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1.
We prove that rays in linearly elastic anisotropic nonuniform media obey Fermat's principle of stationary traveltime. First, we formulate the concept of rays, which emerges from the Hamilton equations. Then, we show that these rays are solutions of the variational problem stated by Fermat's principle. This proof is valid for all rays except the ones associated with infection points on the phase-slowness surface.  相似文献   
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We present the database of maser sources in H2 O, OH and Si O lines that can be used to identify and study variable stars at evolved stages. Detecting the maser emission in H2 O, OH and Si O molecules toward infrared-excess objects is one of the methods for identifing long-period variables(LPVs, including miras and semiregulars), because these stars exhibit maser activity in their circumstellar shells. Our sample contains 1803 known LPV objects. Forty-six percent of these stars(832 objects) manifest maser emission in the line of at least one molecule: H2 O, OH or Si O. We use the database of circumstellar masers in order to search for LPVs which are not included in the General Catalogue of Variable Stars(GCVS). Our database contains 4806 objects(3866 objects without associations in GCVS) with maser detection in at least one molecule. Therefore it is possible to use the database in order to locate and study the large sample of LPV stars. The database can be accessed at http://maserdb.net.  相似文献   
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Since 2002 the Istituto Nazionale di Oceanografia e di Geofisica Sperimentale (OGS) in Udine (Italy), the Agencija Republike Slovenije za Okolje (ARSO) in Ljubljana (Slovenia) and the Zentralanstalt für Meteorologie und Geodynamik (ZAMG) in Vienna (Austria), are collecting, analyzing, archiving and exchanging seismic data in real time, initially in the framework of the EU Interreg IIIa Italia-Austria project “Trans-national seismological networks in the South-Eastern Alps”. As outcome of the successful cooperation, in the 2013 OGS, ARSO and ZAMG decided to officially merge their seismic monitoring efforts into the “Central and Eastern European Earthquake Research Network—CE3RN”. This work reports the results of a nine-month real-time test of the earthquake early warning (EEW) algorithm probabilistic and evolutionary early warning system carried out at the CE3RN. The study allowed identifying the actions to be implemented in order to let the CE3RN become in the next future an efficient cross-border EEW system.

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Zusammenfassung Orkan und Taifun werden als aus logarithmisch gekrümmten Austauschwalzen aufgehaut betrachtet. Sie bestehen aus doppelten Spiralen, entstanden beim Zusammentreffen zweier Luftströme: der im Zentrum röhrenförmig aufsteigenden tropischen Warmluft und einer zweiten horizontalen Komponente. Einige Merkmale, wie Art der Regenfälle, Art der elektrischen Entladungen, die Wolkenbilder und die Schleppe, passen zu dieser Vorstellung.
Summary Hurricane and typhoon are considered as built up from logarithmically curved exchange cylinders. These bihelices are formed by the confluence of two air-currents: the tropical warm air in shape of a tube rising in the center and a second horizontal component. Some characteristics such as the shape of the rainfalls and of the electrical discharges, the species of clouds and the train are in agreement with this conception.

Résumé Ouragan et typhon sont regardés comme construits par cylindres échangeants — courbées dans un sens logarithmique. Ils se composent d'hélices doubles formées par le confluent de deux courants d'air: de l'air chaud tropical ascendant dans le centre sous forme d'un tube et d'une deuxième composante horizontale. Quelque caractéristiques comme la forme des chutes de pluie et des décharges électriques, les formations des nuages et la traîne sont en bon accord avec ce concept.


Mit 4 Textabbildungen  相似文献   
6.
Dinaric喀斯特的主要特征是各种各样的洼地,包括坡立谷、漏斗、塌陷漏斗及其它类似塌陷漏斗的洼地.这类地形的一些大尺度洼地分布于高喀斯特台地(如斯洛文尼亚的Pokljuka,Jelovica和Sne(z)nik)、喀斯特接触带(如(S)kocjanske溶洞)、坡立谷上的基面(如Imotski坡立谷上的红湖)和大型喀斯特泉群之后(如Malni泉群上的Un(s)ka koli(s)evka漏斗).喀斯特洼地的许多术语都是依据据斯洛文尼亚的地貌定义的.  相似文献   
7.
The broad X-ray iron line observed in many active galactic nuclei spectra is thought to originate from the accretion disc surrounding the putative supermassive black hole. We show here how to perform the analytical integration of the geodesic equations that describe the photon trajectories in the general case of a rotating black hole (Kerr metric), in order to write a fast and efficient numerical code for modelling emission line profiles from accretion discs.  相似文献   
8.
The U.S. Navy is supporting the research to develop and validate stochastic, time-dependent, mine burial prediction models to aid the tactical decision making process. This research requires continuous monitoring of both mine behavior during burial, and the near-field processes responsible for burial. A new instrumented mine has been developed that far exceeds the capabilities of the earlier optically instrumented mine in terms of the burial processes that can be measured. The acoustic-instrumented mine (AIM) utilizes acoustic transducers to measure burial and scour, localized flow rates, and sediment size and concentration in the water column. The AIM also includes sensors for measuring mine orientation and movement, as well as oceanographic information such as significant waveheights, wave period, and water temperature. Four AIMs were constructed and deployed during the Indian Rocks Beach (IRB, FL) and Martha's Vineyard Coastal Observatory (MVCO, Edgartown, MA) mine burial experiments. The results from the field experiments have proven that the sensor suite is viable in providing a wealth of data that are critical in understanding and modeling the complex subsequent burial process.  相似文献   
9.
Our mainly R band photometry of V1493 Aql (1999) during its outburst, indicates periodic variations with a period of 0.156 days, seen only 5 days after the maximum in V. This period can be orbital. The light curve indicates in addition, the presence of a faint eclipse like feature. We try to explain its extremely low amlitude, as being due to the eclipse of an expanded white dwarf component of the binary below an optically thick wind. We discuss what conditions would be required for such an interpretation to work.  相似文献   
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