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    30 September 1999, Volume 11 Issue 3 Previous Issue    Next Issue

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    THE STUDY ON THE DEPOSITIONAL STYLES OF MAJOR IONS AND THE CLIMATIC EFFECT OF nssSO_4 ~(2-)IN PRINCESS ELIZABETH LAND,ANTARCTICA
    1999, 11 (3):  161-168. 
    Abstract ( 1803 )   PDF (185KB) ( 1219 )  
    Snow samples collected from a 50 meter firn core along the route of the 1996/1997 Chinese First Antarctic Inland Traverse Expedition in Princess Elizabeth Land,East Antarctica,have been analyzed for chemical composition and oxygen isotope ratio. Analyzing the relationship between the concentration and flux of major ions and accumulation rate can draw the following conclusions. 1) The concentrations of major ions in the atmosphere in the study region is big enough to guarantee the concentrations of the ions do not vary with snow accumulation rate,that is to say,the concentrations of major chemical species are independent of snow accumulation rate. 2) The results of analyzing the depositional styles of major chemical species suggest that wet deposition dominate the major ions flux. In addition,there is no apparent correlation between nssSO 2- 4 fluctuations and isotope profile. This would indicate the climatic effect of volcanism is not evident in the region.
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    THE DISCOVERY AND GEOLOGICAL SIGNIFICANCE OF PEBBLY MUDSTONE IN THE MIERS BLUFF FORMATION IN LIVINGSTON ISLAND, WEST ANTARCTICA
    1999, 11 (3):  169-178. 
    Abstract ( 2625 )   PDF (350KB) ( 2474 )  

    Livingston Island constains several distinctive sedimentary and volcanic sequences, which document the history and evolution of an important part of the South Shetland Islands magmatic arc. The sedimentary sequence is named the Miers Bluff Formation (MBF) and is interpreted as turbidite since the first geological study on South Shetland Islands. It base and top are not exposed, but a thickness of more than 3000m has been suggested and seems plausible. The turbidite is overlain by Mid-Cretaceous volcanic rocks and intruded by Eocene tonalites. The Miers Bluff Formation and its correlatives, including Trinity Peninsula Group(TPG) in Graham Land, Antarctic Peninsula and Greywacke-Shale Formation (GSF) in South Orkney Islands, display the same lithology and tectonic style, share a common provenance and possibly the same age, but the age is poorly constrained Late Carboniferous-Early Triassic. The pebbly mudstone is common in the TPG, but is scarce in MBF outcrops. In the 1997-1998 year field exploration, four pebbly mudstone layers are distinguished near the Spanish Antarctic Base-“Juan Carles I” Station in Hurd Peninsula, Livingston Island. These layers of pebbly mudstone are massive and no-traction flow structure, and usually over ten meters thick and contain great amount of igneous,sedimentary and metamorphic pebbles. In general, grained size is 4-7 cm, the largest pebble is up to 85 cm, but the bigger pebbles(>50cm) are sparse and are preserved near upper surface in common. Their sorting is bad but their psephicity is well-rounded. These layers of pebbly mudstone are sharply contact with thickened sandstones, they are common in the MBF. The pebbly mudstone is the typical rock of debris flow, may belongs to sediments in the mouth of canyon, the channel of and upper and middle fan of submarine fan and the boundary between the deep sea basin and steep slope. Meanwhile, the depositional environment of MBF is the upper and lower of mid-fan of submarine fan. Hence, the depositonal environment of pebbly mudstone may be the channel of mid fan of submarine fan. MBF has the same tectonic setting, therefore, as the TPG, may be the same history of sedimentary and metamorphism as TPG, too, and Livingston Island contacts with Antarctic Peninsula before the formation of Mesozoic-Cenozoic magmatic arc.

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    STUDY ON ENVIRONMENTAL CHANGE AND PHYSICOCHEMICAL CHARACTERISTICS OF AEROSOL IN ANTARCTICA
    1999, 11 (3):  179-191. 
    Abstract ( 1917 )   PDF (602KB) ( 1594 )  

    The present study situation of the aerosal in Antarctica was reviewed in this paper. Taking the volcanic eruption of Pinatubo Mt. and Cerro Hudson Mt. (from during Jun,1991 to September,1991) on the aerosol as an example,the effect of the volcanic eruption activity on aerosol was analyzed. This paper studies the source,The sink and the physicochemical characteristics of the aerosol,and also analyses the mass-size distribution and transitive processes of aerosol in aerosphere.It was shown that the effect of the aerosol from these volcanic eruption on the global environment ant Antarctic environment.

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    A METHOD OF DITERMINATION OF AURORA SHIFT
    1999, 11 (3):  192-202. 
    Abstract ( 1767 )   PDF (350KB) ( 1327 )  

    Auroral images taken by all sky camera are one of important data sources for studying dynamic processes in the polar regions related with magnetospheric substorm, particle precipitation and upper atmospheric properties. It is also essential for understanding solar wind magnetosphere ionosphere coupling. In this paper we use a correlation analysis technique of moving random pattern to calculate the shift velocity of auroral image. Thus the obtained velocity is a kind of “bulk” or “average” velocity of whole image, instead of the velocity for some certain points or parts in the auroral pattern. The technique is used to analyze an example of aurora australis recorded at Zhongshang Station in the Antarctica on June 23, 1997. The results show that the maximal velocity of the auroral pattern in this event is 2.8km/s in east-west direction. Since it takes only a few seconds for energetic particles to travel from the magnetotail to the ionosphere, the obtained aurora velocities would directly reflect the shift situation of the auroral particle source region in the magnetotail.

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    AURORAL PARTICLE PRECIPITATION AND ITS SPECTRA TRANSPORT IN THE ATMOSPHERE IN ANTARCTIC REGION
    1999, 11 (3):  203-220. 
    Abstract ( 1744 )   PDF (463KB) ( 1420 )  

    Auroral precipation electron and proton fluxes and spectra are reviewed in the Antarctic region, those region includes auroral oval, polar cap, the south Atlantic anomaly(SAA), polar cusp/cleft. And two new auroral particle spectra are given based on recent' result of magnesphere study. One is kappa distribution spectra; the other is kappa distribution plus one or more monoenergetic electrons or ions spectra. the two kinds of particles precipation may source from magnetatil neutral sheet non adibatic region and adibatic region. And then an approximate analytic description of the energy spectrum of auroral electrons and ions at any atmosphere depth is derived for incident spectra of precipitation particles-such as Maxillian distribution; Velocity distribution; Kappa distribution; monoenergtic distribution spectra etc. These spectra transpoting in the atmosphere isillustrated vs altitude profiles.

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    LITHOSPHERE VELOCITY STRUCTURE IN TRANSANTARCTIC MOUNTAINS ALONG 167°E PRINCIPAL VERTICAL CIRCLE
    1999, 11 (3):  221-227. 
    Abstract ( 1564 )   PDF (357KB) ( 1302 )  

    This paper is based on the Rayleigh surface wave seismogram along earth's great circle across SPA and SBA seismic stations. We computed a phase velocity dispersion of Rayleigh surface wave and obtained lithosphere structure of 200km path below two stations. Our result shows that crust thickness of transantarctic mountains is 45 km. In depth of 55~75 km there are clear layers of low velocity. It displays deep fused magma.

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    ANALYSING OF THE AURORA AND GEOMAGNETIC DISTURBANCE IN ZHONGSHAN STATION,ANTARCTICA
    1999, 11 (3):  228-234. 
    Abstract ( 1614 )   PDF (141KB) ( 997 )  

    The passage outlined of the dispersion law over time of the frequency that three different aurora(strong,middle,weak) had occurred during the night(GUT 11:00-24:00) in Antarctic Zhongshan Station has relationship with geomagnetic field disturbance by analysizing the observed aurora and disturbance. The weak aurora appeared at 10:00 o'clock and its frequency of occurrence reached the peak at 15:00;The middle appeared at 11:00,reached the peak during 21:00-22:00, and especially its frequency is stable at 19:00; the strong ones occurred at 16:00 and reached the peak during 20:00-21:00. The dispersion over time of frequency that all kinds of aurora occurred is approximately compliant with the disturance of geomagnetic field. The weak aurora accompanies disturbance of small amplitude. The strong aurora correspond with large amplitude. The time of aurora occurrence is partially the same as that of disturbance.This partially correspondence relates to the various status of aurora. Furthermore,this various aurora status is affected by space environment.

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    RESEARCH ON CHINESE ANTARCTIC DATA DIRECTORY SYSTEM Ⅰ. COLLECTING,PROCESSING,EXAMINING AND SUBMITTING DATA DIRECTORY
    1999, 11 (3):  235-240. 
    Abstract ( 1672 )   PDF (138KB) ( 987 )  
    With the general framework of ADDS established by JCADM, The CN ADDS project is going on, the research and activity of which keep to the available method and technique in ADDS development and allow for the Chinese specific status in Antarctic data management. At present, Authoring and submitting timely Antarctic data directory in China is one of the key issues that is to be deal with necessarily. In this context, the authors address an integrated process of collecting, processing, examining and submitting data directory after great efforts of several years in this paper. Undoubtedly, it provides a concrete means and groundwork for the next work. Subsequently, the efficient management of data directory collection is also discussed to ensure that data directory may be authored and submitted as expected, and that the CN ADDS will be accomplished and operate successfully.
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