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Condensation production in comet tail plasma      comet tail plasma  Condensation production       font style='font-size:12px;'> 2009/6/4
Condensation production in comet tail plasma。
Azimuthal field perturbations in the jovian magnetosphere:ulysses observations。
Theoretical investigation of cosmic ray processing of solar system ices     cosmic ray  solar system ices       font style='font-size:12px;'> 2009/5/27
Space ices containing water, carbon- and nitrogen-rich structures are important in certain chemical and radiation induced processes in Solar System dust systems. Up to now there are no detailed invest...
Correct normalization of the Dst index     The Dst index  magnetic storms  ring current       font style='font-size:12px;'> 2009/5/27
The Dst index has been one of the most important solar-terrestrial indices for decades, and it is used in numerous studies as a measure of the temporal development and intensity of magnetic storms and...
We study the propagation of energetic particles, accelerated by interplanetary shock waves, upstream of the shock, considering the possibility of having anomalous transport. The theoretical treatment ...
Precise measurement of irradiance over the earth under various circumstances like solar flares, coronal mass ejections, over an 11-year solar cycle, etc. leads to better understanding of Sun–earth r...
OBSERVATIONS OF THE SUN AND PLANETS WITH THE BELGRADE LARGE MERIDIAN CIRCLE。
BOSE INSTABILITY IN KERR BLACK HOLES     KERR BLACK HOLES  BOSE INSTABILITY       font style='font-size:12px;'> 2009/4/8
Bose instability in rotating (Kerr) black holes (BH’s) consists in exponential increase in time of small perturbations of Bose mass fields, corresponding to superradiative, quasi bound levels. The m...
太阳大气等离子体的电流研究     等离子  太阳大气       font style='font-size:12px;'> 2009/2/20
太阳大气等离子体的电流研究。
太阳表面磁场的分布与演化研究进展     磁场  太阳表面       font style='font-size:12px;'> 2009/2/20
太阳表面磁场的分布与演化研究进展。
PROPAGATION OF HIGH FREQUENCY WAVES IN THE QUIET SOLAR ATMOSPHERE     SUN:oscillations-SUN  atmosphere       font style='font-size:12px;'> 2009/2/5
High-frequency waves (5 mHz to 20 mHz) have previously been suggested as a source of energy accounting for partial heating of the quiet solar atmosphere. The dynamics of previously detected high-fre...

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