南极中山站固体潮观测分析

中国南极中山站位于南极拉斯曼丘陵地区，１９９１年３月至１９９３年２月，用Ｌａｃｏｓｔｅ ＥＴ型重力仪，在这个地区进行了为斯的两年的观测，取得了６００多天有效资料，经调和分析和流变模型，海潮负荷必正后得到：δｏｌ＝１．２２５３±０．００３１，Δψｏｌ＝０．７３°±０．１４°；δｍ２＝１．０７８５±０．００４５，Δψｍ２＝－３．５５°±０．２９°从资料分析的精度来看，观测资料是比较好的；但由于海潮负荷     

青藏高原4月—10月光合有效量子值的气候学计算

根据１９９４年４月～１０月青藏高原太阳分光辐射的实测资料，计算出太阳总辐射中，光合有效辐射（ＰＡＲ）所占比例η＝０．４３９±０．００９，ＰＡＲ每１Ｊ的能量含有４．４３μｍｏｌ的量子。在青藏高原的气候学计算中，可用下式估算旬平均的ＰＡＲ能量日总量ＨＰＡＲ（ＭＪ·ｍ－２ｄ－１）和量子日总量ＵＰＡＲ（ｍｏｌ·ｍ－２ｄ－１）：ＨＰＡＲ＝（０．３９９＋０．０３６ｌｇＥ＊）ＨＵＰＡＲ＝（１．７６８＋０．１５９ｌｇＥ＊）Ｈ式中Ｈ（ＭＪ·ｍ－２ｄ－１）为总辐射旬平均日总量，Ｅ＊＝Ｅ·Ｐ０／Ｐ，Ｐ０（ｈｐａ）为标准大气压，Ｐ（ｈｐａ）为测点大气压，Ｅ（ｈｐａ）为地面水汽压。     

1988／1989年夏季南极长城海湾生态环境观测

自１９８８年１１月至１９８９年３月，对南极长城湾（６２°１３′Ｓ，５８°５７′Ｗ）中５个站位的水温、ｐＨ值、海水透明度、水下照度、水中和海冰中叶绿素含量、磷酸盐含量、亚硝酸盐和硝酸盐含量等理化要素，每月进行１至２次不定期的常规测定。在整个调查期间，海水温度变化范围在－１．６～２．２°Ｃ之间，ｐＨ值变化范围在８．０～９．１之间，海水中叶绿素ａ的变化范围在０．３０～１．４８ｍｇ／ｍ３之间，叶绿素ａ的最大值出现在１１月２６日５号站的表层水中，海冰中叶绿素ａ的含量远远高于海水中的含量，海冰中叶绿素ａ的变化范围在２．５５～５６．８４ｍｇ／ｍ３之间。磷酸盐含量变化范围在１．０２３～２．１８７μｇＰ／Ｌ，亚硝酸盐含量变化范围在０．０９３～０．１８６μｇＮ／Ｌ之间，硝酸盐含量变化范围在１３．３０８～２６．５８４μｇＮ／Ｌ之间。本文对以上结果作了初步探讨     

西太平洋海-气二氧化碳分压差及其通量研究

本文研究了中国第八次南极科学考察青岛至南极航渡中所观测到的大气与海水二氧化碳分压资料,结果表明：７°Ｎ以北、０°至２°Ｓ、１０°Ｓ至４３°Ｓ之间及５８°Ｓ以南的海域是大气二氧化碳的汇区,其间碳通量平均约为６．１ｍｇ／（ｍ２ｈ）;７°Ｎ至０°、２°Ｓ至１０°Ｓ及４３°Ｓ至５８°Ｓ则为大气二氧化碳的源区,其间碳通量约为４．０ｍｇ／（ｍ２ｈ）。     

南北两极海冰的涛动关系

本文将南极海冰分为４个区：ＳＰＩ１（０°－１２０°Ｅ），东南极海冰；ＳＰＩ２（１２０°Ｅ－１２０°Ｗ），以罗斯海为主体的海冰区；ＳＰＩ３（１２０°Ｗ－０°），以威德尔海为主体的海冰区；ＳＰＩ４，全南极海冰区。北极海冰区分为３个区：ＮＰＩ１（９０°Ｅ－１８０°－９０°Ｗ），太平洋侧冰区；ＮＰＩ２（９０°Ｗ－０°－９０°Ｅ），大西洋侧冰区；ＮＰＩ３，全北极冰区。本文使用了ＷＤＣ－Ａ的ＳＩＧＲＩＤ海冰资料，以分析南极和北极各冰区之间的相互关系。发现两极各冰区之间存在着非常复杂的相互作用。其中最突出的特征是：两极海冰之间相互作用的振源是ＮＰＩ２。ＳＰＩ３是影响南极海冰的正反馈中心。ＳＰＩ２则是南北两极海冰的负反馈中心。ＮＰＩ２，ＳＰＩ３和ＳＰＩ２之间的相互作用最强，形成涛动关系。这种涛动关系不是同时期的，而是有较长的滞后时间差。两极海冰形成周期变化，其周期为５－６年，正与ＮＰＩ２和ＳＰＩ３自身变化周期一致。另外还有更长的循环周期９－１１年     

1989年3月13日磁暴的亚极光区电离层效应

利用南极长城站（６２°１３′Ｓ，５８°５８′Ｗ）频高图和磁照图研究了１９８９年３月１３日磁暴的亚极光区电离层效应。在紧接着磁暴急始后Ｆ层的虚高ｈ′Ｆ急剧上升，临频ｆ０Ｆ２急剧下降，然后出现扩展Ｆ并持续几小时。在磁暴主相，电离层出现严重的吸收，但有时仍能观测到ｈ′Ｆ的增加和伴随着的ｆ０Ｆ２的降低。在磁暴急始后的第二和第三个晚上观测到极光型Ｅｓ和夜间Ｅ层，其峰值电子浓度高达７．５×１０５ｅｌ／ｃｍ３，文中讨论了造成这些现象的原因。在同一经度扇区的４个电离层站的ｈ′Ｆ和ｆ０Ｆ２的行为表明，观测站的纬度越高出现的吸收越严重，ｆ０Ｆ２呈下降的时间越长。     

1991／1992年夏季南极普里兹湾邻近海域网采浮游植物的聚类分析

本文报道了１９９１／１９９２年南极夏季在普里兹湾邻近海域浮游植物调查的研究结果。经鉴定共有浮游植物３门２６属７８种；其平均细胞丰度为１２０±１７４×１０＾５个／ｍ＾３，密集区分布在６２°Ｓ，７８°－１０３°Ｅ，这一海域其细胞丰度在１１０×１０＾５－８６４×１－１０＾５个／ｍ＾３之间。     

对流电场产生电离层扰动的典型事例

用欧空局ＥＩＳＣＡＴ极光区非相干散射雷达观测资料，南极中山站电离层垂测站和我国１３０°Ｅ电离层链ｆ０Ｆ２资料，分析了１９９１年５月２－３日一次主要由磁层对流引起的电离层扰动过程。从形态特征上看，它与热层中性大气参与动力耦合过程明显地不同。对照比较表明，这是一次典型的磁层－电离层电动耦合事例。     

对流电场产生电离层扰动的典型事例

用欧空局ＥＩＳＣＡＴ极光区非相干散射雷达观测资料、南极中山站电离层垂测站和我国１２０°Ｅ电离层站链ｆ０Ｆ２资料，分析了１９９１年５月２～３日一次主要由磁层对流引起的电离层扰动过程。从形态特征上看，它与热层中性大气参与的动力耦合过程明显地不同。对照比较表明，这是一次典型的磁层－电离层电动耦合事例。全球地磁站网资料从另一侧面证实，本文讨论的耦合机制是正确的。     

Preliminary result of imaging riometer at Zhongshan Station, Antarctica

１ＩｎｔｒｏｄｕｃｔｉｏｎＺｈｏｎｇｓｈａｎＳｔａｔｉｏｎ（７６°２２′Ｅ,６９°２２′Ｓ）ｏｆＡｎｔａｒｃｔｉｃａｉｓｌｏｃａｔｅｄｉｎａｎｉｄｅａｐｌａｃｅｆｏｒｏｂｓｅｒｖｉｎｇｓｏｌａｒ－ｔｅｒｅｓｔｒｉａｌｐｈｅｎｏｍｅｎａ．ＡｔＺｈｏｎｇ...     

Absolute gravity values in Norway

Absolute gravity observations yield insight into geophysical phenomena such as postglacial rebound, change in the Earth's hydrological cycle, sea level change, and changes in the Earth's cryosphere. In the article, the first gravity values at 16 Norwegian stations measured by a modern absolute gravimeter of the FG5 type are presented. The gravity observations were corrected for Earth tides, varying atmospheric pressure, polar motion, and ocean tide loading. The ocean tide loading corrections were subject to special attention. A model based on locally observed ocean tides was applied at some of the stations. The authors estimated the total uncertainties of the gravity values to range from 3 to 4 µgal (1 µgal = 10^?8 m s^?2). These errors are of magnitude one order less than previously presented absolute gravity values from Norway. The final gravity values are time tagged and will change due to postglacial rebound. The maximum effect is expected to be approximately ?1 µgal yr^?1.     

Tidal gravity variations revisited at Vostok Station, Antarctica

In 1969, prior to the discovery of the subglacial Lake Vostok, an Askania Gs-11 gravimeter was operated at Vostok Station (78.466°S, 106.832°E; 3478 m asl) to observe tidal gravity variations. To gain a better understanding of the lake's tidal dynamics, we reanalyzed these data using a Bayesian Tidal Analysis Program Grouping method (BAYTAP-G and -L programs). The obtained phase leads for the semidiurnal waves M2 (6.6 ± 2.1°) and S2 (10.1 ± 4.2°) are more pronounced than those of the diurnal waves, among which the largest phase lead (for K1) was 5.0 ± 0.5°. The obtained δ factor for M2 was 0.890 ± 0.032, significantly less than the theoretical value of 1.16. For three global ocean tide models (NAO99b, FES2004, and TPXO6.2), the estimated load tides on waves Q1, O1, P1, K1, M2, and S2 range from 0.1–0.2 μGal (Q1 and S2) to 0.6–0.7 μGal (K1). The difference in amplitude among the three models is less than 0.14 μGal (M2), and the difference in phase is generally less than 10°. In calculating the residual tide vectors using the ocean models, the TPXO6.2 model generally gave the smallest residual amplitudes. Our result for the K1 wave was anomalously large (1.36 ± 0.25 μGal), while that for the M2 wave was sufficiently small (0.37 ± 0.17 μGal). The associated uncertainty is half that reported in previous studies. It is interesting that the residual K1 tide is approximately 90° phase-leaded, while the M2 tide is approximately 180° phase-leaded (delayed). Importantly, a similar reanalysis of data collected at Asuka Station (71.5°S, 24.1°E) gave residual tides within 0.2–0.3 μGal for all major diurnal and semidiurnal waves, including the K1 wave. Therefore, the anomalous K1 residual tide observed at Vostok Station must be linked to the existence of the subglacial lake and the nature of solid–ice–water dynamics in the region.     

极地冰雪氢氧同位素指标及其指示意义

本文综述了水汽来源状况、降水季节变化、火山喷发、太阳活动等气候环境因素对极地冰雪中同位素含量的可能影响及其程度 ,以及降水区域不均衡性、降水年际不均衡性、逆温层和同位素在冰雪中的扩散迁移作用等几种不稳定因素可能对冰雪同位素分析造成的干扰 ;在此基础上 ,综述了极地冰雪中δ1 8O、δD和其差值d(d =δD - 8δ1 8O)与局部或全球气温之间的一些线性关系 (包括全球尺度 ,格陵兰地区 ,南极地区等 )及它们在空间分布上的变化规律     

南极长城站验潮站数据处理和潮汐特点初步分析

继在南极中山站建成我国南极首个永久性验潮站后,2012年1月在南极长城站又建成了我国南极第二个永久性验潮站。通过对长城站验潮站相关数据进行分析处理,得到了验潮基准系统的水准网平差结果和验潮仪零点标定结果,以及长城站附近海域海洋潮汐170个分潮的调和常数,并据此进行了潮汐预报,同时分析了长城站潮汐余水位的变化特征,探讨了利用附近的Antarctic Base Prat验潮站的余水位改正长城站潮汐预报的可行性,结果表明使用Antarctic Base Prat验潮站余水位改正长城站潮汐预报,可以显著提高长城站验潮站潮汐预报的精度,余水位改正后2014时段的潮汐预报中误差为±3.42 cm,明显好于改正前的预报中误差±10.43 cm。     

中国南极长城站测绘基准系统的建立

经1985年12月～1987年3月,三年度夏测绘科学考察,在中国南极长城站地区建立了一套完整的、精确的测绘基准系统。它包括大地坐标系统、高程系统和重力参考系统。本文叙述了建立这些基准系统的方法和数学模型,并分析了测量精度。     

Modelling the pole tide and its effect on the Earth's rotation

Summary. The pole tide is the response of the ocean to incremental centrifugal forces associated with the Chandler wobble. The tide has a potentially important effect on the period and damping of the wobble, but it is at present not well constrained by observations. Here, we construct both analytical and numerical models for the pole tide. The analytical models consider the tide first in a global ocean and then in an enclosed basin on a beta-plane. The results are found to approach equilibrium linearly with decreasing frequency and inversely with increasing basin depth. The numerical models solve Laplace's tidal equations over the world's oceans using realistic continental boundaries and bottom topography. The results indicate that the effects of the non-equilibrium portion of the deep ocean tide on the Chandler wobble period and damping are negligible.     

New aspects of the equilibrium pole tide

Summary. We have developed a new spherical harmonic algorithm for the calculation of the loading and self-gravitating equilibrium pole tide. Based on a suggestion of Dahlen, this approach minimizes the distortions in tide height caused by an incomplete representation of the ocean function. With slight modification our approach easily could be used to compute self-gravitating and loading luni-solar tides as well.
Using our algorithm we have compared the static pole tide with tide observations at a variety of locations around the world. We find statistically significant evidence for pole tide enhancements in mid-ocean as well as the shallow seas.
We have also re-investigated the effect of the static tide on the Chandler wobble period. The difference between the wobble period of an oceanless, elastic earth with a fluid core (Smith & Dahlen) and the period of an earth minus static oceans yields a 7.4-day discrepancy. We conclude from tide observations that much of the discrepancy can probably be accounted for by non-equilibrium pole tide behaviour in the deep oceans.     

Extraction of the M2 ocean tide from SEASAT altimeter data

Summary. Three complementary methods for the extraction of the M2 ocean tide using SEASAT altimetry are presented and compared. The first method (that developed by Cartwright & Alcock), which provides 'point measurements'of the tide at the crossovers of the SEASAT repeat orbit ground track, has been applied to a study of the tide in tropical ocean areas. The other two methods involve spatial expansions of M2 in terms of either surface spherical harmonics (in the case of the method developed by Mazzega) or Platzman normal modes of the world ocean. The results obtained by each method from only one month of SEASAT data reproduce many features of the tide represented in recent tidal models, and promise well for satellite altimetry as a future source of tidal knowledge.     

利用FG5绝对重力仪进行南极长城站绝对重力测定

在南极地区进行重力测量是建立高程基准的基础,2005年,在南极长城站进行了绝对重力测量,观测仪器采用FG5绝对重力仪,经固体潮改正、海潮改正、极移改正及气压改正等,精度达±3×10-8m s-2,并同时利用2台LCR相对重力仪进行了重力垂直梯度测量和水平梯度测量。长城站绝对重力测量的实施,对于新一代卫星重力计划如CHAMP、GRACE和GOCE的地面校准及建立南极地区的高精度、高分辨率的大地水准面模型提供了基础数据。     

The absolute gravity measurement by FG5 gravimeter at Great Wall Station,Antarctica

Gravity measurement is of great importance to the height datum in Antarctica.The absolute gravity measurement was carried out at Great Wall Station,Antarctica,using FG5 absolute gravity instrument.The gravity data was processed with corrections of earth tide,ocean tide,polar motion and the atmospher,and the RMS is within ±3×10-8 ms-2.The vertical and horizontal gravity gradients were measured using 2 LaCoaste & Romberg(LCR) gravimeters.The absolute gravity measurement provides the fundamental data for the validation and calibration of the satellite gravity projects such as CHAMP,GRACE and GOCE,and for the high accuracy geoid model.