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111.
The structure of the mid- and high-latitude ionosphere during the November 2004 storm event obtained from GPS observations 总被引:1,自引:1,他引:1
Andrzej Krankowski Irk I. Shagimuratov Lubomir W. Baran Galina Yakimova 《Acta Geophysica》2007,55(4):490-508
GPS data from the International GNSS Service (IGS) network were used to study the development of the severe geomagnetic storm
of November 7–12, 2004, in the total electron content (TEC) on a global scale. The TEC maps were produced for analyzing the
storm. For producing the maps over European and North American sectors, GPS measurements from more than 100 stations were
used. The dense network of GPS stations provided TEC measurements with a high temporal and spatial resolution. To present
the temporal and spatial variation of TEC during the storm, differential TEC maps relative to a quiet day (November 6, 2004)
were created.
The features of geomagnetic storm attributed to the complex development of ionospheric storm depend on latitude, longitude
and local time. The positive, as well as negative effects were detected in TEC variations as a consequence of the evolution
of the geomagnetic storm. The maximal effect was registered in the subauroral/auroral ionosphere during substorm activity
in the evening and night period. The latitudinal profiles obtained from TEC maps for Europe gave rise to the storm-time dynamic
of the ionospheric trough, which was detected on November 7 and 9 at latitudes below 50°N. In the report, features of the
response of TEC to the storm for European and North American sectors are analyzed. 相似文献
112.
113.
A numerical model is proposed to describe the formation of ice jams under the effect of a release wave. 相似文献
114.
Maximum extent of the Eurasian ice sheets in the Barents and Kara Sea region during the Weichselian 总被引:1,自引:0,他引:1
JOHN INGE SVENDSEN VALERY I. ASTAKHOV DMITRI YU. BOLSHIYANOV IGOR DEMIDOV JULIAN A. DOWDESWELL VALERY GATAULLIN CHRISTIAN HJORT HANS W. HUBBERTEN EILIV LARSEN JAN MANGERUD MARTIN MELLES PER MÖLLER MATTI SAARNISTO MARTIN J. SIEGERT 《Boreas: An International Journal of Quaternary Research》1999,28(1):234-242
Based on field investigations in northern Russia and interpretation of offshore seismic data, we have made a preliminary reconstruction of the maximum ice-sheet extent in the Barents and Kara Sea region during the Early/Middle Weichselian and the Late Weichselian. Our investigations indicate that the Barents and Kara ice sheets attained their maximum Weichselian positions in northern Russia prior to 50 000 yr BP, whereas the northeastern flank of the Scandinavian Ice Sheet advanced to a maximum position shortly after 17 000 calendar years ago. During the Late Weichselian (25 000-10 000 yr BP), much of the Russian Arctic remained ice-free. According to our reconstruction, the extent of the ice sheets in the Barents and Kara Sea region during the Late Weichselian glacial maximum was less than half that of the maximum model which, up to now, has been widely used as a boundary condition for testing and refining General Circulation Models (GCMs). Preliminary numerical-modelling experiments predict Late Weichselian ice sheets which are larger than the ice extent implied for the Kara Sea region from dated geological evidence, suggesting very low precipitation. 相似文献
115.
We performed polarization observations of giant radio pulses from the millisecond pulsar B1937+21. The observations were carried out in July 2002 with the 64-m Kalyazin radio telescope at a frequency of 600 MHz in two polarization channels with left-and right-hand circular polarizations (RCP and LCP). We used the S2 data acquisition system with a time resolution of 125 ns. The duration of an observing session was 20 min. We detected twelve giant radio pulses with peak flux densities higher than 1000 Jy; five and seven of these pulses appeared in the RCP and LCP channels, respectively. We found no event that exceeded the established detection threshold simultaneously in the two polarization channels. Thus, we may conclude that the detected giant pulses have a high degree of circular polarization, with the frequency of occurrence of RCP and LCP pulses being the same. 相似文献
116.
S. A. Medina-Moreno Ph.D. D. Jiménez-Islas Ph.D. J. N. Gracida-Rodríguez Ph.D. M. Gutiérrez-Rojas I. J. Díaz-Ramírez Ph.D. 《International Journal of Environmental Science and Technology》2011,8(3):471-482
A mathematical model to predict the rhamnolipids production by Pseudomonas aeruginosa from oleic acid in a two phase liquid-liquid batch reaction system, was developed in this study. The model was based on two theoretical assumptions: 1) the convective oleic acid mass transfer is coupled to a bioreaction in the aqueous liquid bulk, and 2) the volume of the immiscible oleic acid drops and the saturation concentration at the interface are a function of rhamnolipids production. The model was able to accurately predict the experimental growth of the Pseudomonas aeruginosa strain, and the rhamnolipids production data with oleic acid as carbon source. This mathematical approach indicated a high correspondence between the saturation dimensionless profiles of oleic acid at the interface and the experimental profiles of surface tension difference. This modeling approach may constitute a useful tool in the design and scaling-up of bioreactors applied to the production of biosurfactants with immiscible carbon sources. 相似文献
117.
A mudcake formed on the borehole wall between a fluid-filled porous formation and the borehole fluid can affect Stoneley wave propagation used to estimate the formation permeability. The mudcake effect on the permeability dependence of radial oscillations of borehole fluid is investigated in a system with a source generating radial acoustic waves in the borehole and hydrophones (pressure sensors) that record the respective attenuating oscillations of the borehole fluid. The permeability of the porous formation is estimated from theoretical permeability dependence of the attenuation exponent, knowing the time dependence of the exponential attenuation of borehole fluid oscillations. 相似文献
118.
贵州大方煤田主采煤层的矿物学异常及其对元素地球化学的影响 总被引:19,自引:0,他引:19
运用电感耦合等离子体质谱(ICP-MS)、X射线荧光光谱(XRF)、带能谱仪的扫描电镜(SEM-EDX)、逐级化学提取(SCEP)和光学显微镜等方法,对贵州大方煤田11号煤层的地球化学和矿物学进行了研究。结果表明,大方煤田11号煤层中有高含量的脉状石英(11.4%)和脉状铁白云石(10.2%),铁白云石周边常被针铁矿所包裹,在脉状石英中发现有热液成因的黄铜矿、闪锌矿和硒方铅矿,此外,还有少量高岭石充填在脉中,这7种矿物常常同脉共存。脉状石英和脉状铁白云石分别来源于硅质和富铁的钙质低温热液流体,形成温度分别为180℃和85℃。脉状石英早于脉状铁白云石形成。根据Ca/Sr和Fe/Mn值,确定出铁白云石的形成至少经历了3个时期。这7种矿物按照从早到晚的生成顺序为硫化物、石英、高岭石、铁白云石和针铁矿。铁白云石是煤中Mn、Cu、Ni、Pb和Zn富集的主要原因,这5种微量元素的含量分别为0.09%、74.0μg/g、33.6μg/g、185μg/g和289μg/g。脉状石英是煤中铂族元素Pd、Pt和Ir的主要载体,它们在煤中的含量分别为1.57μg/g、0.15μg/g和0.007μg/g。另外,黄铜矿、闪锌矿和硒方铅矿亦是11号煤层中Cu、Zn和Pb的重要载体。 相似文献
119.
Our investigation has been carried using the instruments onboard the Solar Dynamics Observatory (SDO) providing a high resolution of images (AIA photographs and HMI magnetograms). We have investigated the structure and magnetic evolution of several coronal bright points and small scale N-S polarity magnetic fluxes closely associated with them. We also compare the evolution of the magnetic polarities of elementary isolated sources of positive and negative fluxes (magnetic bipoles) and coronal bright points. Tiny (“elementary”) coronal bright points have been detected. A standard coronal bright point is shown to be a group of “elementary” coronal bright points that flare up sequentially. Our investigation shows that a change in the magnetic fluxes of opposite polarities is observed before the flare of a coronal bright point. We show that not all cases of the formation of coronal bright points are described by the magnetic reconnection model. This result has not been considered previously and has not been pointed out by other authors. 相似文献
120.
P. F. Svistov N. A. Pershina M. T. Pavlova A. I. Polishchuk E. S. Semenets 《Russian Meteorology and Hydrology》2017,42(5):314-318
The results of observations of the chemical composition of precipitation in the Russian Arctic in 2007-2015 are summarized including the data from NP-35 drifting ice station obtained in 2007-2008 in the framework of the joint program of Arctic and Antarctic Research Institute and Voeikov Main Geophysical Observatory. The qualitative and quantitative difference in the chemical composition of precipitation in the Atlantic, Siberian, and Pacific sectors of the Russian Arctic is revealed. It is found that the concentration of microelements (heavy metals) in precipitation at NP-35 ice station did not exceed 12% of total ions at the lowest mineralization. The comparative analysis is presented of the concentration of sulfate ions in precipitation in Norilsk and at NP-35 ice stations. 相似文献