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We use the method introduced by Karami & Mohebi (2007), and Karami & Teimoorinia (2007) which enable us to derive the orbital parameters of the spectroscopic binary stars by the nonlinear least squa...
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...
Solar flares are known to release a large amount of energy. It is believed that the flares can excite velocity oscillations in active regions. We report here the changes in velocity signals in three...
We discuss needs in dielectronic recombination data motivated by recent work directed at a quantitative understanding of ion charge states of various elements observed in situ in the solar wind and ...
We apply the ring diagram technique to source regions of halo coronal mass ejections (CMEs) to study changes in acoustic mode parameters before, during, and after the onset of CMEs.We find that CME ...
ANALYSIS OF THE SYSTEMATIC EFFECTS AFFECTING (O-C) DETERMINATION OF THE OUTER PLANETS OBSERVED WITH THE BELGRADE VERTICAL CIRCLE。
AN ANALYSIS OF NINE MOVING-CLUSTERS     MOVING-CLUSTERS  NINE       2009/4/8
AN ANALYSIS OF NINE MOVING-CLUSTERS。
ESTIMATION OF THE SW LAC PARAMETERS BASED ON THE LIGHT-CURVE ANALYSIS
AN ANALYSIS OF THE LIGHT CURVES OF THE CLOSE BINARY ST IND。
We present the analysis of V and R light curves of the late type contact binary V523 Cas for the season of 2006. These observations make part of the monitoring program aimed at studying the long-term ...
Because of poor meteorological conditions, the obtained observational material has not an even distribution in time. Therefore a special method was devised for treating this material. Using this met...
The problem of weights in the task of longitude-network adjustment has not been solved yet because the structure of the observational variances is unknown. During the adjustment of a part of the Eur...
The equivalent width and central depth data of Mn 539.4 nm solar spectral line, observed in the period from 1979 to 1992 at Kitt Peak Observatory, was analyzed in pursuit for periodic changes. As th...
We present the light curve analysis of late-type binary V523 Cas for the season 2005. The spot has been revealed on the secondary. According to theoretical considerations, the spot appeared to be ho...
An analysis of the relation between radio surface brightness and diameter, so-called §¡D relation, for planetary nebulae (PNe) is presented: i) the theoretical § ¡ D relation for the evo...

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