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    30 December 1991, Volume 3 Issue 4 Previous Issue    Next Issue

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    THE SURFACE FLOW OF NELSON ICE CAP, WEST ANTARCTICA
    1991, 3 (4):  11-17. 
    Abstract ( 1616 )   PDF (200KB) ( 1119 )  

    In the present paper, authors analysed the spacial distributions and seasonal variation of the surface flow velocities of Nelson ice cap, the non-verticality between the flow vector and the contour at the same point, then explained the strain-rates along profiles N and E through the highest point on the surface of Nelson ice cap and the relation between the strain-rates and crevasses. Finally, authors compared these characteristics to the continental ice caps in China in order to show the marine features of Nelson ice cap in glacier dynamics. The following conclusions could be reached with those mentioned above: 1. The surface flow velocities become large gradually from the highest point to the edge of Nelson ice cap, and get their maximum at the edge. The summer velocities, which are 20.6 m/a and 18.6 m/a at the termini of Profile N and Profile E respectively, are higher than the maximum velocities on the continental ice caps. The mean annual velocities take 66-88% of the summer velocities. Spacially, the more close to the edge, the more the velocity vectors direct down to the surface. Therefore, it can be concluded that the balance equilibrium line appears near to the edge, or, ice-falls to sea water play an important role in the ablation of the ice cap. 2. The principal strain-rates are positive at the top of Nelson ice cap, 1 and 2 are +0.0079/a and +0.0034/a, respectively. 3. The limit of the principal extension strain-rates for the appearance of the ice crevasses on the surface is +0.007/a, on Profile N, and +0.0122/a on Profile E respectively.

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    EARLY TERTIARY PALAEO CLIMATE OF KING GEORGE ISLAND, ANTARCTICA
    1991, 3 (4):  18-23. 
    Abstract ( 1716 )   PDF (211KB) ( 1234 )  

    The Fossil Hill flora from the Fildes Peninsula of the King George Island, Antarctica has been studied, which consists of more than. 40 forms of ferns, gymnosperms and angiosperms, being a mixture of subantarctic and neotropical elements, mostly resembling the Early Tertiary South American palaeoflora. According to "the nearest living relative method" and "leaf physiognomical analysis", the plants of the Fossil Hill flora probably grew under the following environmental conditions: 1. The mean annual temperature was approximately 14-16℃. 2. The mean temperature of the coldest month was about 10℃. 3. The mean temperature of the warmest month was about 20℃. 4. The mean annual range of temperature was probably 7-10℃. 5. There was a lack of solar radiation during winter as a result of being the high latitude. 6. There was high precipitation (more than 1000 mm per year). 7. The area where the plants of the Fossil Hill flora were growing was at rather low altitude. The author tried to determine what caused the warm and humid climate during the time when the plants were growing, and proposes the following hypothesis. During Cretaceous and Early-Middle Palaeogene, Antarctica, Australia and South America as parts of the Gondwana formed a nearly continuous landmass along the southern margin of the Pacific Ocean. The Southern Pacific was effectively separated from other oceans and continents at that time and it is reasonable to assume that in the Southern Pacific the oceanic circulation of a warm current southward from the equator transported huge quantity of heat to Gondwana. The Circum- Polar Current developed about 38 Ma ago; since then the antarctic climate began deteriorating. The development of a Circum-Polar Current as it exists today requires deep sea conditions around the whole of Antarctica; this did not appear until the end of the Oligocene.

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    A STUDY OF FIUORIDE ANOMALY IN ANTARCTIC KRILL
    1991, 3 (4):  24-30. 
    Abstract ( 1726 )   PDF (585KB) ( 1278 )  

    The aim of the study is to investigate the existing form and the partitioning pattern of fluoride in krill (Euphausin superba) by analysing the fluoride and other elements in various part of klill, primarily to approach the potential accumulation mechanism and the effect of fluoride in klill on the geochemical characteristics of fluoride in the Antarctic ecoenvironment. The results of the study show that the amount of flu oride in various part of krill has a considerable difference. Most of fluoride is enriched in the carapace, up to 4028μg/g, and the head and legs, respectively 2724μg/g and 2828μg/g. The muscle contains the least fluoride with amount of 226μg/g. The amount of fluoride in whole freeze- dried krill is averagely 1232μg/g, which indicates that the functional position of fluoride in krill is mainly located at the crust. Only a few of fluoride is found in the chitin of the carapaces (200μg/g), which exhibits that fluoride in the carapaces exists mostly in the form of the nonchitious constituent.In addition, the varition and emichment of fluoride is related closely to some other elements such as P, Ca. Thus, fluoride in the carapaces is likely to exist as the form of the inorganic salt with P and Ca. It is also estimated from the study that a slightl yhigher concentration of fluoride in seawater and lower in sediment of the area relative to other oceans is possibly affected by the enrichment of fluoride in the huge storage of krill in the area. The bioprocesses and precipitation with relation to the activity of krill should be very important and key section to the geochemical cycling of the fluoride in Antarctic ocean.

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    OBSERVATIONAL STUDY OF RADIATION BALANCE COMPONENTS OVER LARESMAN HILLS
    1991, 3 (4):  42-53. 
    Abstract ( 1622 )   PDF (881KB) ( 975 )  

    A measurement project to obtain continuously surface radiation balance components as a part of CHINARE-IV research program was carried out over the Laresman Hills on which Zhongshan station (69?22'S, 76?22' E) is located, from Feb. 1990-Jan. 1991. The micro-computer sampling system was used with pyranometers and pyrradiometers for measurement of radiation flux, including direct solar radiation, global radiation, reflected radiation and net radiation (0.3-30μm). These values were sampled digi tally and recoided every minute at the height of 1.5m above the surface. In this paper, on basis of the data series obtained between Feb. 1990 and Jan. 1991 , analyses of seasonal means of these component in response to changing synoptic conditions are presented. Each radiative element has a characteristic of the marked diurnal and seasonal variation. In the summer, the flux of direct radiation is stronge, while in winter it is small (it becomes zero during polar night of 58 days). The transparent coefficients (Pm=/Sm/S.) are generally over 0.8 with a small seasonal change, indicating that the transparency of the atmosphere in sunny day is very high and the air is very clea n with few aerosol particles in it. The annual mean value of the global radiation is 119.2 W/m2 about 90% of which is obtained between October-March, The peak value of the instantaneous flux could be as large as 1095W/m2 since the cloud has a strong effect ons catting radiation in December. The annual mean albedo is 0.42, and the albedo varies very large from day to day because of changing status of the snow surface closely related to the weather condition. The mean albedo in the summer is 0.27 on the bareland surface and it is 0.51 in the cold season on the snow surface. The albedo over 0.9 could be observed on the fresh snow covered surface. The annual mean value of the net radiation is 11.7 W/m2.It is indicating that the surface of the region is a heat source to the air. Therefore the budget of the radiation energy over the region differs greatly from that in Antarctic inland area. The mean value of the net radiation from October to March is positive (64.1 W/m2) and it is negative (-40.6 W/m2) in rest time. It means that the heat is absorbed by the surface in summer half year, and the heat lost from surface in the winter half year. This variation should be considered in analysis on the effect of the polar radiation status on the global circulation.

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    VARIATION CHARACTERISTICS OF SUMMER BOTTOM WATER TEMPERATURE IN THE GREAT WALL BAY, ANTARCTICA
    1991, 3 (4):  54-59. 
    Abstract ( 1707 )   PDF (253KB) ( 1041 )  

    The successive three-month bottom water temperature observational data were, acquired in the Great Wall Bay, Antarctica, in the summer of 1987. In this paper the observation is described and the data is statistically analysed. The conclusions arc as follows: 1. The bottom water temperature in the Great Wall Bay is relatively low and has no obvious change in summer due to the geographical location. The mean, the maximum and the minimum of that summer's bottom water temperature were 0.83℃, 2.70℃ and-1.32℃, respectively. The monthly mean maximum temperature occu- red in February, whose mean, maximum and minimum were 1.28℃,2.70℃ and 0.56℃, respectively, and all these were the highest among the months of that summer. 2. The daily mean temperature of the bottom water increased slowly at a mean speed of 0.05℃/d from January 10 to February 10, and reached the maximum, 2,16℃, on February 9, then decreased rapidly at a mean rate of 0.15℃/d from February 10 to February 20, and kept basically unchanged from February 20 to March 15, after that it gradually decreased again to below 0℃ on April 1 and then to -1.02℃ till April 9. The daily mean bottom water temperature decreased roughly with the decreasing of sunshine time, but there was a time lag in existence. 3. Owing to the effect of local physical geographic conditions, the diurnal change of the bottom water temperature in the Great Wall Bay is not very evident. In that summer, the daytime mean temperature of the bottom water was 0.88C, and the night time was 0.76℃, their difference was only 0.12℃.The minimum occuiedat5o'clock with an average of 0.74C while the maximum at 14 o'clock, whose average was 0.98℃. The minimum daily range was 0.14℃ and the maximum was only 1.25℃. 4. Because the Great Wall Ba y is relatively shallow, the bottom water temperature is affected by the local air temperature. On the average of that summer, the daily mean temperature of bottom water was only about 0.47℃ higher than that of the air; the daily range of bottom water temperature (0.24℃) was much smaller than that of the air tem perature (1.37℃); and the daily maximum and minimum of bottom water temperature occured 2h and 5h later than that of the air's, respectively. 5. The compulated results of the power spectrum show that the spectral peak of the bottom water temperatuie appeals at the frequency of 1 cpd, which is the same with the air's temperature. Both of them have apparently diurnal change. The co-herence function, R(lcpd) =0.94 means that the bottom water temperature is closely correlated with the air temperature at the frequency of 1 cpd.

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