Solar Activity and Algal-bloom Occurrences in the Northern Adriatic Sea: Geomagnetic Connection

Summary The high-speed particle flux (solar wind) escaping from the Sun controls the geomagnetic activity at middle latitudes. The latter is found to be negatively correlated to the difference of atmospheric pressure between January and April averaged out in the area of the Northern Adriatic. This difference is again related to the water volume flowing from the South into the Northern Adriatic Sea and is a necessary (though not sufficient) condition for the occurrence of strong algal-blooms in summer. A physical model involving geomagnetic activity, mean atmospheric pressured difference between latitude 35 °N and 55 °N in the European area and atmospheric pressure difference from winter to spring in the Northern Adriatic basin is proposed. The possibility of predicting the long-term variations of geomagnetic activity allows one to obtain long-term predictions of winter minus spring pressure and therefore indications of the risk of strong summer-time algal-bloom episodes. Received March 29, 1996 Revised February 14, 1997     

A high resolution AMIP integration using the Hadley Centre model HadAM2b

 A high resolution (0.833° latitude by 1.25° longitude) AMIP (Atmospheric Model Intercomparison Project) integration is compared with a control integration at standard resolution (2.5° by 3.75°). Both integrations use HadAM2b, a recent version of the Hadley Centre atmospheric general circulation model. ECMWF reanalysis data for the AMIP period (1979–1988), together with other climatologies, are used to evaluate the results. An additional integration at standard resolution using the high resolution shorter time step is used to help distinguish between changes due to model resolution and those which are due to time step dependencies in the physical parametrizations. Enhanced resolution increases the vertical motion, intensifies the hydrological cycle, reduces slightly the model’s cold bias in the troposphere, shifts the westerly jets poleward and tends to increase the eddy kinetic energy and variability of the model. The high resolution simulation has less mid-latitude cloud, so altering the radiation balance. There is no evidence to suggest that increasing resolution has an impact on the model’s response to SST forcing. Received: 7 October 1997 / Accepted: 16 June 1998     

A steady two-dimensional climate model with residual circulation

Based on dynamical energy transport and thermodynamic energy balance in the earth’s atmosphere-ocean system a steady two-dimensional climate model with residual circulation is proposed. In the model, we include some important physical processes with feedbacks such as ice caps-albedo, water vapor-tempera-ture, etc. The simulated steady temperature field is very close to that of the real atmosphere. The numerical experiments show that doubling of the atmospheric carbon dioxide results in temperature increase of 1~2oC at the low latitude surface and 6~8oC at the high latitude surface. It is shown that a 6% decrease in the solar constant is required for the -10oC ice edge to move from its present latitude ~70o to~50o.     

Association among geomagnetic activity,atmospheric electric field and selected meteorological parameters

The association among the geomagnetic activity (Ap index) and atmospheric electric field, meteorological parameters was investigated using a long series of continuous data set available for Colaba (18o53’N, 72o48’E, 11m ASL) for the period 1936-1966. The meteorological parameters used for the investigation are the surface pressure, temperature, wind velocity and relative humidity. The results of the above study indicate that the atmospheric electric field and the meteorological parameters are associated with the geomagnetic storms with Ap > 100. The atmospheric electric field shows an increasing trend after the geomagnetic storm. The surface pressure dips and surface tempera-tures increase after a geomagnetic storm. The wind velocity shows a decreasing trend and the relative humidity shows an increasing trend after the geomagnetic storm.     

The 60-year solar modulation of global air temperature: the Earth’s rotation and atmospheric circulation connection

Summary Spectral analysis of geomagnetic activity, global air temperature, Earth’s rotation rate and zonal circulation, when smoothed from secular trend and periods shorter than 23 years, shows a concentration of energy around the 60-year period explaining more than 80% of the entire variance. This information has enabled the set-up of a cascade physical model that integrates the Sun-atmosphere-Earth system as a single unit and ties solar corpuscular radiation to global warming through Earth’s rotation and atmospheric circulation. Our results suggest that changes in geomagnetic activity, and in the Earth’s rotation, could be used as long- and short-term indicators, respectively, of future changes in global air temperature.     

2009年和2010年夏季我国及周边地区STE模拟与对比分析

夏季是深对流多发的季节,深对流在STE(Stratosphere Troposphere Exchange,对流层-平流层交换)过程中起着重要作用。对2005-2012年夏季我国及周边地区的深对流统计发现,2009年深对流发生的次数较少,2010年深对流发生的次数较多。通过拉格朗日输送模式对2009年和2010年夏季的大气运动状态进行模拟并统计分析,发现30°N以南和以北的地区具有明显不同的平流层-对流层交换特征,30°N以北我国及周边地区TST(Troposphere to Stratosphere Transport,对流层向平流层输送)和STT(Stratosphere to Troposphere Transport,平流层向对流层输送)较为活跃,30°N以南远没有30°N以北地区活跃,但其净输送量却大致相当。在30°N以南,6-8月净输送是对流层向平流层输送。在30°N以北,6月净输送是平流层向对流层输送,7-8月净输送是对流层向平流层输送。比较深对流出现较少的2009年夏季和深对流出现较多的2010年夏季的TST和TST-STT,发现2010年6-8月这3个月的TST和TST-STT总量都超过2009年,表明2010年夏季我国及周边地区对流层向平流层的输送和净输送都强于2009年,与深对流活动的多少可能表现出正相关。     

Seasonal variations of gravity waves revealed in rawinsonde data at Pohang,Korea

Summary Seasonal variations of gravity wave characteristics are investigated using rawinsonde data observed at Pohang observatory, Korea (36°2′N, 129°23′E) during the one-year period of 1998. Analysis is carried out for two atmospheric layers representing the troposphere (2–9 km) and stratosphere (17–30 km). There exist clear seasonal variations in amplitudes of temperature and wind perturbations and wave energy in the stratosphere, with their maxima in wintertime and minima in summertime. A strong correlation is found between the wave activity and the strength of the jet stream, but there is no clear correlation between the wave activity and the vertical gradient of static stability. The intrinsic frequency and vertical and horizontal wavelengths of gravity waves in the stratosphere are 2f–3f, where f is the Coriolis parameter, and 2–3 km and 300–500 km, respectively. The intrinsic phase velocity directs westward in January and northeastward in July. The vertical flux of the stratospheric zonal momentum is mostly negative except in summertime with a maximum magnitude in January. Topography seems to be a major source of stratospheric gravity waves in wintertime. Convection can be a source of gravity waves in summertime, but it is required to know convective sources at nearby stations, due to their intermittency and locations relative to floating balloons.     

Apposite of atmospheric electric parameters with the energy coupling function (ε) during geomagnetic storms at high latitude

In this paper we are concerned with the variation of the atmospheric electric field and the air–earth current due to the excessive power generated by the solar wind-magnetosphere dynamo during geomagnetic storms, recorded at Maitri in Antarctica during 2004. A major part of the power generated by the solar wind-magnetosphere dynamo is used in the formation of the ring current and the rest is utilized for Joule heating and auroral particle precipitation. The method adopted by Frank-Kamenetsky et al. [Frank-Kamenetsky A.V., Troshichev O.A., Burns G.B., Papitashvili V.O., 2001. Variations of atmospheric electric field in the near-pole region related to the interplanetary magnetic field. J. Geophys. Res. 106, A1, 179–190.] was utilized to delineate the variations due to the signatures of tropical thunderstorm activity from the geoelectric data; while statistical methods used in our earlier studies were used to delimit variation due to the constant buffeting of the solar wind. We find that the solar wind-magnetosphere energy coupling function (ε) to be well correlated with the atmospheric electric parameters during the onset of geomagnetic disturbances. However the correlation breaks down during minor storms and sub-storm events.     

Lunar phases and atmospheric electric field

The association between the lunar phases and the atmospheric electric field has been investigated from the superposed epoch analysis of the lone series of continuous data of the vertical electric field for Colaba, Bombay (18o53’N, 73o48’E 11 mASL) for the period 1947-1966. Also the periodicities in the atmospheric electric field have been studied from the spectral analysis of the data. The study has indicated that when the full moon is within 4o of the ecliptic plane i. e., Bf 4o, the electric field peaks on the day of the full moon followed by a steep fall in the field val-ues up to 4 days following the full moon day and there after it showed a steep increase. Also, the electric field has exhibited 5-9 day periodicity and its multiples are nearly always present. The periodicity in the electric field corresponds with the average time interval between the successive magnetic sector boundary (MSB) crossings i.e., 7 days. On most of the occasions, the MSB crossing day is associated with a maximum of one or more of the wavelengths derived from the spectral analysis of the atmospheric electric field.     

Potential of occultation atmospheric sounding using an extended radiation source

A possibility is considered of measuring the ozone in the upper atmosphere of the Earth using solar occultation sounding without mechanical scanning of the solar disk. The estimates are given of the error and vertical resolution of atmospheric transmission function profile retrieved from the solar radiation measurements carried out by the instrument with the field of view of more than 0.5°. These algorithm elements are computed using the Backus-Gilbert method. It is shown that using the measurements in UV spectrum region carried out in this way, it is possible to retrieve transmission functions with the vertical resolution of 3–4 km and error of not more than 0.003.     

强对流天气对O3和CO的垂直输送作用

利用ACTIVE（aerosol and chemical transport in tropical convection）试验资料,取2006年1月20日澳大利亚北部达尔文岛附近发生的一次飑线强对流天气的AE17航次和2006年1月27日无对流天气的AE21航次飞行路径中的探测资料,对澳大利亚达尔文地区夏季风盛行期间发生的有无强对流发生时O₃和CO浓度垂直分布变化进行对比,考察强对流性天气发生对O₃和CO浓度垂直输送作用。深对流云内强烈的垂直上升运动将O₃和CO等化学气体携带输送至对流层上部并在对流层顶堆积,从而在对流层上部产生浓度峰值。当有强对流发生,飞机进入对流云上层时,O₃浓度和CO浓度升高,O₃和CO浓度变率增大,在对流层上部浓度出现峰值;当飞机飞出对流云时,O₃和CO浓度相对较低,在对流云外出现谷值。在无对流发生的条件下O₃和CO浓度相对较小,浓度变率也较小,无峰值产生。分析表明:O₃和CO浓度分布不仅与强对流的垂直输送作用关系密切,且与气象要素垂直和水平分布以及动力输送过程密切相关。     

The effect of mountainous topography on moisture exchange between the “surface” and the free atmosphere

Typical numerical weather and climate prediction models apply parameterizations to describe the subgrid-scale exchange of moisture, heat and momentum between the surface and the free atmosphere. To a large degree, the underlying assumptions are based on empirical knowledge obtained from measurements in the atmospheric boundary layer over flat and homogeneous topography. It is, however, still unclear what happens if the topography is complex and steep. Not only is the applicability of classical turbulence schemes questionable in principle over such terrain, but mountains additionally induce vertical fluxes on the meso-γ scale. Examples are thermally or mechanically driven valley winds, which are neither resolved nor parameterized by climate models but nevertheless contribute to vertical exchange. Attempts to quantify these processes and to evaluate their impact on climate simulations have so far been scarce. Here, results from a case study in the Riviera Valley in southern Switzerland are presented. In previous work, measurements from the MAP-Riviera field campaign have been used to evaluate and configure a high-resolution large-eddy simulation code (ARPS). This model is here applied with a horizontal grid spacing of 350 m to detect and quantify the relevant exchange processes between the valley atmosphere (i.e. the ground “surface” in a coarse model) and the free atmosphere aloft. As an example, vertical export of moisture is evaluated for three fair-weather summer days. The simulations show that moisture exchange with the free atmosphere is indeed no longer governed by turbulent motions alone. Other mechanisms become important, such as mass export due to topographic narrowing or the interaction of thermally driven cross-valley circulations. Under certain atmospheric conditions, these topographical-related mechanisms exceed the “classical” turbulent contributions a coarse model would see by several times. The study shows that conventional subgrid-scale parameterizations can indeed be far off from reality if applied over complex topography, and that large-eddy simulations could provide a helpful tool for their improvement.     

珠穆朗玛峰北坡局地环流日变化的观测研究

青藏高原地-气间的物质/能量交换是高原与全球大气系统相联系的重要纽带.陡峭的地形和强烈的地表差异在高原山区形成特殊的局地大气环流系统,在地气交换中起着重要作用.为研究珠峰北坡的局地环流系统,于2006年5～6月间在珠峰北坡绒布河谷实施强化观测实验HEST2006,对该地区的局地环流以及辐射和热力状况进行观测,分析了该地区局地环流的日变化过程,包括:(1)地面风场的分布和变化;(2)风场垂直结构;(3)垂直运动及可能的驱动机制.研究表明,该地区局地大气环流是由地形与地表状态调整的大气辐射加热和冷却所驱动,包含多种不同的山地环流成分,与典型山谷风环流不同,具有很强的特殊性,对地气问的交换有重要影响.     

西宁夏季对流层臭氧垂直分布变化与气象要素的关系

根据臭氧、气象探空观测数据,分析了1996年7月5日至8月3日西宁（36°44’N,101°45＇E,海拔高度2296m）上空对流层臭氧垂直分布变化与气象要素之间的关系。对流层臭氧浓度的增加（减少）总伴随着干、冷（暖、湿）气流的输送变化,而这又与大气垂直方向的运动是紧密联系在一起的。分析表明天气动力输送过程对对流层臭氧垂直分布变化有重要作用。     

Molecular Line Parameters for the “MASTER” (Millimeter Wave Acquisitions for Stratosphere/Troposphere Exchange Research) Database

In order to investigate the upper troposphere/lower stratosphere (UTLS) region of the earth's atmosphere, ESA/ESTEC (European space agency) is considering the opportunity to develop the spaceborne limb sounding millimeter sensor “MASTER” (millimeter wave acquisitions for stratosphere/troposphere exchange research). This instrument is part of the “atmospheric composition explorer for chemistry and climate interactions” (ACECHEM) project. In addition, ESA/ESTEC is developing the “MARSCHALS” (millimeter-wave airborne receiver for spectroscopic characterization of atmospheric limb sounding) airborne instrument which will demonstrate the feasibility of MASTER. The present paper describes the line-by-line database which was generated in order to meet at best the needs of the MASTER (or MARSCHALS) instrument. The linelist involves line positions, line intensities, line broadening and line shift parameters in the 294–305, 316–325, 342–348, 497–506 and 624–626 GHz spectral microwindows. This database was first generated for the target molecules for MASTER (H₂O, O₃, N₂O, CO, O₂, HNO₃, HCl, ClO, CH₃Cl, BrO). In addition, ten additional molecules (SO₂, NO₂, OCS, H₂CO, HOCl, HCN, H₂O₂, COF₂, HO₂ and HOBr) had also to be considered in the database as “possible interfering species” for the retrieval of the target molecules of MASTER. The line parameters were derived, depending on their estimated accuracy, (i) from a combination of spectral parameters included in the JPL and HITRAN catalogs (ii) from data taken into the literature or (iii) using data obtained through experimental measurements (and/or) calculations performed during the present study.     

Seasonal variations in the vertical structure of water vapor optical depth in the lower troposphere over a tropical station

Spatio-temporal variations of water vapor optical depth in the lower troposphere (450-3850 m) over Punt (18o32’N, 73o51’E, 559 m Above Mean Sea Level), India have been studied over a period of five years. The mean ver-tical structure showed that the moisture content is greatest at the lowest level and decreases with increasing altitude, except in the south-west monsoon season (June to September) where an increase upto 950 m has been found. Optical depths are maximum in the monsoon season. The increase from pre-monsoon (March-May) to monsoon season in moisture content on an average is by about 58% in the above altitude range. The temporal variations in surface Rela-tive Humidity and optical depth at 450 m show positive correlation. The amplitude of seasonal oscillation is the larg-est at 1465 m altitude. The time-height cross-sections of water vapor optical depths in the lower troposphere showed a contrast between years of good and bad monsoon.     

台湾地形对台风Meranti(1010)经过海峡地区时迅速增强的影响研究

台风在趋近大陆过程中强度一般衰减, 但Meranti(1010)北上进入台湾海峡过程中却迅速加强, 且在登陆福建时达到最强。采用中国气象局台风资料、NCEP GFS 0.5°×0.5°再分析资料及台湾雷达资料, 结合中尺度数值模式WRF(The Weather Research and Forecasting Model)开展台湾地形敏感性试验, 研究Meranti进入台湾海峡过程中的结构变化及迅速加强机理。结果表明:台湾地形是Meranti迅速加强的一个重要影响因子。Meranti北上过程中, 一方面通过台湾岛地形分流作用及其背风坡效应在台湾海峡内诱生中尺度涡旋, 形成正负相间的涡度分布, 激发出与台风相关的扰动波列。地形强迫抬升及扰动波列可加强垂直运动和积云对流, 有利于台风对流发展。另一方面, 台湾地形还通过改变环境气流使台风高空辐散场加强, 环境风垂直切变减小, 形成有利于台风发展的环流背景。比较不同高度台湾地形试验中台风动能收支发现, 台湾地形激发的扰动波列和积云对流增强了次网格尺度系统与台风间能量的交换, 成为Meranti登陆前迅速加强的主要动能源。     

西北太平洋近赤道热带气旋生成的特征分析

1979—2012年西北太平洋存在70个形成于0°～5°N的低纬度地区的热带气旋(TC),占TC总量的8%,其中达到台风等级的个数占64%。而针对此类缺少一定科氏力作用而形成的罕见TC生成的研究相对较少。本文利用JTWC的TC最佳观测资料、ERA-Interim再分析资料,以及NOAA-OISST海温资料,以西北太平洋近赤道TC为研究对象,统计诊断了其年际、年代际、季节分布特征,分析了其大尺度环境背景场,重点探讨了近赤道TC生成的影响因子。研究结果表明,近赤道TC具有明显的年际与年代际变化,并且近赤道TC具有与西北太平洋总TC恰好相反的季节变化。近赤道TC生成的大尺度环境背景场是东北冬季风与其在近赤道地区偏转形成的西北风之间的气旋性环流。对流层低层的绝对涡度动力项与对流层中层的湿度热量项是近赤道TC生成的主要贡献因子,并且相对于5°～10°N生成的TC,近赤道TC对对流层低层的正涡度与对流层中层的湿度条件的要求更高。     

全球变暖背景下青藏高原夏季气温在对流层上下反相变化及其与降水和环流的关系

本文利用NCEP/NCAR月平均再分析资料及中国596个测站月降水资料,采用线性倾向估计、经验正交函数分解(EOF)、相关分析、合成分析等方法,对青藏高原夏季对流层气温垂直变化及其与降水和环流的关系进行了分析。气温垂直变化特征分析表明:自1971年以来,青藏高原夏季对流层低层至对流层中上部气温呈现显著增暖趋势,对流层上部气温呈现显著变冷趋势,高原对流层低层至中上部气温及对流层上部气温在年际、年代际尺度上均呈较显著负相关,且均存在2~4 a及8~13 a的周期;夏季青藏高原地区沿27.5°N~40°N平均的气温距平垂直分布的EOF分解第一模态特征向量在对流层表现为"下降温上增温"的反相变化,其时间系数呈显著负趋势,且存在1978年及1994年的突变点。高原夏季气温在对流层的上下反相变化与我国夏季降水的关系在年际、年代际尺度上均显示:当高原对流层低层至对流层中上部升温而对流层上部降温时,我国夏季降水表现为南方型,其中以江南至华南地区降水显著偏多而我国东北地区降水显著偏少为主要分布特征;另外,长江流域的局部地区及我国西北的部分地区降水也明显偏少,而华北东部的局部地区、青藏高原中部及东部地区以及新疆西北部地区降水明显偏多;降水异常分布在年代际尺度上比年际尺度更显著。环流分析显示:当高原对流层低层至对流层中上部升温而对流层上部降温时东亚中高纬度地区为异常高压控制,中低纬度地区受异常低压影响。环流场与降水分布有较好的配置关系。     

雷暴闪电放电活动对电离层影响的研究进展

雷暴中的闪电放电能够产生强静电场以及电磁辐射场,从而对空间电离层产生重要影响,引起电离层电子密度分布的扰动。研究表明:闪电放电引起电离层扰动的方式有两种:直接耦合和间接耦合。其中,直接耦合主要来自于闪电产生的准静电场及电磁场的作用,在甚低频 (VLF) 反射信号上表现出快VLF事件, 而间接耦合主要是闪电低频电磁波在传播过程中与磁层相互作用,在辐射带产生闪电诱导电子沉降 (LEP) 现象。雷暴闪电活动能够改变电离层从D层到F层的电子密度分布,影响对流层大气和电离层之间的场,导致中高层瞬态放电淘气精灵 (elves) 及红闪 (sprite) 等现象的激发。闪电VLF传输反射信号可用于反演电离层密度的变化,目前已成为一种探测电离层扰动的常用方法,而引起电离层扰动的强度不但和闪电放电参量密切相关,也和闪电放电过程、类型有关。该文重点阐述了闪电放电与电离层直接耦合和间接耦合作用以及导致的相关现象。