导致甘肃输电线路舞动的蒙古气旋的形成及增风机理研究（英文）

受一次向东南方向移动蒙古气旋强风的影响,2020年4月18日甘肃省白银市的高压输电线路出现了严重的舞动,这造成了该地区的输电线路跳闸事故.基于0.5度逐小时分辨率的ERA5再分析数据,本文研究了这次蒙古气旋及其强风的形成机理.涡度收支的结果表明,辐合相关的垂直伸展以及垂直运动向上的正涡度输送是本次蒙古气旋形成的主因,而倾斜项的负涡度制造以及从气旋中心区域向外的正涡度输送在一定程度上不利于蒙古气旋的形成.动能收支的结果表明,蒙古气旋所伴随的风场主要由于气压梯度力的做功而迅速增强.与我国西北部其它的典型强风事件不同的是在本次事件中,未发现显著的来自于对流层高层的动量下传现象,垂直的动能输送在本次事件中仅对强风的形成有些许的促进作用.此外,水平风场对动能的输送作用使得蒙古气旋大风区的动能存在向外的净输出,这对蒙古气旋强风的生成有一定的延缓作用.     

气旋快速发展的机制分析

本文主要分析爆发性气旋的形成机制。通过对一个爆发性气旋生成的个例分析表明,高空急流核的东传及高空强风动量的下传加强了低层强风带及气旋性涡度切变;涡度及位涡垂直分布显示,以对流层中高层的强涡度为背景,气旋在中低层得以爆发性发展,使得强盛期的气旋发展成为一个上下一致的垂直涡度柱;低空强风带的加强一方面由于高空急流的动力强迫作用,另一方面来源于低纬空气质点对强风动量的输送作用。另外,本文还利用拉格朗日方法进行空气质点的轨迹积分,以分析高空纬向气流及低层强风带的变化及输送作用。     

登陆台风Matsa (麦莎) 中尺度扰动特征分析

地面中尺度自动站和多普勒雷达资料的分析都表明, 台风Matsa登陆后的低层螺旋云带中活跃着中尺度气旋性涡旋系统。本文使用新一代中尺度WRF模式对台风Matsa登陆后的变化特征进行了数值模拟, 使用四维变分多普勒雷达分析系统 (4D-VDRAS) 对台风Matsa多普勒雷达径向风进行了风场反演。在此基础上对台风Matsa登陆后中尺度扰动特性进行了初步探讨; 对台风Matsa与其螺旋云带的中尺度系统之间动能和涡度的相互转换进行了诊断分析。分析表明: (1) 数值模拟和雷达风场反演结果表明, 登陆台风Matsa的低层螺旋云带中活跃着中尺度气旋式涡旋系统, 与之相伴随的为较强的中尺度上升区, 而且, 中尺度垂直上升运动的强弱与雷达对流回波强度成正相关, 中尺度垂直上升运动越强, 雷达对流回波发展越旺盛。 (2) 台风Matsa与其中尺度系统动能转换的诊断分析说明, 低层中尺度系统从台风Matsa环流中获得动能而发展; Matsa在陆地上长久维持主要是从高层获得动能。 (3) 台风Matsa与其中尺度系统涡度转换的诊断分析说明, 低层中尺度系统向Matsa输送正涡度主要依靠中尺度垂直运动来完成; 高层正涡度的转换通过水平输送和垂直输送共同来完成。所以, 中尺度系统所产生的正涡度源源不断地向Matsa输送, 使Matsa的气旋性环流可以在陆地上长久维持。     

热带气旋登陆维持和迅速消亡的诊断研究

采用动态合成方法, 对登陆后长久维持热带气旋(LTC)和迅速衰亡热带气旋(STC)的涡度、动能、热量和水汽的收支平衡进行计算和对比分析.结果表明: (1)LTC在陆上长久维持过程中, 其低层正涡度衰减缓慢并保持一定强度.STC登陆后正涡度减弱较快.(2)热带气旋登陆后涡度的收支主要取决于水平散度项、平流项和剩余项.散度项使LTC低层正涡度增加, 高层减少, 平流项和剩余项则使其低层涡度减弱, 高层涡度增加.总体而言, LTC自高层获得正涡度的补充, STC则没有获得环境正涡度.(3)低层, 摩擦耗散使LTC动能减少, 但动能通量辐合可补充部分动能而减缓衰减.中高层, LTC登陆后36～60 h动能收大于支, 动能的增加一部分来自于斜压动能制造, 一部分来自于次网格尺度.STC有类似的动能耗散, 却无动能补充.(4)LTC登陆后保持一定强度, 并从外界获得热量和水汽补充来支持积云对流发展, 而积云对流对LTC的维持具有正反馈作用.STC登陆后没有这一过程.     

梅雨锋上引发暴雨的低压动力学研究

对1998年"二度梅"结束前后长江中下游地区准静止锋上一次气旋发生发展过程进行了涡度收支的诊断分析.结果表明:(1)风场(尤其是辐散风场)对该气旋发生发展有重要影响;(2)低层辐合场是直接决定气旋发生发展的动力因子,它导致低层正涡度制造,对气旋的发展起直接作用;(3)涡度平流上正下负的配置和水汽凝结潜热释放,通过影响上升运动及低层辐合对地面气旋的发展起间接作用.在系列研究工作的基础上,提出了梅雨锋上第二类气旋(低压)的概念模型.     

由台风低压倒槽引发的山东暴雨过程研究

2004年8月26-28日发生在山东省的大到暴雨过程主要是由"艾莉"台风减弱的低压和西风带冷空气远距离相互作用造成的,台风倒槽的发展与低空东南气流的加强及台风低压外围热量和动量的向北输送密切相关.采用双向三重嵌套网格非静力模式MM5对这一过程进行了数值模拟,研究了台风倒槽的中尺度结构特征,并通过涡度收支探讨了台风倒槽及中尺度低涡发生发展的物理过程.结果表明,强降水是在台风倒槽顶部强风中心与弱风中心之间的强辐合作用下触发的,台风倒槽的增强和中尺度低涡的形成是低空急流及其动力作用的结果,降水的非绝热加热也起着重要作用.涡度方程的收支诊断表明,对流层低层的散度项、对流层中层的水平平流项和铅直输送项是正涡度的主要贡献者,在同一等压面上散度项和水平平流项的作用是相反的.对流层中层铅直输送项的贡献为正,扭转项为负贡献,涡度变化的总趋势是它们相互作用的净结果.等压面上相对涡度的变化趋势并不是均匀的,中尺度低涡的东南象限相对涡度局地变化较强,这是强降水发生在此的重要原因.低层正涡度的增加是由水平辐合引起的,而高层正涡度的增加是涡度由低层向高层垂直输送的结果.因此台风倒槽的发展和中尺度低涡的形成主要是由于低层的涡度制造,另一方面来自中低层涡度的垂直输送.     

2017年1月上旬泰国南部暴雨反复发生机制的研究

基于0.25°×0.25°的CMORPH日降水量产品以及ECMWF 0.25°×0.25°的ERA5再分析数据,本文对2017年1月上旬泰国南部反复发生暴雨事件的机制进行了研究,这些暴雨事件造成了Ko Samui和Ko Phangan近三十多年来最强的洪水事件。结果表明,初生于中南半岛西南方,向东北方向移动的一个中尺度涡旋是泰国南部重复发生暴雨事件的直接原因。涡度收支分析表明,水平辐合项是这个中尺度涡旋维持的最有利因子,倾斜项是第二有利的因子,而水平和垂直输送则主要造成了涡旋三维空间范围内正涡度向外的净输出,这是不利于涡旋维持的。进一步的分析表明,倾斜项与垂直涡度输送项分别对涡旋的移动及涡旋周边对流层低层的涡度增长较为敏感,这两个作用项在涡旋维持的两个不同阶段内各自表现出了完全不同的作用。     

2017年1月上旬泰国南部暴雨反复发生机制的研究（英文）

基于0.25°×0.25°的CMORPH日降水量产品以及ECMWF 0.25°×0.25°的ERA5再分析数据,本文对2017年1月上旬泰国南部反复发生暴雨事件的机制进行了研究,这些暴雨事件造成了Ko Samui和Ko Phangan近三十多年来最强的洪水事件。结果表明,初生于中南半岛西南方,向东北方向移动的一个中尺度涡旋是泰国南部重复发生暴雨事件的直接原因。涡度收支分析表明,水平辐合项是这个中尺度涡旋维持的最有利因子,倾斜项是第二有利的因子,而水平和垂直输送则主要造成了涡旋三维空间范围内正涡度向外的净输出,这是不利于涡旋维持的。进一步的分析表明,倾斜项与垂直涡度输送项分别对涡旋的移动及涡旋周边对流层低层的涡度增长较为敏感,这两个作用项在涡旋维持的两个不同阶段内各自表现出了完全不同的作用。     

一次典型蒙古气旋沙尘暴的对流层顶演变及沙尘垂直输送特征

利用高分辨率中尺度数值模拟结果,对一次蒙古气旋沙尘暴过程的对流层顶折叠和沙尘对流层-平流层输送特征进行分析研究。结果发现:本次过程蒙古气旋的发展由对流层中低层斜压强迫引发,对流层中高层高空位涡下传是蒙古气旋发展的另一影响因素。蒙古气旋发展阶段,对流层中高层为低压槽,对流层顶折叠呈漏斗状;随着蒙古气旋的成熟及高空切断低涡的形成,对流层顶折叠变为双漏斗状,位置偏于低涡区南侧,分别位于低槽槽线中段和低涡中心附近。之后的气旋减弱阶段,对流层顶折叠逐渐与低涡区趋于重合。高空急流位于漏斗状对流层顶折叠区南支附近,当对流层顶折叠加强时,高空急流核向下拉伸,反之,高空急流核则趋于水平。对流层顶折叠呈漏斗状的气旋发展阶段,对流层-平流层输送气流位于漏斗东侧、北侧,即气旋暖区螺旋上升气流,位置越偏东、偏北,输送气流的强度和范围越大;气旋成熟阶段,对流层顶折叠呈双漏斗状(经向)和平直带状(纬向),低涡中心附近的准垂直上升气流、低涡中心以东的低涡区偏南上升气流、以及低涡前部槽前强上升气流均产生明显的对流层-平流层输送。气旋减弱阶段,偏南上升气流、准垂直上升气流导致的对流层-平流层输送明显减弱,低涡东北象限偏东气流则能够形成不可逆的对流层-平流层输送。     

东北低压爆发性发展过程的诊断分析

本文对一次东北低压的快速强烈发展过程做了扰动动能、扰动有效位能及涡度收支平衡分析。结果表明:1.气旋爆发性发展前后,扰动动能的产生项变化剧烈,是主要的扰动动能源。气旋爆发性发展前期,以斜压过程为主,而在爆发期,由正压过程制造的扰动动能也有大量增加,同样是不可忽视的,且这时扰动动能通过系统边界与外界的交换很小。2.扰动有效位能在气旋强烈发展前有大幅度增长,由潜热释放造成的扰动有效位能的产生数值很小,平均有效位能向扰动有效位能的转换是扰动有效位能的主要来源。3.在气旋的爆发期,对流层中层及上层的涡度变化最为显著,涡度平衡中,散度项对对流层中下层正涡度的增长贡献最大,而网格尺度及次网格尺度的垂直输送项和涡度平流项对中上层正涡度的迅速增加有着重要意义。     

On the formation and wind enhancement mechanisms of a Mongolian cyclone that caused a transmission line galloping trip in Gansu province: 导致甘肃输电线路舞动的蒙古气旋的形成及增风机理研究

Influenced by strong winds associated with a southeastward-moving Mongolian cyclone, a severe transmission line galloping occurred in Baiyin City, Gansu Province, on 14 April 2020. This caused a tripping incident of the transmission line in this region. Based on the hourly, 0.5°  ×  0.5°, ECMWF ERA5 reanalysis data, this study investigated the formation mechanisms of the Mongolian cyclone and its associated strong winds. Results from the vorticity budget indicate that the convergence-related vertical stretching and the upward transport of cyclonic vorticity governed formation of the Mongolian cyclone in this event; whereas, tilting and export of cyclonic vorticity from the central region of the cyclone mainly decelerated the cyclone's formation. The kinetic energy (KE) budget shows that the wind associated with the Mongolian cyclone was mainly enhanced by the positive work of the pressure gradient force. Unlike some typical strong wind events in Northwest China, during this event, no significant downward momentum transportation from the upper troposphere was found. The vertical transport of KE exerted a slightly favorable effect on the KE increase around the location where the transmission line galloping trip appeared. In contrast, the horizontal transport mainly caused an export of KE from this region, which applied an overall negative effect on the wind enhancement associated with the Mongolian cyclone.摘要受一次向东南方向移动蒙古气旋强风的影响, 2020年4月18日甘肃省白银市的高压输电线路出现了严重的舞动, 这造成了该地区的输电线路跳闸事故.基于0.5度逐小时分辨率的ERA5再分析数据, 本文研究了这次蒙古气旋及其强风的形成机理.涡度收支的结果表明, 辐合相关的垂直伸展以及垂直运动向上的正涡度输送是本次蒙古气旋形成的主因, 而倾斜项的负涡度制造以及从气旋中心区域向外的正涡度输送在一定程度上不利于蒙古气旋的形成.动能收支的结果表明, 蒙古气旋所伴随的风场主要由于气压梯度力的做功而迅速增强.与我国西北部其它的典型强风事件不同的是在本次事件中, 未发现显著的来自于对流层高层的动量下传现象, 垂直的动能输送在本次事件中仅对强风的形成有些许的促进作用.此外, 水平风场对动能的输送作用使得蒙古气旋大风区的动能存在向外的净输出, 这对蒙古气旋强风的生成有一定的延缓作用.     

Simulation of formation of a near-equatorial typhoon Vamei (2001)

Summary A community mesoscale model is used to simulate and understand processes that led to the formation and intensification of the near-equatorial typhoon Vamei that formed in the South China Sea in December, 2001. The simulated typhoon resembles the observed in that it had a short lifetime and a small size, formed near the equator (south of 2° N), and reached category-one intensity. The formation involved the interactions between the scales of the background cyclonic circulation (the Borneo Vortex of order ∼100 km) and of mesoscale convective vortices (MCVs, in the order ∼10 km). Before tropical cyclone formation MCVs formed along a convergent, horizontal shear vorticity line on the eastern edge of an exceptionally strong monsoonal northerly wind surge. The typhoon genesis is marked by three rapid intensification periods, which are associated with the rapid growth of potential vorticity (PV). A vorticity budget analysis reveals that the increases in low-level vorticity during the rapid intensification periods are attributed to enhanced horizontal vorticity fluxes into the storm core. The increase of the horizontal vorticity flux is associated with the merging of areas of high PV associated with MCVs into the storm core as they are advected by background cyclonic flows. The increases in PV at upper levels are associated with the evaporation of upper level stratiform precipitation and increases of vertical potential temperature gradient below the maximum stratiform cloud layer. It appears that two key sources of PV at upper and lower levels are crucial for the build up of high PV and a deepening of a cyclonic layer throughout the troposphere.     

A Case Study on MJO Energy Transport Path in a Local Multi-scale Interaction Framework

A new local kinetic energy (KE) budget for the Madden-Julian Oscillation (MJO) is constructed in a multi-scale framework. This energy budget framework allows us to analyze the local energy conversion processes of the MJO with the high-frequency disturbances and the low-frequency background state. The KE budget analysis is applied to a pronounced MJO event during the DYNAMO field campaign to investigate the KE transport path of the MJO. The work done by the pressure gradient force and the conversion of available potential energy at the MJO scale are the two dominant processes that affect the MJO KE tendency. The MJO winds transport MJO KE into the MJO convection region in the lower troposphere while it is transported away from the MJO convection region in the upper troposphere. The energy cascade process is relatively weak, but the interaction between high-frequency disturbances and the MJO plays an important role in maintaining the high-frequency disturbances within the MJO convection. The MJO KE mainly converts to interaction KE between MJO and high-frequency disturbances over the area where the MJO zonal wind is strong. This interaction KE over the MJO convection region is enhanced through its flux convergence and further transport KE to the high-frequency disturbances. This process is conducive to maintaining the MJO convection. This study highlights the importance of KE interaction between the MJO and the high-frequency disturbances in maintaining the MJO convection.     

Mechanisms governing the evolution of a long-lived northwest vortex that caused a series of disasters in Northwest China

西北涡是我国西北地区一类发生频率较高的中尺度涡旋,其所引发灾害的强度与西南低涡,高原涡相当,但相关研究却远远少于前两种涡旋.为了深化对西北涡的认识,本文利用水汽与环流收支对一次长生命史西北涡(其在西北地区引发了一系列暴雨过程,导致了严重的输电线路故障与城市内涝)进行了研究,发现,东海与渤海是此西北涡引发暴雨的主要水汽来...     

A Study on a Heavy Rainfall Event Triggered by an Inverted Typhoon Trough in Shandong Province

A heavy rainfall event that occurred in Shandong Province in 26 28 August 2004 was caused mainly by Typhoon Acre and cold air activities related to a westerly trough. The event was triggered by an inverted typhoon trough, which was closely associated with the intensification of the low-level southeasterly flow and the northward transport of heat and momentum in the periphery of the typhoon low. A numerical simulation of this event is performed using the nonhydrostatic mesoscale model MM5 with two-way interactive and triply-nested grids, and the structure of the inverted typhoon trough is studied. Furthermore, the formation and development mechanism of the inverted typhoon trough and a mesoscale vortex are discussed through a vorticity budget analysis. The results show that the heavy rainfall was induced by the strong convergence between the strong and weak winds within the inverted typhoon trough. Dynamic effects of the low-level jet and the diabatic heating of precipitation played an important role in the development of the inverted typhoon trough and the formation of the mesoscale vortex. The vorticity budget analysis suggests that the divergence term in the low troposphere, the horizontal advection term, and the convection term in the middle troposphere were main contributors to positive vorticity. Nonetheless, at the same pressure level, the effect of the divergence term and that of the adveetion term were opposite to each other. In the middle troposphere, the vertical transport term made a positive contribution while the tilting term made a negative contribution, and the total vorticity tendency was the net result of their counteractions. It is found that the change tendency of the relative vorticity was not uniform horizontally. A strong positive vorticity tendency occurred in the southeast of the mesoscale vortex, which is why the heavy rainfall was concentrated there. The increase of positive vorticity in the low （upper） troposphere was caused by horizontal convergence （upward transport of vorticity from the lower troposphere）. Therefore, the development of the inverted typhoon trough and the formation of the mesoscale vortex were mainly attributed to the vorticity generated in the low troposphere, and also the vertical transport of vorticity from the low and middle troposphere.     

Study of the structure of a monsoon depression over the Bay of Bengal during Summer MONEX

Based on the data gathered during the Summer MONEX over the Bay of Bengal in July, 1979, a detailed observational study of the structure of a monsoon depression during the period of 3-8, July has been made. It has been revealed that the early disturbance of this depression was a mid-tropospheric cyclone. The subsequent rapid development was due mainly to the barotropic instability process of the basic zonal and meridional airflows.The cyclonic circulation of the depression extended in vertical upward to 500-400 mb level. Prior to the formation of the depression, the extremely strong westerly and northerly winds at the lower and middle levels, reaching the intensity of the low-level jet (22 m/s and 18.5 m/s, respectively), were observed. Post to the formation of the depression, a strong wind ring at the radius of 300-350 km from the depression center encircled the depression, with the wind maximum being at 850 mb. During this period, the maximum of the positive vorticity was of the magnitude of order of 10-4/s. The warm core at 400-300 mb was very remarkable. Finally, intrusion of the dry air over the depression may be an important factor leading to the weakening of the depression.     

一次华南强飑线过程的数值模拟及后方入流作用诊断

利用WRF中尺度模式对2014年3月30—31日发生在华南的一次强飑线过程进行数值模拟。本次飑线过程受高空槽和低涡切变线影响,水汽条件充足,低层垂直风切变较强。模拟结果表明:发展阶段,后方入流缺口开始出现,飑线逐渐呈弓形结构;成熟阶段,飑线后方入流逐渐下沉到地面并延伸至对流区前沿,冷池完全移入残留冷区并加强,配合九连山下坡过程,飑线得以加强。后方入流对本次飑线过程的发展和维持十分重要。后方入流受环境风及中层负压力扰动作用开始形成,随后受对流区后侧中低层涡旋对的影响迅速发展增强而进入发展阶段,反气旋式涡旋的北侧风场促进了后方入流的形成和发展;成熟阶段,气旋式涡旋的南侧风场使后方入流迅速增强。气旋式涡旋区域主要受涡管拉伸作用增长,反气旋式涡旋区主要受涡度倾斜增长作用。涡旋对垂直涡度主要是由低层水平涡度向上倾斜引起,而水平涡度则是由斜压作用产生。     

一次热带气旋减弱远离后出现暴雨的成因分析

利用常规气象资料、加密气象站观测资料、NCEP的1°×1。分析资料以及多普勒雷达资料,对2011年6月12日热带气旋减弱远离后广东发生的一次暴雨过程进行了诊断分析。结果表明：（1）地而辐合、低空切变、中层气旋式环流和高空辐散的共同作用导致了此次的暴雨过程;（2）垂直上升运动在强降水发生前即有明显反映,中低层正涡度、高层负涡度的配置也有利于上升运动的维持和强降水的发生;（3）前期不稳定能量的累积是必要条件,而K、SI指数在维持高度不稳定的条件下,其24h变化量对此次暴雨的发生有一定的提前指示意义;（4）中尺度切变、辐合对强降水的发生时间和落区移动都有较好的指示作用．中低层乖盲风切蛮增大有利于风暴的发展。     

东北冷涡下一次飑线和MCV的形成与水平涡度的关系

利用WRF中尺度数值模式,NCEP/NCAR分析资料,多普勒雷达观测资料等,对2016年7月25日一次东北冷涡下的飑线过程进行数值模拟,研究了飑线形成和维持与水平涡度的关系及飑线过程中中尺度对流涡旋(MCV)的形成机制,分析发现,高低层水平涡度逆时针旋转对本次飑线的形成和维持有很好的指示意义。(1)飑线发生前,高层渤海湾西侧出现水平涡度的逆时针旋转中心,并有较强的辐散配合,低层水平涡度为逆时针弯曲,为飑线产生提供了有利的上升运动条件。随后高层多个对流单体的水平涡度气旋式涡旋合并形成较大范围的气旋式涡旋结构,触发低层的上升运动,同时低层对流区前部形成一致的气旋式弯曲使得对流单体组织成带状结构,形成飑线。(2)飑线成熟时期高层水平涡度表现为统一大范围气旋式涡旋结构,低层则呈现典型的S型弯曲结构,水平涡度x方向的分量沿对流带从南至北表现为正负正,y方向的分量始终为正,并由对流带的中心向两侧减小,显示出水平涡度矢量旋转的方向对飑线影响的重要性。(3)由垂直涡度方程的分析得出,在飑线发展中期,MCV形成前,雷达反射率回波在500 hPa左右表现出明显的旋转,此时主要与500 hPa以上强的正涡度水平平流项及中层倾侧项和水平散度项有关,之后,在这几项的作用下使得中层风场产生气旋式旋转,形成MCV。      

IMPACT OF AIR-SEA INTERACTION ON THE GENESIS OF TROPICAL INCIPIENT VORTEX OVER SOUTH CHINA SEA: A CASE STUDY

Based on 6-hourly sensible heat flux and latent heat flux from the NCEP Climate Forecast System Reanalysis (CFSR) and circulation data from the Japanese 25-year Reanalysis (JRA-25), the initial developing process of tropical cyclone Mindulle (1005) in 2010 has been diagnosed to reveal the impact of air-sea interaction over the South China Sea (SCS) on the genesis of its incipient vortex. The results show that the incipient vortex first occurred east of the Luzon Island on 0000 UTC 20 August, suggesting that the topographic forcing of the Luzon Island for easterly winds over the western Pacific might be one of the factors responsible for the formation of the incipient vortex. During the formation stage of the incipient vortex, strong southeasterlies over the SCS caused warm water of the middle and eastern SCS to flow toward the Luzon Island due to Ekman transport resulting from wind stress, leading to an increase of the sea surface temperature and sensible heat flux into the atmosphere. Although the anomalous sensible heating favored surface pressure to reduce, it was not conducive to the increase of local vorticity associated with the vortex above the heating area because, according to the atmospheric thermal adaptation theory, the anticyclonic vorticity would be created in the lower troposphere due to the decreased vertical gradient of the sensible heating. However, the ascending motions occurred over the eastern area of the anomalous sensible heating due to the augmentation of the vorticity advection with increasing height, causing water vapor to condense in the middle and upper troposphere. In turn, cyclonic vorticity was generated in the lower troposphere due to the increased vertical gradient of the condensation latent heating, resulting in the formation and further growth of the incipient vortex. Therefore, the vorticity creation due to the condensation heating played a dominant role during the subsequent enhancing stage of the incipient vortex.