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  • 1
    Publication Date: 2017-04-04
    Description: The opening of a new magnetic observatory is one of the activities aimed at by the creation of a scientific base at DomeC, Antarctica (lat. 75° 06’S, long. 123° 21’E, elev. 3200m). There are many reasons supporting this objective: all Antarctic magnetic observatories providing absolute values are located along the shore and are therefore subject to coast effects and crustal field contamination. DomeC and Vostok will be so far the sole observatories free from these effects. On one hand, high latitude absolute observatories are very useful to global or regional modeling based upon satellite data, because, at high latitudes, only total field measurements can be used due to the strong influence of field aligned currents. On the other hand, the availability of magnetic data from the well distributed observatories of Terra Nova Bay (TNB), Scott Base (SBA), Dumont d’Urville (DRV), Casey (CSY) and Vostok (VOS) will provide strong support to auroral and polar cap ionosphere studies as well as asymmetry analyses between Northern and Southern hemispheres. This paper summarizes the results gathered during three summer campaigns, in 1999-2000, 2001 and 2003-2004.
    Description: Published
    Description: Kakioka Magnetic Observatory / Tsukuba Center for Institutes, Japan
    Description: 1.6. Osservazioni di geomagnetismo
    Description: 3.4. Geomagnetismo
    Description: open
    Keywords: Antarctica ; Magnetic observatory ; Dome C ; 04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniques
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Conference paper
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  • 2
    Publication Date: 2017-04-04
    Description: The magnetic observatory deployed at DomeC, Antarctica, in the French-Italian base known as Concordia has now been permanently running for more than three years. This paper focuses on these long-term results which are more relevant for an observatory intended to provide absolute values of the field. The problems which emerged in this fairly long record are discussed and solutions suggested to upgrade the observatory to the standards of an absolute one (i.e. Intermagnet standards).
    Description: Published
    Description: 15-26
    Description: 1.6. Osservazioni di geomagnetismo
    Description: 3.4. Geomagnetismo
    Description: JCR Journal
    Description: open
    Keywords: Antarctica ; Dome C ; magnetic observatory ; continuos records ; 04. Solid Earth::04.05. Geomagnetism::04.05.03. Global and regional models ; 04. Solid Earth::04.05. Geomagnetism::04.05.05. Main geomagnetic field ; 04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniques
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 3
    Publication Date: 2017-04-04
    Description: The magnetic observatory deployed at DomeC, Antarctica, in the French-Italian base known as Concordia base, is now permanently running for more than three years. This paper focuses on these long-term results which are more relevant for an observatory intended to provide absolute values of the field. The problems which came up in the light of this fairly long record are discussed and solutions suggested in order to upgrade the observatory to the standards of an absolute one (i.e. Intermagnet standards).
    Description: Submitted
    Description: 1.6. Osservazioni di geomagnetismo
    Description: 3.4. Geomagnetismo
    Description: 3.9. Fisica della magnetosfera, ionosfera e meteorologia spaziale
    Description: JCR Journal
    Description: open
    Keywords: Geomagnetic observatory ; Antarctica ; 04. Solid Earth::04.05. Geomagnetism::04.05.03. Global and regional models ; 04. Solid Earth::04.05. Geomagnetism::04.05.04. Magnetic anomalies ; 04. Solid Earth::04.05. Geomagnetism::04.05.05. Main geomagnetic field
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: manuscript
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  • 4
    Publication Date: 2017-04-04
    Description: We conduct an analysis of the geomagnetic field variations recorded at the new Antarctic station Dome C, located very close to the geomagnetic pole, which has been operating for approximately one month during the 1999–2000 campaign. We also perform a comparison with simultaneous measurements at the Italian Antarctic station Terra Nova Bay, in order to investigate the spatial extension of the phenomena observed at very high latitude. Our results show that between the two stations the daily variation is similar and the fluctuations with f 1 mHz are coherent, provided that in both cases the comparison is made between geographically oriented components, suggesting that ionospheric currents related to the geographic position, more than field-aligned currents, are responsible for the lowest frequency variations; conversely, higher frequency (Pc5) fluctuations are substantially decoupled between the two stations. We also found that at Dome C the fluctuation power in the 0.55–6.7 mHz frequency band is well related with the solar wind speed during the whole day and that at Terra Nova Bay the correlation is also high, except around local geomagnetic noon, when the station approaches the polar cusp. These results indicate that the solar wind speed control of the geomagnetic field fluctuation power is very strict in the polar cap and less important close to the polar cusp.
    Description: Published
    Description: 923-932
    Description: 1.6. Osservazioni di geomagnetismo
    Description: 3.4. Geomagnetismo
    Description: 3.9. Fisica della magnetosfera, ionosfera e meteorologia spaziale
    Description: JCR Journal
    Description: reserved
    Keywords: Magnetospheric physics ; MHD waves and instabilities ; Polar cap phenomena ; Solar wind-magnetosphere interactions ; 01. Atmosphere::01.03. Magnetosphere::01.03.03. Magnetospheric physics
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 5
    Publication Date: 2017-04-04
    Description: During the 1986-87 austral summer a geomagnetic observatory was installed at the Italian Antarctic Base Mario Zucchelli Station (TNB, geographic coordinates:74.7S, 164.1E; corrected geomagnetic coordinates: 80.0S, 307.7E; magnetic local time MLT=UT-8). In the first years the measurements of the geomagnetic field were carried out only during summer expeditions. Since 1991 the recording was implemented with an automatic acquisition system operating through the year. More recently,after two short test surveys, from October 2004 a geomagnetic French-Italian observatory was installed on the Antarctic plateau (Dome C, DMC), very close to the geomagnetic pole (geographic coordinates: 75.1S, 123.4E; corrected geomagnetic coordinates:88.8S, 55.6E; magnetic local time MLT=UT-1). In this work we present some results obtained from TNB observations coming from almost twenty years of observations and also the preliminary results obtained from the analysis of the first year of data from DMC.
    Description: Unpublished
    Description: Vienna, Austria
    Description: open
    Keywords: antartica ; Geomagnetic field ; 04. Solid Earth::04.05. Geomagnetism::04.05.05. Main geomagnetic field
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Poster session
    Format: 10469599 bytes
    Format: application/pdf
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  • 6
    Publication Date: 2017-04-04
    Description: After some short test surveys, during the 2004–2005 summer expedition in Antarctica, a geomagnetic French-Italian observatory was installed on the plateau (geographic coordinates: 75.1 S, 123.4 E; corrected geomagnetic coordinates: 88.9 S, 54.3 E; UT=LT−8) very close to the geomagnetic pole. In this paper we present some peculiarities of the daily variation as observed at this polar cap observatory during the years 2005 and 2006, taking into account the different Loyd seasons and different interplanetary magnetic field conditions. Some interesting results emerge from the analysis, confirming the dependence of the daily variation (and of the associated polar current systems) on the IMF Bz and By components. In particular the analysis showed that different Bz conditions correspond to different contribution to daily variation of ionospheric and field aligned currents, while particular By conditions lead to a time shift of the diurnal variation, indicating an asymmetry with respect to the noon meridian.
    Description: Published
    Description: 2045–2051
    Description: 3.9. Fisica della magnetosfera, ionosfera e meteorologia spaziale
    Description: 1.6. Osservazioni di geomagnetismo
    Description: JCR Journal
    Description: reserved
    Keywords: Geomagnetism and paleomagnetism (Time variations, diurnal to secular) ; Magnetospheric physics (Polar cap phenomena; Solar wind-magnetosphere interactions) ; 01. Atmosphere::01.03. Magnetosphere::01.03.99. General or miscellaneous
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 7
    Publication Date: 2019-07-17
    Description: The main objective was to assess the influence of the seasonal stratospheric ozone depletion on the UV climate in Antarctica by using a biological test system. This method is based on the UV sensitivity of a DNA repair-deficient strain of Bacillus subtilis (TKJ 6321). In our field experiment, dried layers of B. subtilis spores on quartz discs were exposed in different seasons in an exposure box open to solar radiation at the German Antarctic Georg von Neumayer Station (70°37' S, 8°22' W). The UV-induced loss of the colony-forming ability was chosen as the biological end point and taken as a measure for the absorbed biologically harmful UV radiation. Inactivation constants were calculated from the resulting dose-response curves. The results of field experiments performed in different seasons indicate strongly season-dependent trend of the daily UV-B level. Exposures performed at extremely depleted ozone concentrations (October 1990) gave higher biologically harmful UV-B levels than expected from the calculated season-dependent trend, which was determined at normal ozone values. These values were similar to values which were measured during the Antarctic summer, indicating that the depleted ozone column thickness has an extreme influence on the biologically harmful UV climate on ground.
    Repository Name: EPIC Alfred Wegener Institut
    Type: Article , peerRev
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  • 8
    Publication Date: 2019-11-04
    Description: Geomagnetic field measurements at two Antarctic stations are compared during two weeks in the local summer (January 1-15, 1992). Low frequency (0.6-6 mHz) pulsations are observed at each station near local magnetic noon. The same wave packets appear in some cases also at the other station, although with a significant attenuation, more clearly in the morning sector; the waves show a near noon reversal of the polarization sense from counter-clockwise in the morning to clockwise in the afternoon indicating a westward and an eastward propagation, respectively.
    Description: JCR Journal
    Description: open
    Keywords: Geomagnetic pulsations ; Antartica ; 04. Solid Earth::04.05. Geomagnetism::04.05.02. Geomagnetic field variations and reversals
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
    Format: 2312070 bytes
    Format: application/pdf
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  • 9
    Electronic Resource
    Electronic Resource
    s.l. : American Chemical Society
    Journal of the American Chemical Society 39 (1917), S. 731-742 
    ISSN: 1520-5126
    Source: ACS Legacy Archives
    Topics: Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 10
    ISSN: 1432-1866
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Description / Table of Contents: Résumé Les auteurs montrent que des faits précis issus de la minéralogie expérimentale permettent d'attribuer un rôle important aux actions mécaniques et aux gradients thermiques dans l'étude des migrations et des concentrations d'éléments chimiques au sein de la lithosphère. Les actions mécaniques liées à la tectonique sont à l'origine d'une microporosité susceptible de transformer les roches mécaniquement non uniformes en immenses réservoirs de fluides. Les déformation tectoniques peuvent entraîner des tassements de cette porosité, si elles sont modérées, ou, au contraire, une large ouverture par microfissuration intragranulaire à partir de seuils de contraintes qui diffèrent selon la nature et l'histoire tectonique des roches. C'est ainsi que, sous des actions mécaniques comparables, certaines roches peuvent se tasser, tandis que les roches adjacentes peuvent s'ouvrir. Enfin, la microfissuration est susceptible de faciliter la libération des fluides essentiels (H2O, CO2) et d'accroître la solubilité de nombreux minéraux. Les roches poreuses et imprégnées de fluides sont soumises à un gradient thermique: le gradient géothermique. L'effet thermogravitationnel résultant de la thermodiffusion et de la gravité, peut permettre, à partir de solutions même diluées, d'obtenir des concentrations suffisantes pour donner lieu à des cristallisations sans déplacement de liquide. Les calculs réalisés à partir d'une théorie élémentaire montrent qu'avec des gradients géothermiques plausibles, les temps et les épaisseurs de roches poreuses, nécessaires pour réaliser des cristallisations, sont faibles à l'échelle géologique. Ce processus est aussi permanent que le gradient géothermique. Ce mode de concentration rend parfaitement compte de l'aspect rubanné des dépôts filoniens sans qu'il soit nécessaire d'imaginer d'importants déplacements de liquide. Il rend compte aussi de la concentration préférentielle de gîtes métallifères sur les coupoles des batholites éruptifs.
    Notes: Abstract The authors demonstrate that precise facts arising from experimental mineralogy enable an important role to be ascribed to the mechanical actions and thermal gradients in the study of the migrations and concentrations of the chemical elements to be found within the lithosphere. The mechanical actions associated with tectonic are, in the production of a micro-porosity, capable of transforming mechanically non-uniform rocks into immense reservoirs for fluids. The tectonic deformations can bring about reduction of the porosity if moderate or, on the contrary, can lead to a considerable opening-up by intragranular microfissuration commencing at different stress levels depending on the nature and tectonic history of the rocks. In this way, under the influence of comparable mechanical action, certain rocks may consolidate, whilst adjacent rocks may open up. Finally, micro-fissuration is capable of facilitating the release of essential fluids and gasses (H2O, CO2) and of increasing the solubility of many minerals. The fluid-impregnated porous rocks are subjected to the geothermal gradient. The effect of thermal diffusion and gravity provides concentrations, even in the case of diluted solutions, sufficient to induce crystallisation without displacement of the liquid. Calculations based on an elementary theory show that, with entirely plausible geothermal gradients, the times and the thicknesses of porous rock necessary to produce crystallisation are low when compared to the overall geological scale. This process is as permanent as is the geothermal gradient. The mode of concentration takes full account of the layered aspect of the venous deposits without the necessity to envisage large displacements of liquid. It also takes account of the preferential concentration of the metalbearing deposits on the domes of the batholiths.
    Type of Medium: Electronic Resource
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