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The problem of solar wind-magnetosphere coupling is investigated for intense geomagnetic storms (Dst γ -100 nT) that occurred during solar cycle 23. For this purpose interplanetary plasma and fie...
A fluxgate digital magnetometer is used to study the variation of magnitude of H component during geomagnetic storm events of April, July and November 2004 at southern subauroral localized region at...
This paper presents the effect of geomagnetic storm on geomagnetic field components at Southern (Maitri) and Northern (Kiruna) Hemispheres. The Indian Antarctic Station Maitri is located at geom. lo...
We study the magnetic and velocity field evolution in the two magnetically complex active regions NOAA 10486 and NOAA 10488 observed during October–November 2003.We have used the available data to ...
Seismic Study of Magnetic Field in the Solar Interior     Sun  oscillations  interior  magnetic field       font style='font-size:12px;'> 2009/5/6
Magnetic field in the solar interior contributes to the even order splitting coefficients, but it is not possible to separate the effect of magnetic field from those due to other deviations from sph...
In this paper, we study the evolution of vector magnetic field of AR 10656 by using the observations of Huairou Solar Observing Station (HSOS, China) and Big Bear Solar Observatory (BBSO, USA). Th...
SOME RESULTS OF SYSTEMATIC OBSERVATIONS OF GEOMAGNETIC FIELD CHANGES IN THE WIDER AREA OF RUDNIK THRUST REGION。
ON THE ORBITAL MOTION OF A BODY IN A SPHERICALLY SYMMETRIC FIELD IN ROSEN'S BIMETRIC GRAVITATION THEORY。
THE ROLE OF GEOMAGNETIC FIELD CONFIGURATION ON THE GPS SIGNAL PATHS THROUGH THE MAGNETOSPHERE AND IONOSPHERE。
UNPERTURBED TRAJECTORIES IN MANEFF’S GRAVITATIONAL FIELD ARE ELLIPSES IN VELOCITY PLANE。
COLLISION AND ESCAPE IN EINSTEIN’S PN FIELD     orbits  near-escape orbits  PN formalism       font style='font-size:12px;'> 2009/3/31
A two-body system is being considered in a PN formalism involving higher powers of variables and mixed terms. The McGehee-type coordinate transformations are used to blow up the collision singularit...
All gasdynamical models for the evolution of gaseous content of galaxies assume that cooling from the hot, virialized phase to the cold phase occured through some sort of thermal instability. Subseq...
The gravitational field effect on atomic data for H and C IV transitions are considered as a perturbation of initial and final energy levels. We found that this perturbation increases with the princ...
We test the prediction of Hamilton and Helfand (1993) that faint radio selected galaxies are a new class contributing to the diffuse X-ray background (XRB) radiation. The test is based on the correl...
Several assumptions used in the recent review paper on the search for extraterrestrial intelligence (SETI) by Duric and Field (2003) are critically dis- cussed. New astrobiological results|in partic...

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