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    30 September 2001, Volume 13 Issue 3 Previous Issue    Next Issue

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    DEPENDENCE OF THE POSTNOON AURORAL INTENSITY UPON THE SOLAR WIND PARAMETERS
    2001, 13 (3):  151-158. 
    Abstract ( 1509 )   PDF (211KB) ( 2382 )  

    Based on auroral observations of a multi channels scanning photometer at Zhongshan Station, Antarctica and solar wind parameters data obtained by WIND Satellite at the upstream of the bow shock in 1997 and 1998, the dependence of the high latitude postnoon auroral intensity upon the solar wind parameters are studied quantitatively. It is shown that the 630 0nm intensity depends on the solar wind parameters more directly than the 557 7nm does. The 630 0nm intensity increases as the solar wind plasma density, dynamic pressure and speed increasing, with a correlation coefficient of 0 84, 0 88 and 0 61 respectively. While the dependence of 557 7nm intensity upon the solar wind parameters are not so clear. The difference between the dependences of 630 0nm and 557 7nm intensities upon the solar wind parameters indicates that the 630 0nm emission is influenced by solar wind more directly than the 557 7nm is, while the 557 7nm emission is related to magnetospheric dynamic processes sometimes.

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    OXYGEN ISOTOPE COMPOSITION OF SURFACE SNOW COLLECTED IN THE AUSTRAL SUMMER ALONG THE TRAVERSE ROUTE FROM ZHONGSHAN STATION TO DOME A,ANTARCTICA
    2001, 13 (3):  159-164. 
    Abstract ( 1539 )   PDF (165KB) ( 1208 )  

    Oxygen isotope composition of surface snow sampled in the austral summer of 1998/1999 along the traverse route from Zhongshan Station to Dome A, Antarctica is measured with the conventional mass spectrometer technique. The results of measurement show that oxygen isotope composition of surface snow varies in a wide range from -22.51‰ to -50.67‰, and has a tendency that isotopic values gradually decrease with the increases of distance from Zhongshan Station and altitude. The linear regression analyses indicate that there exists good correlation between oxygen isotope composition of surface snow and distance from Zhongshan Station, altitude or latitude, which actually reflects the close relation between stable isotope composition and temperature.

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    2001, 13 (3):  165-174. 
    Abstract ( 1533 )   PDF (258KB) ( 1337 )  

    Physical and chemical factors (such as pH, T, S, conductivity, turbidity, DO, COD and nutrients), chlorophyll in the sea water column were monitored at eight sites in the coastal zone in Zhongshan Station, East Antarctica from Dec. 11, 1998 to Jan. 13, 1999. The samples were collected at several layer of sea water at six sites among them, meanwhile, domestic sewage of Zhongshan Station was monitored hourly for two days at the mouth of a drain pipe located at the beach near Zhongshan Station. The results indicated that the physical and chemical factors changed sharp within the sea water column from about 1m under the bottom of the sea ice to the surface, and changed gently in the water column below about 1m under the bottom of the sea ice, the obvious rules were observed in the vertical distribution of the nutrients ( such as PO 4 P, NO 3 N, NO 2 N and NH 4 N) in the water column. DO and pH in the monitored sea water belong to Category I sea water quality standard of China, the concentration of inorganic nitrogen belong to Category I and Category II sea water quality standard, the concentration of PO 4 P exceeds Category III sea water quality standard. The concentration of chlorophyll a in the surface of sea water ranged from 0.090 to 2.468mg/m 3, and the average concentration was 0.671 mg/m 3. COD, pH and suspended matter in the domestic sewage of Zhongshan Station meet the waste water effluent standard of China, only the concentration of PO 4 P exceeds Category I effluent standard. The monitoring methods of ecological environment conducted in the coastal zone in Zhongshan Station were discussed in this paper.

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    AIR-SEA FLUXES AND THE DISTRIBUTION OF SINK AND SOURCE OF CO_2 BETWEEN 80°W AND 80°E IN THE SOUTHERN OCEAN
    2001, 13 (3):  175-186. 
    Abstract ( 1670 )   PDF (577KB) ( 1685 )  

    The partial pressure of carbon dioxide in surface water and atmosphere along the track between Zhongshan Station and the Great Wall Station in the Southern Ocean was continually measured during the summer voyage for CHINARE XVI from December 1999 to February 2000. The results show that there is a sink for atmospheric CO 2 during summer between 80°W to 80°E in the Southern Ocean, especially in the area of 45°W to 30°W and 10°W to 10°E. The similar pattern of sink distribution can also be observed from the return observations from the Great Wall Station to Zhongshan Station. Absorbing CO 2 from air to sea in the investigated waters in January was twice higher than that in December. Using the newest calculation of transfer velocity of CO 2, fluxes of CO 2 was 3.98 and 2.13 mol/ (m 2·a) in January and December respectively. The average of total CO 2 fluxes in the Southern Ocean during summer was 3.06 mol/(m 2·a), suggesting an important summer sink of CO 2 in the South Hemisphere.

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    ANALYSIS ON THE 6 SPECIES OF ALGAE AND LICHEN BY SR-XRF IN THE FILDES PENINSULA OF ANTARCTICA
    2001, 13 (3):  187-194. 
    Abstract ( 1361 )   PDF (232KB) ( 1372 )  

    In order to study the relationship between the plant and the environment, and to make an inquiry into the function of testing surrounding, without a standard specimen, we had analyzed 6 species of algae and lichen about elements in the Fildes Peninsula of Antarctica by mini-beam XRF. Specimens are Ulva pertusa , Halymenia sp. and Lyngbya major which belong to algae, and Cladonia borealis , C. fimbriata and Usnea sp. which belong to lichen. The result turns out to be that various algae show different absorption for every elements. In XRF spectra, Ulva pertusa possesses more elements than Halymenia sp., like Br, As and Rb. The content of Cu and Zn is high too. In XRF spectra of Lyngbya major , the content of K is lower than Ca, the content of Zn is high. The element component in 3 species of lichen of Antarctica is very similar each other,but the relative content of Mn, Fe, Cu and Zn is different.

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    THE BIOGEOCHEMISTRY OF CARBON CYCLE IN SUMMER OF THE PRYDZ BAY,ANTARCTICA Ⅱ:CHARACTERISTICS OF POC DISTRIBUTION
    2001, 13 (3):  195-204. 
    Abstract ( 1402 )   PDF (183KB) ( 1185 )  

    The distribution and content of particulate organic carbon (POC) in Prydz Bay were investigated during CHINARE 15. The results showed that the concentration of POC in the surface layer of Prydz Bay was 94.20-1124.00μg/l,average concentration was 279.11μg/l . The surface POC distribution in summer shows that POC is much higher in Prydz Bay than that out of Prydz Bay. From the POC concentrations with the depth, we can see that the POC content in upper layer is higher than that in bottom, and in 100m the POC content is the highest. POC content has good correlation with chl a ( r=0.889, n=91 ) suggests that POC was mainly from the biological production in the local water columns. The value of POC/chl a in Prydz Bay is higher than that in other areas but similar to the value in Ross Sea. Furthermore there was negative relationship between POC and inorganic nutrient(DIN?PO 3- 4 ), the value of the " r " is -0.607 and -0.486( n =86)respectively.

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    STUDY AND OBSERVATION OF THE GREAT SOLAR EVENT IN JULY OF 2000 AT CUSP LATITUDE
    2001, 13 (3):  205-212. 
    Abstract ( 1737 )   PDF (346KB) ( 1533 )  

    A series of solar flare and coronal mass ejection (CME) event occurred in July of 2000, particularly the largest flare (X5.7/3B) with CME on 14 July since 1989, which induced a great geomagnetic storm with Dst index reaching -300nT. A set of data is obtained from the Chinese Antarctic Zhongshan Station (ZHS,INT Lat. 74.5°, L≈14), which is located at cusp latitude, and from the ACE satellite. Analyzed these data and got the results as follows: a lot of solar highly energized particles penetrated into the polar ionosphere and ionized it, which significantly increased the cosmic noise absorption (CNA) and blanked the DPS 4 data for more than two days. The magnetic pulsation in Pc 3/5 frequency band on the ground has a high relation with the fluctuation of interplanetary magnetic field (IMF) Bz, which shows the contribution of interplanetary MHD waves to the Pc 3/5 pulsation on the ground. The Pc 3/5 pulsation was intensified much during the great magnetic storm. H component of the magnetic field at ZHS varied with the IMF Bz but lagged about 8-10h, while Dst index responded to the variation of the IMF Bz very quickly, which suggested that the magnetic storm occurred at low latitude firstly and then effected the ionospheric current at high latitude.

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    ACTIVE SUBSTANCES IN THE ANTARCTIC KRILL
    2001, 13 (3):  213-216. 
    Abstract ( 2062 )   PDF (215KB) ( 2151 )  

    The digestive proteinases and other active substances derived from Antarctic Krill was introduced. The biochemical composition and its potential chemonucleolytic agents value was also summarized.

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    APPLICATION OF GEOGRAPHIC INFORMATION SYSTEM(GIS) FOR ANTARCTIC EXPEDITION AND RESEARCH
    2001, 13 (3):  217-228. 
    Abstract ( 1494 )   PDF (200KB) ( 1935 )  

    In recent 10 years, Geographic Information System (GIS) was applied more and more widely in Antarctic expedition and research since most of data collected and analyzed by the scientists and logistician is spatial. GIS Application in Antarctica includes various aspects such as spatial data collection, display and maintenance, scientific research, environmental evaluation, logistic management, and decision-making. Large international GIS projects usually developed by the Working Group on Geodesy and Geographic Information (WG-GGI) of the Scientific Committee on Antarctic Research (SCAR) are presented every two years. Some projects, such as Antarctic Digital Database (ADD), Antarctic Geographic Data Integration (AGDI), King George Island GIS (KGIS), Spatial Data Standards, have achieved considerable success, exerted a widespread influence in Antarctic research field. In addition, a lot GIS programs have been developed and conducted by the major Antarctic expedition countries, which will provide reference for our Antarctic GIS work in future.

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