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    30 September 2003, Volume 15 Issue 3 Previous Issue    Next Issue

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    OVERVIEW OF METEORITE COLLECTIONS FROM GROVE MOUNTAINS, ANTARCTICA
    2003, 15 (3):  161-170. 
    Abstract ( 1401 )   PDF (340KB) ( 1404 )  

    Petrography, mineral chemistry and classification of 32 meteorites collected by the 15 th and 16 th Chinese Antarctic Research Expeditions (CHINARE) were summarized. These meteorites include 23 equilibrated ordinary chondrites, 6 unequilibrated ordinary chondrites, 1 Martian lherzolite, 1 eucrite, and 1 ungrouped iron meteorite. Possible meteorite concentrating mechanisms in Grove Mountains area, unusually low cosmic ray explosion age of GRV 98004 (H5), and ejection ages of Martian meteorites are discussed. In addition, several aspects in the future study of Grove Mountains meteorites are proposed.

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    ABUNDANCE AND ADAPTABILITY TO TEMPERATURE OF GENERAL AEROBIC HETEROTROPHIC BACTERIA FROM THE CHUKCHI SEA AND BERING SEA
    2003, 15 (3):  171-176. 
    Abstract ( 1759 )   PDF (283KB) ( 1577 )  

    The abundance of general aerobic heterotrophic bacteria (GAB)from the water and sediment in the Bering Sea and the Chukchi Sea was determined by using petri dish cultivation and counting method. The abundance of GAB among the different sea areas, sampling sites, layers of sediments surveyed and adaptability to differential temperatures were studied. The result obtained showed that: the occurrence percentage of GAB in the surface water was higher than that in sediment, but the abundance was only 0.07% of sediment. The occurrence percentage of GAB in surficial layer of sediment was higher than that in the other layers. The occurrence percentage, abundance and its variation of GAB in Bering Sea were higher than that in the Chukchi Sea respectively. The average value of the abundance in the all sediment surveyed was 3166.3×10 2CFU·g -1 (Wet.). The abundance of GAB in sediment showed a trend: roughly higher in the lower latitudinal area than higher latitude. The results from temperature test mean that: the majority of bacteria tested were cold adapted ones, minority might be mesophilic bacteria. The results indicated that, arctic ocean bacteria had a stronger adaptability to environmental temperature.

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    IMPACTS OF STATION GARBAGE ON THE DIET OF ANTARCTIC SKUAS IN KING GEORGE ISLAND
    2003, 15 (3):  177-185. 
    Abstract ( 1355 )   PDF (367KB) ( 1675 )  

    Diet of South Polar and Brown skuas C. maccormicki and C.s.lonnbergi were investigated during the years of 2001—2003 in Fildes Peninsula, King George Island, Antarctica. The results show that percentage components of natural food in their food composition were 63.4% for Brown skua and 77.8% for South Polar skua. Meanwhile the components of the food from station waste were 36.6% and 22.3% respectively. It is clear that foraging of skuas near Great Wall Station was dependent on both of natural resources and station garbage. This is much related to environmental status as well as management of waste material in the stations. Closed treatment technique should be used for station waste, for the benefit of Antarctic environmental protection.

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    THE FEATURES OF f_0F2 AT ZHONGSHAN STATION OF ANTARCTICA
    2003, 15 (3):  186-194. 
    Abstract ( 1677 )   PDF (159KB) ( 1756 )  

    The data of f 0 F2, measured by a Digisonde Portable Sounder (DPS 4) at Zhongshan Station of Antarctica in 1995, the hemispheric power index and the midnight equatorward boundary of the aurora, estimated by observations of American NOAA and DMSP satellites are used to examine features of the polar ionosphere. The results show that the major source of electron and ion production at Zhongshan Station is almost completely dependent on particles precipitated from the magnetosphere. Under a quiet environment of the solar activity and geomagnetic variation, the soft particles in the cleft are the controlling source of ionospheric ionization at dipole magnetic noon. The ionized effect of energy particles is also important during several hours both in the morning and afternoon when the station lies in the auroral region. The electron density is much lower at night in the polar cap areas. The ionization action of solar EUV radiation in summer makes the monthly median of f 0 F2 1—1.5hr MHz larger than that in winter, and the time of the peak of the f 0 F2 diurnal variation in summer is 1—2hr earlier than in winter. During a strong disturbance period, the cleft and auroral regions move toward lower latitudes. The electron density will decrease a lot and the ionospheric echo may often not be received when the station is located at the polar cap area. The situation is more complex under a moderate disturbed environment. Since at high latitudes the magnetospheric convection velocity can become very large and the recombination coefficient of the colliding ion and neutral is highly increased, global meridional thermospheric circulation has not led a remarkable intension of electron density in the high latitude ionospheres. During disturbed periods the southward plasma flux carried by convection has not noticeable effect to increase f 0 F2 at Zhongshan Station too.

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    UPPER OCEAN HYDROGRAPHIC PROPERTIES OF SOUTHEAST INDIAN OCEAN IN AUSTRAL SUMMER, 2003
    2003, 15 (3):  195-206. 
    Abstract ( 1398 )   PDF (437KB) ( 1665 )  

    The data of 28 XBTs and 25 XCTDs obtained by the 19 th Chinese National Antarctic Research Expedition in the section from Prydz Bay, Antarctica to Frementle, Australia in February, 2003 are used to analyze the properties of water masses distribution and fronts of the upper ocean, and the influence of sea ice, precipitation and advection on the freshwater and heat input of sea surface south of Polar Front (PF) is discussed. An unusual low salinity (34.58) water mass is observed at the depth of 800—900m in the location around 63.5°S,79.7°E. The Antarctic Slope Front (ASF), Polar Front (PF), Subantarctic Front (SAF) and Subtropical Front (STF) appear in the investigation section from south to north. PF lies on 54°S, ,90.4°E; SAF locates at 45.3°—47.5°S ,102.5°—104.4°E and reaches the bottom of the measured depth with two high temperature gradient cores; For the first time double STF structures is discovered and locate at 41.9°—42.6°S, ,106.7°—107.3°E and 37.7°—38.9°S, 109.8°—110.7°E, respectively. PF, SAF and STF can be identified from the properties of surface layer in some degree. Especially, the representation of SAF in the temperature and salinity of surface layer is distinct. The flow cores of ACC passing the investigation section locate at PF and SAF, which is in consistent with the historical data. The variation trend of freshwater and heat input on the sea surface south of PF is in close correlation with the meridional distribution of the thickness of sea ice and the range of sea ice extending northward in this region in austral winter.

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    AN ASSESSMENT OF VARIATIONS IN MERCURY DEPOSITION TO ANTARCTICA OVER THE PAST 34000 YEARS
    2003, 15 (3):  207-213. 
    Abstract ( 1433 )   PDF (274KB) ( 1373 )  

    Comparing the variation of the Hg concentrations in 14 subsamples from Antarctic Dome C ice core (Vandal et al., 1993) with the precipitation proxies such as δ 18 O values and 10 Be concentrations in the Dome C ice more, we found a significant correlation between Hg concentrations and δ 18 O values, 10 Be concentrations. And this clearly indicates that the accumulation rate in Dome C is one of the key factors to the variations of Hg concentrations. Therefore, Hg concentrations in ice core can be used as a proxy of precipitation rate. In this paper, we reassess the variations in mercury deposition flux in Antarctica over the past 34,000 years on the base of the high resolution δ 18 O values, which can be used as a good proxy reconstructing the precipitation rates. In our results, the highest mercury deposition flux is about 3.80pg cm -2 a -1 during the Last Glacial Maxium (LGM), as high as 3.5 times of the mercury deposition flux (about 1.08 pg cm -2 a -1 ) in Holocene. And this is because of the fluctuations in natural mercury emissions such as the oceanic biological emission.

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    INVESTIGATION ON POLAR SCIENCE INFORMATION RESOURCES UNDER THE WEB ENVIRONMENT
    2003, 15 (3):  214-222. 
    Abstract ( 1465 )   PDF (137KB) ( 1600 )  

    This paper introduced the polar scientific information resources of the Internet systematically, including the polar search engine, polar organization and programs, scientific research results (database, electronic periodicals and online publications). Through collecting and investigating the polar science website information, we suggested that the navigation database of the polar scientific information should be built.

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    VOLCANISM RECORDED IN POLAR ICE CORES AND ITS EFFECTS ON CLIMATE
    2003, 15 (3):  223-232. 
    Abstract ( 1680 )   PDF (408KB) ( 1730 )  

    Major volcanic eruptions leave traces in polar ice mainly as strong acids like sulphuric acid. Historical volcanism can be detected in polar ice by continuous ECM (Electrical Conductivity Method) measurements or sulfate concentrations in melted samples, while known volcanic eruptions may be used to date ice cores. Volcanic signals preserved in polar ice cores depend on not only the magnitude, type, geographical location and composition of acid gases from volcanic eruptions, but also atmospheric aerosol transportation efficiency, local annual accumulation and post depositional process at precipitation sites, and so on. A single volcanic eruption usually lead to relative climate cooling of several months to a few years on hemispherical or even global scale, but further work is needed to improve understanding of the climate volcanism connection and the effects of large scale volcanic eruptions on long term (several decades or more) climate changes.

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    STUDY OF VERTICAL PARTICLE FLUXES IN THE DEEP OCEAN OF THE NORTH OPEN SEA OF PRYDZ BAY,ANTARCTIC I:SOURCES OF ERRORS IN SEDIMENT TRAP MEASUREMENT AND RECOMMENDATIONS
    2003, 15 (3):  233-238. 
    Abstract ( 1288 )   PDF (113KB) ( 1416 )  

    Much of the current understanding of biogeochemical processes can be traced directly to data from sediment traps. Traps are used to quantify not only the flux patterns with space, time and depth, but also to serve as collectors for sampling sinking particles for chemical and physical analysis. While traps are widely relied upon to serve as accurate “particle gauges” in the oceans, there are different opinions about the absolute accuracy of traps. In this paper, based on the current researches, we report the results about the sources of errors in sediment trap measurements and corresponding recommendations, and focus primarily on the problems of “swimmers” removal methods and conservation of particles.

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