Effect of solar radiation and the subsequent dark periods on two newly isolated and characterized Antarctic marine bacteria

Two strains of psychrotolerant Antarctic marine bacteria were isolated and characterized using biochemical and molecular techniques. Sequencing of 16S rRNA gene showed that UVvi strain belongs to the genus Arthrobacter whereas UVps strain is related to the Flexibacter-Cytophaga-Bacteroides (FCB) group. Response of the strains to solar radiation was studied during the summer of 1999 in Potter Cove, near Jubany station (South Shetland Island, Antarctica). The effect of photosynthetically available radiation (PAR, 400-700 nm), ultraviolet-A (UV-A, 320-400 nm) and ultraviolet-B radiation (UV-B, 280-320 nm) on cell viability was studied using mixed cultures in quartz bottles covered with interferential filters and exposed to solar radiation. In all experiments, four treatments were used: dark (with light screened out), PAR (with UV radiation screened out), PAR+UV-A (UV-B screened out) and PAR+UV-A+UV-B. Under the assayed conditions, PAR+UV-A and PAR+UV-A+UV-B radiation showed similar negative effects on the viability of the studied strains. However, at the end of the exposure time, mortality values in PAR+UV-A+UV-B treatments were higher than those observed under PAR+UV-A treatments. In both PAR+UV-A and PAR+UV-A+UV-B treatments we observed high levels of hydrogen peroxide compared with the dark control. The Arthrobacter UVvi strain showed significant recovery in dark conditions after exposure to the PAR+UV-A but not after the PAR+UV-A+UV-B treatment. This strain proved to be more resistant to UV radiation than the FCB group-related UVps strain. The results showed that UV radiation has a deleterious effect on these Antarctic marine bacteria and also revealed that the analysed components of the Antarctic bacterioplankton may have different responses when they are exposed to the same irradiance conditions.     

MEASURED ALTITUDINAL PROFILES OF UV-B IRRADIANCE IN HAWAI'I

Erythemally weighted UV-B irradiance was measured between sea level and 4,205 m in several midday altitudinal transects and continuously for several months at sea level and 3,400 m on the Island of Hawai'i. Between sea level and 4,205 m, standardized UV-B increased 25% and 29% for solar zenith angles of 10° and 45°, respectively, under clear-sky conditions. The standardized diffuse component constituted 28% to 58% of the total as a function of optical path length. Under all sky conditions, the monthly average UV-B irradiance increased 50% in summer and 103% in winter from a cloudy, windward, sea-level location to a site at 3,400 m in generally clear skies above the trade-wind inversion. [Key words: solar radiation, ultraviolet-B irradiance, Hawai'i.]     

Physical properties, spectral reflectance and thickness development of first year fast ice in Kongsfjorden, Svalbard

A ground truth study was performed on first year fast ice in Kongsfjorden, Svalbard, during spring 1997 and 1998. The survey included sea ice thickness monitoring as well as observation of surface albedo, attenuation of optical radiation in the ice, physical properties and texture of snow and sea ice. The average total sea ice thickness in May was about 0.9 m, including a 0.2 m thick snow layer on top. Within a few weeks in both years, the snow melted almost completely, whereas the ice thickness decreased by not more than 0.05 m. During spring, the lower part of the snow refroze into a solid layer. The sea ice became more porous. Temperatures in the sea ice increased and the measurable salinity of the sea ice decreased with time. Due to snow cover thinning and snow grain growth, maximum surface albedo decreased from 0.96 to 0.74. Texture analysis on cores showed columnar ice with large crystals (max. crystal lenght > 0.1 m) below a 0.11 m thick mixed surface layer of granular ice with smaller crystals. In both years, we observed sea ice algae at the bottom part of the ice. This layer has a significant effect on the radiation transmissivity.     

利用北冰洋多光谱数据计算光合有效辐射的研究

光合有效辐射（PAR）是重要的生物光学量,与海洋浮游植物的初级生产过程有密切联系。PAR通常由单波段的PAR传感器直接测量,也可以由多光谱数据计算。在极区用多光谱数据计算PAR不仅面对不同谱宽度的问题,而且还有海冰的影响。本文研究了4种可能导致PAR计算误差的主要因素。多光谱仪器避开了大气对太阳辐射的主要吸收带,用多光谱数据计算会对PAR高估。实测数据分析表明多光谱计算的PAR与高光谱数据的计算结果非常接近,误差在1%以内。用本文建立的拟合函数进行校正,校正后的结果与高光谱数据计算的结果达到同样的精度。计算PAR的衰减率要用到进入海水表面的PAR（PAR0）,本文提出先确定表层衰减系数,再通过最小二乘拟合确定PAR0值,与水下观测数据有很好的衔接。海上同一站位不同时间的观测数据计算的PAR衰减系数相差很小,表明PAR的衰减系数是海水的光学性质,与辐射强度无关。在海冰覆盖的条件下,PAR的观测结果与无冰海水的PAR有明显差别。由于海冰选择性的吸收,穿透海冰进入海洋的PAR组分已经不同,海水对PAR的衰减系数也会相应变化。由此可以推断,不同海冰中成分的差别将导致进入海水中PAR的差别,影响PAR的衰减特性。通过本文的研究,解决了在极区用多光谱计算PAR的各种问题,使多光谱数据成为PAR的重要数据源。     

Vertical migration as a response to UVR stress in Calanus finmarchicus females and nauplii

We conducted laboratory experiments to study the behavioural responses of Calanus finmarchicus females and nauplii exposed to artificial ultraviolet radiation (UVR) and photosynthetically active radiation (PAR). Both nauplii and females migrated downwards when exposed to UVR. Nauplii reacted mainly to UV-B radiation, while females responded also to UV-A. Nauplii were also collected in the field to check if vertical distributions supported the experimental findings. Light measurements in Vestfjorden showed that plankton were exposed to quite low doses of UVR most of the time. However, on days with a thin ozone layer, clear sky and low turbidity UV-B doses in the surface waters might be harmful. Strong turbulence in the surface layer prevents nauplii from adjusting their position, exposing them to fluctuating levels of UVR due to vertical mixing. Under calm conditions, however, copepods could migrate sufficiently to avoid harmful UVR doses.     

Penetration of ultraviolet B, blue and quanta irradiance into Svalbard waters

Observations from August 1991 and 1993 of downward UV-B, blue and quanta irradiances, and of colour indices and Secchi disc depths in the Greenland Sea and the northern part of the Barents Sea, are presented. The UV-B irradiance (306 nm) is on average reduced to 10% of its surface value at 5 metres depth, and to 1% at 10 m. Blue irradiance (465 nm) is reduced to 10% at 21 m, and to 1% at 41 m. The integrated quanta irradiance obtains the same reductions at 16 m and 35 m, respectively. These penetration depths correspond to Ocean Water Type III in Jerlov's classification. They are about twice the values of May-June 1973 observed by Aas & Berge, but they are half the values observed in September 1979 by Højerslev. This variability may partly be seasonal, caused by the hydrological and light-climate cycles. The UV-B transparency of the Svalbard waters seems to be influenced by yellow substance from different freshwater run-offs, and there is probably no single relation between salinity and yellow substance content in this region. Statistical relations between the quanta irradiance and the colour index, the Secchi disc depth and the blue irradiance differ from one region to another, and from year to year.     

太阳直接辐射光量子通量的气候学计算方法

为了把太阳直接辐射通量密度换算成光量子通量密度,取用了一个简单的大气模式,计算了各种太阳高度、地面气压和大气浑浊度下太阳直接辐射中的光合有效辐射能量通量和光量子通量,从而得到了单位光合有效辐射能量所具有的光量子数。结果表明:这个数是比较稳定的。在平原地区,10—90°的太阳高度范围内,1W.m~(-2)的光合有效辐射通量密度具有4.72±0.11μmol.m~(-2).s~(-1)的光量子通量密度。本文还采用北京地区四个季节定时的太阳直接辐射分光测量资料和高原观测资料检验了模式计算结果的可靠性,获得了满意的结果。     

2013-2014年夏季南极普里兹湾海面反照率走航观测研究

在 2013—2014年南半球夏季时对南极普里兹湾海区的反照率进行了走航观测。利用安装于破冰船船头的高光谱辐照度计测量入射和反射的350—920 nm的太阳短波辐射, 基于此观测数据, 经计算得到了反照率。分析比较不同下垫面的反照率, 通过比较不同航段的观测结果, 得到了反照率的空间变化以及从海冰融化期至冻结初期的变化。不同下垫面的反照率差异较大, 有积雪覆盖的固定冰反照率最大, 有积雪覆盖的浮冰其次, 而积雪融化的浮冰则反照率有所降低。新冰的反照率较低, 有积雪覆盖的新冰反照率迅速增加。比较不同波段的反照率, 发现融化期由于积雪含水量较大, 增加了对近红外辐射的吸收, 降低了该波段的反照率。结合卫星遥感(AMSR-2)和人工观测的海冰密集度, 发现区域平均的反照率主要取决于海冰密集度, 然而也受下垫面物理特征影响, 例如2月底至3月初形成的新冰, 反照率只有老冰的1/3— 1/2。新冰形成, 会直接增加海冰密集度, 但由于其反照率较低, 对空间平均反照率的贡献较小。因此, 若要建立合理的冰水混合区的反照率参数化方案, 必须充分考虑海冰类型和冰面积雪的物理状态, 并考虑反照率的波长依赖性。     

Photosynthetic responses of selected Antarctic plants to solar radiation in the southern maritime Antarctic

The effects of UV-B exclusion and enhancement of solar radiation on photosynthesis of the two phanerogams which occur in the maritime Antarctic, Deschampsia antarctica and Colobanthus quitensis , and the moss Sanionia uncinats were investigated. Data on air temperature and solar radiation illustrate a drastic seasonal variation. Daily O₃ column mean values and UV-B measured at ground level document the occurrence of the O₃"hole" in the spring of 1997, with a concomitant increase in UV-B. The grass, D. antarctica , exhibited a broad temperature optimum for photosynthesis between 10–25°C while photosynthesis did not saturate even at high irradiance. The high water use efficiencies measured in the grass may be one of the features explaining the presence of this species in the maritime Antarctic. The net photosynthesis response to intercellular CO₂ (A/c_i) for D. antarctica was typical of a C₃ plant. Exposure to a biologically effective UV-B irradiance of 0.74 W M^-2 did not result in any significant change in either the maximum rate of photosynthesis at saturating CO₂ and light, or in the initial carboxylation efficiency of Rubisco. (V_c,max). Furthermore while ambient (or enhanced) solar UV-B did not affect photochemical yield, measured in the field, of C. quitensis and D. antarctica , UV-B enhancement did affect negatively photochemical yield in S. uncinata . In D. antarctica plants, exposure to UV-B at low irradiances elicited increased flavonoid synthesis. The observed effects of UV-B enhancement on the moss (decreased photochemical yield) and the grass (increase in flavonoids) require further, separate investigation.     

北冰洋78°N冰站近地层参数的观测研究

利用2003年8月22日-9月3日中国北极科学考察队在北冰洋78°N浮冰站获得的近地层观测资料,采用整体输送法对北冰洋浮冰近地层特征参数进行了分析研究。结果表明,在考察期间,雪面吸收的净辐射仅为3.6 W/m2,其中以感热和潜热向大气输送的能量分别占52%和31%,向海冰深层传导的热量很少;近中性层结条件下的平均拖曳系数Cdn为1.16×10-3,略小于75°N北冰洋浮冰上近中性层结的Cdn。与1999年75°N附近冰站观测结果的对比表明,当海冰密度及冰站所在浮冰的尺度不同时,海冰与大气相互作用的热力学和动力学过程的差异显著,在研究北冰洋地区海/冰/气相互作用对气候过程影响时,应考虑这一问题。     

Experiment of near surface layer parameters in ice camp over Arctic Ocean

Estimates of near surface layer parameters over 78°N drifting ice in ice camp over the Arctic ocean are made using bulk transfer methods with the data from the experiments operated by the Chinese Arctic Scientific Expedition in August 22-September 3,2003.The results show that the net radiation received by the snow surface is only 3.6 W/m2,among which the main part transported into atmosphere in term of sensible heat and latent heat,which account for 52% and 31% respectively,and less part being transported to deep ice in the conductive process.The bulk transfer coefficient of momentum is about 1.16×10-3 in the near neutral layer,which is a little smaller than that obtained over 75°N drifting ice.However,to compare with the results observed over 75°N drifting ice over the Arctic Ocean in 1999,it can be found that the thermodynamic and momentum of interactions between sea and air are significant different with latitudes,concentration and the scale of sea ice.It is very important on considering the effect of sea-air-ice interaction over the Arctic Ocean when studying climate modeling.     

Present status and variations in the Arctic energy balance

The total solar irradiance (TSI, or solar constant) acquired a new value: 1361 W m^?2 instead of 1365 W m^?2. However a long-term variation of TSI was not detected. The solar irradiance at the earth's surface is considerably smaller (170 W m^?2) than previously believed (e.g. 198 W m^?2 of IPCC AR4). The previous overestimation is due to the underestimation of the absorption of solar radiation in the atmosphere. The absorption of solar radiation in the atmosphere at about 90 W m^?2, or 25–28% of the primary solar radiation from space. The global mean atmospheric downward terrestrial radiation is much larger (345 W m^?2) than previously assumed (325 W m^?2 of IPCC AR4). The Arctic has regions of negative annual net radiation, a very rare phenomenon on the globe. These regions are the Central Arctic Ocean with its multi-year ice coverage and the accumulation area of the Greenland ice sheet. The energy balance of these regions is presented. Long-wave incoming radiation has been increasing in the Arctic at a rate of 4–5 W m^?2/Decade. The Greenland ice sheet exhibits a large vertical difference in net radiation from the ablation area to the dry snow zone in summer. It ranges from 80 W m^?2 in the ablation area to 20 W m^?2 at the equilibrium line and to 10 W m^?2 in the dry snow zone. This gradient determines the melt gradient on the ice sheet, and is mainly caused by the altitude variation in atmospheric long-wave radiation, seconded by the albedo variation. The effect of albedo in summer for various surfaces is discussed. Simulation capabilities of radiation for many GCMs are investigated.     

Diel tuning of photosynthetic systems in ice algae at Saroma-ko Lagoon, Hokkaido, Japan

Ice algae are the major primary producers in seasonally ice-covered oceans during the cold season. Diurnal change in solar radiation is inevitable for ice algae, even beneath seasonal sea ice in lower-latitude regions. In this work, we focused on the photosynthetic response of ice algae under diurnally changing irradiance in Saroma-ko Lagoon, Japan. Photosynthetic properties were assessed by pulse-amplitude modulation (PAM) fluorometry. The species composition remained almost the same throughout the investigation. The maximum electron transport rate (rETR_max), which indicates the capacity of photosynthetic electron transport, increased from sunrise until around noon and decreased toward sunset, with no sign of the afternoon depression commonly observed in other photosynthetic organisms. The level of non-photochemical quenching, which indicates photoprotection activity by dissipating excess light energy via thermal processes, changed with diurnal variations in irradiance. The pigment composition appeared constant, except for xanthophyll cycle pigments, which changed irrespective of irradiance. These results indicate that ice algae tune their photosynthetic system harmonically to achieve efficient photosynthesis under diurnally changing irradiance, while avoiding damage to photosystems. This regulation system may be essential for productive photosynthesis in ice algae.     

Ground－based measurements of column abundance of ozone and UV－B radiation over Zhongshan Station，Antarctica in the 1993＂OzoneHole＂

Ｇｒｏｕｎｄ－ｂａｓｅｄｍｅａｓｕｒｅｍｅｎｔｓｏｆｃｏｌｕｍｎａｂｕｎｄａｎｃｅｏｆｏｚｏｎｅａｎｄＵＶ－ＢｒａｄｉａｔｉｏｎｏｖｅｒＺｈｏｎｇｓｈａｎＳｔａｔｉｏｎ,Ａｎｔａｒｃｔｉｃａｉｎｔｈｅ１９９３＂ＯｚｏｎｅＨｏｌｅ＂ＺｈｏｕＸｉｕｊｉ（...     

南极罗斯海2012年夏季海冰特征分析

利用卫星海冰密集度资料和船基海冰走航观测数据分析了2012年12月至2013年3月南极罗斯海海冰密集度、厚度和浮冰尺寸等参数的时空变化特征。12月下旬罗斯海西侧浮冰区南北向宽约1 000 km,沿雪龙船航线平均密集度在5成以上,平均海冰厚度为100 cm,平均冰上积雪厚度为16 cm,高密集度区域主要为尺寸较小的块浮冰(2—20 m)和小浮冰(20—100 m),低密集度区域主要为大尺寸浮冰(500—2 000 m)。1月和2月罗斯海大部分海域无海冰覆盖,3月海冰迅速冻结,下旬即覆盖整个罗斯海。SSMIS和AMSR2两种卫星遥感数据均能较好反映航线上的真实海冰密集度状况,AMSR2产品与观测符合更好。与1978—2012的气候平均值相比,观测区在2012年夏季冰情偏重。本文的分析结果可帮助我们了解罗斯海海冰的时空特征,为中国后续罗斯海科考提供参考。     

Physical properties and stratigraphy of surface snow in western Dronning Maud Land, Antarctica

Information about the spatial variations of snow properties and of annual accumulation on ice sheets is important if we are to understand the results obtained from ice cores, satellite remote sensing data and changes in climate patterns. The layer structure and spatial variations of physical properties of surface snow in western Dronning Maud Land were analysed during the austral summers 1999/2000, 2000/01 and 2003/04 in five different snow zones. The measurements were performed in shallow (1–2 m) snow pits along a transect extending 350 km from the seaward edge of the ice shelf to the polar plateau. These pits covered at least the last annual accumulation and ranged in elevation from near sea level to 2500 m a.s.l. The ع⁸O values and accumulation rates had a good linear correlation with the distance from the coast. The mean accumulation on the ice shelf was 312±28 mm water equivalent (w.e.); in the coastal region it was 215±43 mm w.e. and on the polar plateau it was 92±25 mm w.e. The mean annual conductivity and grain size values decreased exponentially with increasing distance from the ice edge, by 48%/100 km and 18%/100 km respectively. The mean grain size varied between 1.5 and 1.8 mm. Depth hoar layers were a common phenomenon, especially under thin ice crusts, and were associated with low dielectric constant values.     

2010年夏季北极海冰反照率的观测研究

雪和海冰作为北极地区反照率最高的地表类型,可以将大部分入射辐射能量反射回天空,其表面反照率的变化对整个地表-大气辐射平衡系统和全球气候变化都会有重要影响。在2010年中国第4次北极科学考察期间用ASD光谱仪对北极太平洋扇区不同类型的海冰表面反照率进行了现场测量,观测时段为7月27日至8月23日,地理范围在72°18′-87°20′N和152°34′-178°22′W之间。观测结果表明积雪覆盖海冰的反照率最高,干雪覆盖时均值达到0.82,融化的湿雪覆盖时反照率会有一定程度地降低。夏季北极地区存在大量融池,融池海冰按颜色划分为白冰,蓝冰和灰冰,白冰的平均反照率为0.54,蓝冰的为0.31,灰冰的只有0.20,融池水的反照率只有0.16。融池是北极夏季反照率变化的重要原因。     

南极威德尔海周边雪冰和大气气溶胶中的MSA,nssSO_4~(2-)浓度及其比率研究

分析了威德尔海周边雪冰和大气中ＭＳＡ和ｎｓｓＳＯ２－４浓度资料。结果表明,威德尔海是造成这一地区大气中高含量生物硫化物的“源”,其周边岛屿及冰架表层雪冰记载和反映了大气中生物硫化物的空间分布和季节变化特点。源区产出硫化物的强度存在显著差异：靠近南极半岛一侧高于靠近Ｆｉｌｃｈｎｅｒ－Ｒｏｎｎｅ冰架一侧。尽管诸多因素对输运和沉降过程发生影响,表层积雪ＭＳＡ和ｎｓＳＯ２－４浓度仍呈现出很有规律性的空间分布：随沉降地点离海距离和海拔高度的增加,浓度值递减;但在一定海拔之下,“高程效应”不显著。冰芯中ＭＳＡ浓度垂向分布显示出季节分配“滞后”现象,在表层表现为受天气条件制约的输运过程造成的相位差,在深层则归因于有待验证的“迁移”机制作用的结果。大气和雪冰样品对比研究结果表明,在类似威德尔海这样的高纬地区,大气中的ＳＯ２－４和ＭＳＡ“信号”在雪冰样品中会遭到不同程度的减弱。但就空间变化趋势和季节分布而言,表层雪冰仍是大气中组分（在本文是ＳＯ２－４和ＭＳＡ）的良好载体。十分接近的大气和雪冰ＭＳＡ对ｎｓｓＳＯ２－４（或ＳＯ２－４）比率证实,这两种大气组分在由大气洗净和沉降到冰雪过程中只发生微弱的分离作用。这也就是大气和雪冰中     

南极威尔克斯地SGR钻孔处雪冰转化过程中的密度变化特征

本文着重描述了SGR钻孔处冰盖上的积雪在密实化过程中的特征变化,并对该过程进行了分段的和全面的回归分析.结果表明,冰盖密度随深度增大,但增长幅度随深度减小.作者提出密度变化减小度的概念.计算得出的所研究冰芯钻取点的密度变化减小度为-0.15kg/m~3·m~2,粒雪成冰前的密实速率平均值为4.08kg/m~3·a.本文得到的冰盖密度变化“临界点”与以往报道的有所不同.分析这一现象时,作者强调当积雪还在活动层时冰盖温度的影响,并以此解释密度剖面的异常变化以及离差的回升.特别指出,积雪的密度变化具有气候学意义,它在一定程度上能够反映出积雪形成及变化过程中气候变化的某些信息.本文由密度变化确定的钻孔点雪冰转化深度为50米.     

Spaceborne Microwave Remote Sensing of Arctic Sea Ice During Spring

This paper outlines the fundamental roles sea ice plays during the spring Arctic climate, and it demonstrates the use of passive microwave remote sensing in measuring climatically important sea ice variables during the spring transitional period. It discusses the theoretical concepts underlying passive microwave remote sensing of sea ice, and it summarizes the historical use of satellite microwave radiometry in the Arctic region. In addition, this paper discusses the derivation of climatically important sea ice variables, including sea ice extent, concentration, multiyear ice fraction, and snow melt onset, with additional comments on the precision and accuracy of the remote sensing estimates. It also discusses interannual trends in sea ice extent and presents interannual trends in snow melt onset dates. Finally, this paper provides a brief discussion on the future directions in passive microwave remote sensing of climatically important sea ice variables during the spring transitional period.