Multi-instrument ground-based observations of a travelling convection vortices event     

H. Lühr  M. Lockwood  P. E. Sandholt  T. L. Hansen  T. Moretto 《Annales Geophysicae》1996,14(2):162-181

A coordinated ground-based observational campaign using the IMAGE magnetometer network, EISCAT radars and optical instruments on Svalbard has made possible detailed studies of a travelling convection vortices (TCV) event on 6 January 1992. Combining the data from these facilities allows us to draw a very detailed picture of the features and dynamics of this TCV event. On the way from the noon to the drawn meridian, the vortices went through a remarkable development. The propagation velocity in the ionosphere increased from 2.5 to 7.4 km s⁻¹, and the orientation of the major axes of the vortices rotated from being almost parallel to the magnetic meridian near noon to essentially perpendicular at dawn. By combining electric fields obtained by EISCAT and ionospheric currents deduced from magnetic field recordings, conductivities associated with the vortices could be estimated. Contrary to expectations we found higher conductivities below the downward field aligned current (FAC) filament than below the upward directed. Unexpected results also emerged from the optical observations. For most of the time there were no discrete aurora at 557.7 nm associated with the TCVs. Only once did a discrete form appear at the foot of the upward FAC. This aurora subsequently expanded eastward and westward leaving its centre at the same longitude while the TCV continued to travel westward. Also we try to identify the source regions of TCVs in the magnetosphere and discuss possible generation mechanisms.  相似文献   

Die atlantischen Ankerstationen des „Armauer Hansen“ im Jahre 1930 in der Bearbeitung von V. W. Ekman     

Walter Hansen 《Ocean Dynamics》1954,7(1-2):55-58

Summary The main subject of Ekman's most careful and detailed analysis of the current measurements of Armauer Hansen is to elucidate the periodical character of ocean currents. A survey of his results is given in table 2 and by means of an outline chartlet a comparison is made between the values which are derived from the observations on board Armauer Hansen and those attained by the reviewer by numerical calculation.

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Les observations faites à bord du navire Armauer Hansen en 1930 à ses mouillages dans l'Atlantique et leur exploitation par V. W. Ekman

Résumé Le but principal de V. W. Ekman dans son analyse scrupuleuse et détaillée des mesures de courant est d'élucider le caractère periodique des courants océaniques. Les résultats les plus importants en sont donnés dans la table 2; en outre le rapporteur compare ces résultats empiriques d'Ekman avec ses propres calculs numériques en les confrontant dans une petite carte.

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V. W. Ekmann, Studies on Ocean Currents. Geofysiske Publikasjoner Vol. XIX, No. 1, Bergen 1953.  相似文献   

Some weak interaction processes in highly evolved stars     

Carl J. Hansen 《Astrophysics and Space Science》1968,1(4):499-512

Some weak interaction processes which are important in stars whose central temperatures and densities exceed 10^9°K and 10⁶ gm/cm³ are discussed. Simple analytic expressions for reaction rates which are convenient for computer studies of the late stages of stellar evolution are given.Of the National Bureau of Standards and University of Colorado.  相似文献   

Solar-cycle dependence of galactic cosmic ray flux     

G. D. Parker  R. L. Chasson  R. T. Hansen  S. F. Hansen 《Solar physics》1976,48(2):399-410

To investigate the relationship between solar activity and cosmic ray modulation, time series of the nucleonic flux and of solar plages, sunspots, centimeter radio noise, and the brightness of the white light corona at 1.1 and 1.5 solar radii from the center of Sun are cross-correlated. Data pertain to the years 1964–1967 during the ascending phase of the current solar cycle. The amplitudes and phases of correlation functions for filtered and unfiltered indices are discussed. The existence of a superior solar index for relating solar activity to long-term modulation is not yet demonstrated conclusively, and the time lag of modulation is too poorly determined to permit its use in estimating the radius of the modulation region.Presently at the Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona 85721.The National Center for Atmospheric Research is sponsored by the National Science Foundation.  相似文献   

Relations between electric fields,currents, and plasma in the polar magnetosphere-ionosphere system     

A. Bahnsen  A.M. Hansen 《Planetary and Space Science》1976,24(9):841-848

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Thermonuclear detonations in collapsing white dwarf stars     

J. Craig Wheeler  Carl J. Hansen 《Astrophysics and Space Science》1971,11(3):373-397

Collapsing white dwarf stars (or degenerate cores) may occur in binary systems, in the formation of Type I supernovae or in the formation of pulsars. These collapsing configurations may explode their nuclear fuel (¹²C or¹⁶O) by the detonation wave mechanism. A combination of analytical and numerical models is used to investigate the formation of detonation waves. The tentative conclusion is that a detonation wave will form which will lead to the ignition of esentially all the fuel in such a collapsing star. This potentially explosive configuration will be strongly affected, however, by rapid beta processes which occur in the detonated matter and which should cause a fraction of the stellar mass to collapse toward a neutron star state. The nature and effect of such beta processes, which have not yet been incorporated in the dynamical calculations, are discussed.An appendix gives approximate expressions for the pressureP(,T) and the internal energy densityU(,T) for a degenerate relativistic electron gas and an analysis of the errors expected in making such approximations to the standard parametric form of the equation of state. These expressions are useful in analyzing shock waves in a degenerate electron gas.Supported in part by the National Science Foundation [GP-15911, GP-9114, GP-19887] and the Office of Naval Research [Nonr-220 (47)] at the California Institute of Technology, and National Science Foundation Grant GP-12455 at the University of Colorado.  相似文献   

A candidate of the Induan-Olenekian boundary stratotype in the Tethyan region   总被引：10，自引：0，他引：10  

童金南  Yuri D.Zakharov  殷鸿福  Hans J.Hansen 《中国科学D辑(英文版)》2003,46(11):1182-1200

The Olenekian Stage was proposed by Kiparisova and Popov[1] based on the type section along the lower reaches of the Olenek River, Siberia. Later research showed that this section con-tains only the Olenikites spiniplicatus Zone of the Upper Olenekian Sta…  相似文献   

Facies characteristics, morphology and depositional models of clay-slide deposits in terraced fjord valleys, Norway     

Louise Hansen  Raymond S. Eilertsen  Harald Sveian 《Sedimentary Geology》2007,202(4):710-729

Many bedrock-confined fjord valleys along the Norwegian coast contain thick accumulations of fine-grained sediments that were deposited during and after the last deglaciation. The deposits gradually emerged above sea level due to glacioisostatic uplift, and fjord marine sedimentation was gradually followed by shallow marine and fluvial processes. During emergence terraces and river-cut slopes were formed in the valleys. Subsequent leaching of salt ions from the pore water in the marine deposits by groundwater has led to the development of quick clay. The deposits are subject to river erosion and destructive landslides involving quick clay. Most slides are of prehistoric age. Others are known from modern observations as well as from historic records.Landforms such as distinct slide scars or the hummocky terrain of slide deposits may be strongly modified by secondary processes. In addition, deposits from the most liquid part of quick clay slides may have planar surfaces. Clay-slide deposits on a fluvial or deltaic terrace, therefore, are not always easily recognized from morphology, and only exposures may reveal their internal structures and allow them to be distinguished from overbank flood sediments. Detailed sedimentological work shows that slide deposits in such setting consist of distinct facies containing reworked marine sediments. We propose three facies successions of clay-slide deposits that form a continuum. The dominant components of these succession types are: slightly deformed blocks of laminated clay and silt (A), highly deformed clay and silt with gravel clasts (B) and massive to stratified clay and silt with scattered clasts (C). We suggest that in many cases a basal muddy diamicton is a characteristic, and possibly diagnostic feature. Processes and depositional models are interpreted from the different succession types. The results may be relevant for identifying clay-slide deposits elsewhere and may be useful during general mapping of fjord marine deposits and characterization of slide-prone areas as well as during identification of prehistoric slides.  相似文献   

Stellar forensics — II. Millisecond pulsar binaries     

Brad M. S. Hansen  & Sterl Phinney 《Monthly notices of the Royal Astronomical Society》1998,294(4):569-581

We use the grid of models described in Paper I to analyse those millisecond pulsar binaries whose secondaries have been studied optically. In particular, we find cooling ages for these binary systems that range from < 1 to ∼ 15 Gyr. Comparison of cooling ages and characteristic spin-down ages allows us to constrain the initial spin periods and spin-up histories for individual systems, showing that at least some millisecond pulsars had sub-Eddington accretion rates and long magnetic field decay times.  相似文献   

Quasar redshifts: the intrinsic component     

Peter M. Hansen 《Astrophysics and Space Science》2016,361(9):303

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