Explore the source record for details and available documents.
Webber, W. R.↗
Engineering topics
Lezniak, J. A.
Publications and source records attributed to Lezniak, J. A..
Evidence for differences in the energy spectra of cosmic ray nuclei.
Comparison of the intensities of He, C + O, and Fe + Ni cosmic ray nuclei as measured on balloon flights in Canada and Argentina at several energy levels between about 1 and 50 GeV per nucleon. A re-analysis of previous data and those of Juliusson et al. (1972) and Smith et al. (in the press) is carried out. The differences in the spectra of these nuclei are discussed.
Webber, W. R.↗
Evidence for the existence of adiabatic energy loss in interplanetary space from observations of the decay of the February 25-March 2, 1969 series of solar cosmic ray events.
Explore the source record for details and available documents.
Lezniak, J. A.↗
Change in the eleven-year modulation at the time of the June 8, 1969, Forbush decrease.
The functional form of the modulation for the 11-year variation changed abruptly after the Forbush decrease of June 8, 1969. This change in the 11-year modulation suggests that this Forbush decrease was an integral part of the 11-year variation. Some details of the change as observed by neutron monitors and by spacecraft at low energies are discussed.
Lockwood, J. A.↗
Intensities of low-energy cosmic-ray H 2 and He 3 nuclei measured in 1967-1968
Low energy cosmic ray H 2 and He 3 nuclei intensities /1967-1968/ from Pioneer 8 and IMP 4 measurements
Baity, W. H.↗
Solar modulation of cosmic ray protons, helium nuclei, and electrons - A comparison of experiment with theory
Galactic cosmic ray proton and He nuclei spectra measurements aboard Pioneer 8 spacecraft over large energy range, considering solar modulation parameters
Lezniak, J. A.↗
Measurements of the primary electron spectrum in the energy range 0.2 MeV to 15 GeV
Primary interplanetary electron energy spectrum, using Pioneer 8 measurements
Beedle, R. E.↗
The chemical composition and energy spectra of cosmic ray nuclei with Z equals 3 to 30
Cosmic ray nuclei chemical composition and energy spectra in 3-30 Z range by balloon flight and Pioneer 8 space probe, noting propagation models
Lezniak, J. A.↗
Measurements of gradients and anisotropies of cosmic rays in interplanetary space - Pioneer 8
Interplanetary cosmic ray gradients and anisotropies from Pioneer 8 probe
Lezniak, J. A.↗
A comparison of solar modulation effects on protons, electrons and helium nuclei
Galactic cosmic ray proton and He spectrum measurements in 1968 compared to electron spectra, explaining solar modulation features by models incorporating energy loss effects
Lezniak, J. A.↗
Observations on the abundance of nitrogen in the primary cosmic radiation
Primary cosmic ray nitrogen nuclei intensity and spectrum measured by balloons and Pioneer 8 space probe, obtaining abundance difference from solar atmosphere
Lezniak, J. A.↗