Titlebook: Radiation Trapped in the Earth’s Magnetic Field; Proceedings of the A Billy M. McCormac Conference proceedings 1966 D. Reidel Publishing Co

煩憂

Models of the Earth’s Magnetic Fielda dipole approximation to the main field. However, as our knowledge of the field and particle fluctuations extends outward from the earth to the magnetospheric boundary and into the antisolar tail regions, even the theoretical workers will require a better model than that of the extrapolated dipole.

鎮(zhèn)壓

predict

Some Cosmic Ray and Radiation Belt Observations Based on Data from the Anton 302 G-M Counter in Ariesponding threshold for protons is ~ 50 MeV. The counter also responds, but with low efficiency of course, to bremsstrahlung from electrons stopping in the shielding material and to y-rays. In the latter case the efficiency is about 0.4%. The product of counter efficiency for charged particles and the omnidirectional geometrical factor is ~0.5 cm..

Medicare

Ejaculate

Adiabatic Theory of Charged Particle MotionThis method is limited to first order effects in the radius of gyration, since higher order effects become difficult to visualize and one’s intuition becomes unreliable as a guide. Second, the formal theory of KRUSKAL (1962) will be reviewed and some results obtained with it described. This and othe

Factorable

Transfusion

罐里有戒指

抗生素

Low Altitude Measurements of Trapped Electronsradiation belts. For example, by comparing theoretical calculations with the measured decay of electrons injected by the Starfish detonation of July 1962, it has been shown that the loss of electrons trapped on field lines below L ≈1.3 is dominated by atmospheric scattering (WALT and MACDONALD, 1964

CHAFE