Relationship between the direction of the interplanetary magnetic field and steady oscillation conditions

Effect of direction of interplanetary magnetic field on steady oscillation

Determination of the dimensions of the magnetosphere, as measured by the subsolar distance, from the data of terrestrial observations of geomagnetic micropulsations

Geomagnetic micropulsation measurements for magnetosphere and solar wind diagnostic

Pi2-pulsations, aurora oval and plasma density in the magnetosphere

Geomagnetic pulsations Pi2, aurora oval, and plasma density in magnetospher

On the D-wave state component of the deuteron in the Nambu-Jona-Lasinio model of light nuclei

The D-wave state component of the neutron-proton bound state in the deuteron is calculated in the Nambu-Jona-Lasinio model of light nuclei - the relativistically covariant quantum field theoretic approach to the description of low-energy nuclear forces. The theoretical value of the fraction of the D-wave state relative to the S-wave state is equal to eta_d = 0.0238. This agrees well with the phenomenological value eta_d = 0.0256(4) quoted by Kamionkowski and Bahcall (ApJ. 420, 884 (1994)).Comment: 7 pages, latex, no figure

Investigation of type-pi 2 geomagnetic pulsations at magnetoconjugate points

Type pi2 geomagnetic pulsations and Alfven wave resonance on night side of magnetospher