94/220 GHz星载雷达双波长比对非球形冰晶云参数敏感性分析

利用不同形状冰晶的散射特性,获得了非球形冰晶云的94/220 GHz测云雷达双波长比,探讨了非球形冰晶云的双波长比与云内微物理参数的关系,分析了衰减前后的星载雷达反射率因子及双波长比的垂直廓线。结果表明:（1）双波长比可以反映小到0.1 mm中值尺度的冰粒子,对粒子总数、谱的形状参数不敏感,对粒子大小、形状、云衰减较敏感。（2）雷达灵敏度一定时,星载雷达可测云厚与雷达波长、冰含水量（IWC）的垂直分布、云厚及衰减有关;没有进行衰减订正时,双波长比和衰减有关,冰含水量越大,波长越短,衰减越大,双波长比最大值与可探测云厚有关。两部雷达可探测冰含水量为0.001—0.1 g/m3、厚2 km的冰云;当云厚5 km、冰含水量垂直分布在0.001—0.2 g/m3时,云厚的94%基本可以被220 GHz云雷达探测到。（3）如果两部雷达气象方程中用水的介电因子,测量回波强度应进行介电因子的订正后再计算双波长比。      

Effects of the number of stations and time resolution on derivation

For at least 30 years now it has been well known that the Dst index can be modelled using the solar wind as input. Since then, many attempts have been made to improve the predictability of Dst using different approaches. These attempts are useful, for instance, to understand which features of the solar wind–magnetosphere interactions are most important in producing magnetospheric activity and how the Dst index would improve the space weather forecast. The Dst index is by far the most reliable and simple indication that a magnetic storm is in progress. In this work, the effect of using more than four magnetic stations and shorter time intervals than the hourly averages used in Sugiura's procedures is evaluated. The discussion is based on the results presented by Burton in 1975 and Feldstein in 1984 considering 4 or 12 magnetic stations and time averages of 2.5 min for a magnetic disturbed period that occurred from February 7–28, 1967, including two geomagnetic storms. The analysis has shown that the global representation of a magnetic storm by the standard Dst (Sugiura) is well preserved either using 4, 6, 12 magnetic stations or using 1 h, 2.5 min 1 min averages. A brief review of the current understanding of Dst has been included to support the discussions. The analysis performed has shown that a more refined Dst index (time and number of stations>4) would be useful to investigate the intrinsic processes and the different current systems involved in the ring current development during magnetic storms; the standard Dst, as it is conceived, is quite adequate to monitor geomagnetic storms and identify their overall features; concerning the magnetic stations normally considered, the inclusion of higher magnetic latitude stations (>35) may underestimate the observed Dst.     

利用神经网络从118.75 GHz附近通道亮温反演大气温度

为了准确快速地从118.75 GHz附近六通道亮温计算大气温度,作者开展了利用人工神经网络技术反演大气温度的数值模拟研究。与线性统计反演算法比较,海面上大气温度反演的总体均方根误差减小17%,陆面上大气温度反演的总体均方根误差减小15%。两种下垫面条件下的温度反演结果表明,近陆面的温度反演结果优于近海面的温度反演结果。另外,对温度廓线垂直结构反演性能的分析结果表明,对于具有较厚逆温层结构的温度廓线,神经网络反演对廓线的复现能力优于线性统计反演。     

A new ultrasonic interferometer for the determination of equation of state parameters of sub-millimeter single crystals

A new giga-Hertz ultrasonic interferometer has been developed, based on ultrasonic microscopy technology. The interferometer operates from 0.3 GHz to 1.5 GHz. The high frequency and associated small wavelengths together with the large bandwidth make it possible to measure travel times in samples with thicknesses of several microns and allow for unprecedented accuracy in bond corrections. An absolute accuracy of 1 part in 10⁵ in travel time measurements is achievable in single crystals (thickness of 200 microns) or glasses of interest to the earth sciences. The high precision travel time data, combining with sample length measurements using a laser interferometer built in our laboratory, yield very high precision ultrasonic velocities.The interferometer is intended for use in conjunction with a newly developed 4 GPa gas piston cylinder apparatus (Getting andSpetzler, 1993) for equation of state measurements under simultaneous pressure and temperature. A separate correction for the bond will be made for each datum at every point in temperature pressure space.     

基于仿真的6.9 GHz通道亮温改进FY-3D MWRI海面温度产品

海洋表面温度SST（Sea Surface Temperature）是全球海洋和气候研究的重要参数之一,卫星被动微波遥感由于能够实现全天候观测而被越来越多的应用到SST研究中。中国的风云三号（FY 3）卫星搭载的微波成像仪（MWRI）缺少对SST更加敏感的7 GHz附近垂直极化通道,本研究将FY 3 MWRI与具有6.9 GHz通道的Aqua AMSR 2进行时空匹配,采用神经网络方法,利用匹配的FY 3 MWRI的通道亮温模拟仿真AMSR 2的69 GHz垂直极化通道亮温（6.9V）,通过引入仿真的6.9V来提高FY 3 MWRI SST的反演精度。结果表明：引入仿真的6.9V可以改进FY 3 MWRI SST反演精度,对35°～90°S之间海域的SST改进更加显著,主要由于6.9V对低SST的探测灵敏度更高且在低SST反演时受风速的影响较小导致的。如果FY3后续卫星可以搭载6.9 GHz通道,将可进一步提升低SST特别是两极SST的反演精度。     

Salt tectonics and Pliocene stratigraphic framework at MC-118, Gulf of Mexico: An integrated approach with application to deep-water confined structures in salt basins

Integrated tectono-stratigraphic interpretation at MC-118 using 3D seismic, well logs and biostratigraphy reveals an area dominated by allochthonous salt and its related structures. OCS-Block MC-118 is located 130 km southeast of New Orleans on the Gulf of Mexico middle slope in ∼2600 ft of water.The area is divided into three domains based on their structural styles: (1) a western domain consisting of a basinward-dipping normal fault family and associated strata; (2) a central domain composed of a landward-plunging diapiric salt tongue canopy and associated salt welds, two flanking NE–SW trending salt-withdrawal mini-basins, and a crestal fault family; and (3) an eastern domain comprised of basinward/landward-dipping normal and listric normal fault families with their associated rollovers. These structural domains are genetically-and-kinematically related to the salt structure and extend beyond MC-118 boundaries. The salt structure is postulated to have evolved mostly passive, with punctuated active episodes, and by lateral spreading. This is part of a larger regional structure, eastern Gulf of Mexico, which involves some amalgamation between small-scale salt canopies and salt diapirs although collectively they appear mostly disconnected.A Pliocene (3.13–4.95 Ma) third-order genetic stratigraphic sequence, the focus of this study, is as much as ∼3600 ft thick within the mini-basins and contains: muddy mass transport complexes; sandy slope fans; muddy turbidites and condensed sections; and transitional facies flanking the salt structure that collectively have ponded and wedged external geometries. Mass transport complexes and muddy turbidites and condensed sections make most of the studied genetic sequence in a mud-dominated deltaic setting eastern Gulf of Mexico.Facies kinematic indicators and a matching number of genetic sequences accounted on the sea level chart support a eustatically driven mini-basin sedimentation. Nonetheless salt still plays a role in sedimentation (secondary/minor) by slumping generated during passive/active salt diapiric evolution.     

对非球形冰晶94 GHz云雷达后向散射和衰减的研究

针对94 GHz毫米波云雷达的数据处理,基于离散偶极子近似法(DDA)计算了几种非球形冰晶的后向散射及衰减效率,探讨了不同冰云模型下冰云的雷达反射率因子(Z_e)和衰减系数(k)及冰水含量(IWC,记作W)的关系。结果表明:(1)形状对冰晶的散射及衰减效率与粒子大小有关。(2)在实际的冰云中,将六角形冰晶和椭圆冰晶看做同体积的球形粒子将低估其衰减和后向散射。将聚合物冰晶看做等体积球形,将高估其后向散射及衰减,子弹花冰晶的后向散射与同体积的球形相比有减小也有增大,但是衰减比同体积球形的小。(3)冰云模型对Z_e-k、Z_e-W关系具有较大影响,假设滴谱相同的条件下,得到了具体冰云模型下对应Z_e-k、Z_e-W关系的系数。这些探讨为我国W波段云雷达的数据处理提供了参考。     

95GHz云雷达对一次冷锋云系结构的观测分析

利用安徽寿县W-Band云雷达(95GHz,波长3.16mm)、地面微波辐射计、探空和地面观测等资料,对2008年11月5-7日一次冷锋云系的云结构进行了分析。结果表明,云雷达的多普勒速度可以初步确定粒子相态和大小以及是否存在雪晶或雨滴;在0℃层附近有回波暗带产生,这主要是由于波长为3mm的雷达对雪晶的衰减较强以及粒子的非Rayleigh散射引起的;云雷达观测可以清楚地识别混合云中的融化层。冷锋云系发展、演变过程及结构非常不均匀:锋面前部,在5～7km之间有一水凝物含量大值区,不断有长大的冰雪晶下落,使云底逐渐下伸,触地后产生间歇性阵性降水;降水过后,5km左右有一相对干层,上部为高层云,下部为散乱的多层云结构;冷锋临近,云层冷区没有水凝物含量大值区,回波强度较弱,暖区2km以下是干冷的东北气流,限制了雨滴通过暖雨过程增长,导致锋面降水强度较小,持续时间短。锋面后部4～7km高度,由于冰雪晶沉降,相对湿度较小,云层分裂成两层云;冷锋过后,出现了较强的降水,这主要是由暖雨过程产生的。     

94GHz云雷达回波及测云能力分析

重点利用英国的94 GHz Galileo测云雷达,结合35 GHz云雷达、地面雨滴谱仪、雨量计和探空资料等,分析了94 GHz 雷达的回波特征及测云能力。结果表明：（1）94 GHz云雷达能清楚反映出云及弱降水过程的云系结构变化和云内小尺度变化,可以探测到雾,雾的多普勒速度杂乱;（2）94 GHz云雷达区别于厘米波雷达的较显著的回波特征是层状云降水的0℃层亮带下面雷达反射率因子降低不明显或没有降低及0℃层亮带上面存在0℃层暗带,分别是因为雨滴较大及冰晶较大产生非瑞利散射引起的,暗带区域的宽度一般在600 m以下,暗带区域的许多冰晶聚合物最大尺度可超过3 mm,有些暗带区域的许多冰晶聚合物最大尺度可超过6.8 mm,多普勒速度及谱宽显著增大的地方是融化层顶;（3）与35 GHz测云雷达相比,由于衰减和非瑞利散射,降水时的94 GHz雷达反射率因子远小于35 GHz雷达反射率因子,使探测到的高云云顶高度偏低,但94 GHz云雷达抑制地物杂波的能力更高,在晴空低云探测方面具有优势。这些结果为中国正在研制的94 GHz云雷达回波可靠性分析提供了参考。94 GHz云雷达与其他探测手段结合,可揭示各种天气形成的物理机制,对天气预报、云物理的发展、人工影响天气、气候变化的研究均有重要意义。     

35GHz毫米波对生物离体皮肤组织表面辐照温升的研究

研究不同的功率密度35GHz毫米波对离体皮肤组织的辐照温升的问题。低功率辐照10min皮肤温度上升13.6℃;高功率辐照10s内,皮肤表面温升达10℃左右,皮肤的失水量较大。温升曲线和热传导方程计算结果做了对比,结果表明,低功率辐照下2mm厚样品的温升曲线和理论曲线较吻合,很显然,对于理论计算而言,35GHz毫米波辐照下2mm厚度以上的离体皮肤组织可以视为是半无限大的组织。聚焦的高功率毫米波的辐照温升与理论计算结果相比相差较大,文中对导致这种差异的可能原因进行了分析。