“地球动力学”的研究现状与展望——第32届国际地质大会研究成果综述     

刘少峰  程三友  张会平  苏三 《现代地质》2004,18(4):404-414

第32届国际地质大会通过按地域和构造作用过程等形式划分11个专题会场,展示了地球动力学的研究成果。其成果主要包括特提斯域构造演化及其不同阶段的块体裂解、拼合及后期改造的细节过程,地质历史中的超大陆分布和成因,俯冲—碰撞带深部构造和变质机制,安第斯山(Andes)缓倾角平坦式俯冲过程及其地壳变形和岩浆作用的响应,显微构造对动力作用过程的影响和控制,地壳和上地幔熔融、流变学和动力学意义,大洋岩石圈构造与演化,大陆地盾区构造和再活动,稳定大陆区地震,空间大地测量学和现代板块运动等方面。这些研究成果充分显示了地球动力学研究具有多学科、多手段(如古地磁、超深钻、地球物理、大地测量和GPS等)、多尺度(宏观、微观)和多时期、全面、综合、并逐步接近定时、定位和定量地探索和研究的特点,它从地球(主要为上地幔和地壳)的组成、结构构造入手,逐步认识地球(主要为地球岩石圈)的演化和动力学。  相似文献   

A statistical analysis of methanol maser groups     

I. E. Val’tts  S. Yu. Lyubchenko 《Astronomy Reports》2004,48(10):834-839

An analysis of the flux densities of the 5₁-6₀ A ⁺ (6.7 GHz) and 2₀-3_?1 E (12.2 GHz) class II methanol maser lines in a large and homogeneous sample of maser sources has been carried out. For convenience, the maser lines were divided into three groups: group I contains spectral features for the lines most prominent in the 5₁-6₀ A ⁺ (6.7 GHz) transition, group II contains spectral features for the lines strongest in the 2₀-3_?1 E (12.2 GHz) transition, group III contains spectral features for which the velocities of the emission maxima of the two lines coincide. The same dependence was found for group II and group III: log S _6.7=(0.79±0.05)×log S _12.2+(0.79±0.05). The spectral features in group I do not obey this relation, and deviations from a linear dependence are considerably greater. It is suggested that methanol class II masers be divided into a subclass IIa, which has special conditions favoring 6.7 GHz masers, and a subclass IIb, which is comprised of the 12.2 GHz masers and those 6.7 GHz masers that necessarily accompany them under the same conditions.  相似文献   

Relative variations of the physical parameters of variable extragalactic radio sources     

S. A. Tyul’bashev  P. A. Chernikov 《Astronomy Reports》2004,48(9):716-723

A method for studying the physical conditions in compact components of extragalactic radio sources displaying variability on time scales of hundreds of days is proposed. The method can be used to estimate the relative variations of the magnetic-field strength and number density of relativistic electrons in superluminal jets from the cores of quasars and radio galaxies. Results are presented for the jets of the quasars 3C 120, 3C 273, 3C 279, and 3C 345. The energies of the magnetic field and relativistic particles in these objects are not in equipartition. As a rule, the magnetic-field strength decreases appreciably during the evolution of an expanding jet, while the number of relativistic electrons grows.  相似文献   

Dissipationless disk accretion     

S. V. Bogovalov  S. R. Kel’ner 《Astronomy Reports》2005,49(1):57-70

We consider disk accretion resulting purely from the loss of angular momentum due to the outflow of plasma from a magnetized disk. In this limiting case, the dissipation due to the viscosity and finite electrical conductivity of the plasma can be neglected. We have obtained self-consistent, self-similar solutions for dissipationless disk accretion. Such accretion may result in the formation of objects whose bolometric luminosities are lower than the flux of kinetic energy in the ejected material.  相似文献   

Visual extinction towards the Omega Nebula (M17) and the ionization of nitrogen in the nebula     

Yu. I. Glushkov  V. F. Esipov  L. N. Kondrat’eva 《Astronomy Reports》2005,49(1):36-43

We estimate the absolute intensity of the Hα emission line in M17 based on spectroscopic observations with the 70 cm telescope of the Fesenkov Astrophysical Institute and the 1.25 m telescope of the Sternberg Astronomical Institute’s Crimean Laboratory. The visual extinction, A _v , is derived for about 250 regions in the nebula via a comparison of the optical (Hα) and radio (21 cm continuum) emissions. The A _v values for the eastern, optically bright, part of the nebula are 2–6^m. For the western part, which is covered by a dark cloud, the extinction is A _v = 7?14.5^m. We derived I(Hα)/I([NII] λ6584) ratios and estimated the degree of ionization of nitrogen in the nebula; we find that most nitrogen is in the [NIII] state.  相似文献   

The role of socio-environmental networking in the sustainability of rain-fed agriculture in the coastal savanna of Ghana     

Michael O’Neal Campbell 《GeoJournal》2005,61(1):79-88

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Artificial Beach as a Structure for Protecting a Seacoast from Storm Surge Impact (Based on the Example of the Eastern Gulf of Finland)     

Leont’yev  I. O. 《Oceanology》2019,59(2):267-275

Oceanology - A model of an artificial beach is proposed for protecting a seacoast subjected to erosion under significant storm surge impact. The beach profile properties are based on the Dean...  相似文献   

Thermal anomalies on Savich Cone,Kikhpinych Volcano,Kamchatka: IR surveys and land-based observations for 30 years (1982 through 2012)     

O. F. Kardanova  I. K. Dubrovskaya  Ya. D. Murav’ev 《Journal of Volcanology and Seismology》2015,9(6):368-377

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On the Possibility of Deflecting an Asteroid from Collision with the Earth Using the Kinetic Method     

L. L. Sokolov  N. A. Petrov  A. A. Vasil’ev  G. A. Kuteeva  A. S. Shmyrov  B. B. Eskin 《Solar System Research》2018,52(4):338-346

The possibilities of deflecting an asteroid from its collision course with the Earth by changing its velocity with an impact are considered. Using the asteroid Apophis as an example, the time dependence of the positions and sizes of the keyholes leading to collision is studied. It has been found that the possibility of deflecting this asteroid usually exists, and the impact can be accomplished in principle, given the capabilities of modern space technology. A change in the velocity should be performed before the encounter of 2029 in order to use the gravitational maneuver effect. The possible accuracy of determining Apophis’ orbit and the keyholes that lead to collision and are associated with the resonance returns are considered.  相似文献   

Modeling a Shore Profile Formed by Storm Cycle Impact     

Leont’yev  I. O. 《Oceanology》2018,58(6):892-899

Oceanology - A model is developed for predicting the sand shore profile formed by storm event impact. The model takes into account the cumulative effect of elementary processes responsible for...  相似文献