利用机载GNSS反射信号反演海面风速的研究

全球卫星导航定位系统的反射信号(GNSS-R)遥感技术作为一种新型的、低成本的、高机动性的海面微波遥感测风技术,与其他测风手段优势互补,可以增加测风手段的多样性,弥补局部测风手段不足的状况。研究了接收机在机载高度时,GPS反射信号功率理论模型四部分函数的性质,在此基础之上,数值模拟了机载高度下理论相关功率波形,基于海面风速对波形峰值与后沿的影响,提出了一种能够兼顾所有理论波形信息的二维插值风速反演方法。利用该方法,结合实测机载数据对海面风速进行反演,反演的风速均值与附近测站风速均值相差为1.4 m/s,与浮标数据相一致。     

基于多源数据的湘北地区春季一次冰雹过程的观测分析

新型探测资料在强对流短临预报中发挥着重要作用。该文以2020年3月22日湘北地区春季一次冰雹过程为研究对象,运用多普勒天气雷达、风廓线雷达和地基微波辐射计等新型探测资料对该过程观测分析。结果表明：(1)此次过程发生在冷空气南下与南支槽前暖湿空气交汇背景下,受中低层切变线与急流影响,冰雹风暴生成前回暖明显,环境垂直风切变大;风暴由地面辐合线触发产生。(2)此次超级单体降雹过程在雷达回波中表现出“三体散射”“V型缺口”、中气旋等特征;VIL、低仰角大风速核对冰雹和大风预警有很好的指示。(3)风廓线雷达探测到,风暴影响前超低空急流加强,中层有干侵入,低层垂直速度出现波动,风暴临近时超低空急流减弱。(4)地基微波辐射计监测发现,风暴影响前高空湿度增大,K指数、TT指数呈同趋势变化,而K指数预警灵敏度高于TT指数;风暴影响阶段,高空温度、相对湿度和大气不稳定指数出现不同程度跃升和突降。     

风急流对吕宋海峡黑潮路径变异的影响及其动力机制

为研究风急流对吕宋海峡处黑潮路径的影响,本文使用1.5层约化重力浅水模式,设置了与吕宋海峡跨度相接近的缺口宽度,考虑西边界流在西边界缺口处当处于迟滞过程的临界状态时,其路径受风急流影响的动力机制,并初步探讨了在实际海陆边界条件下,实际风急流对黑潮路径的影响。结果显示,理想情况下,当西边界流处在由入侵流态到跨隙流态转变的临界状态时,西风、南风以及西南风风急流可以激发西边界流由入侵流态转变为跨隙流态。当西边界流处在由跨隙流态向入侵流态转变的临界状态时,北风、东风以及东北风风急流可以激发西边界流由跨隙流态转变为入侵流态,并且在风急流消失后西边界流不能再恢复到初始流态。实际情况下,冬季风急流有利于黑潮入侵南海,夏季风急流有利于黑潮跨越吕宋海峡,这和理想情况下的模拟结果以及实际观测结果相一致,这对进一步研究南海北部的上层环流以及南海的质量、能量输送有重要意义。     

Proton and He^2＋ Temperature Anisotropies in the Solar Wind Driven by Ion Cyclotron Waves

We carried out one-dimensional hybrid simulations of resonant scattering of protons and He^2 ions by ion cyclotron waves in an initially homogeneous, collisionless and magnetized plasma. The initial ion cyclotron waves have a power spectrum and propagate both outward and inward. Due to the resonant interaction with the protons and He^2 ions, the wave power will be depleted in the resonance region. Both the protons and He^2 ions can be resonantly heated in the direction perpendicular to the ambient magnetic field and leading to anisotropic velocity distributions, with the anisotropy higher for the He^2 ions than for the protons. At the same time, the anisotropies of the protons and He^2 ions are inversely correlated with the plasma β‖p=8πnpkBT‖p/B0^2, consistent with the prediction of the quasilinear theory (QLT).     

Accuracy of tretyakov precipitation gauge: Result of wmo intercomparison

The Tretyakov non-recording precipitation gauge has been used historically as the official precipitation measurement instrument in the Russian (formerly the USSR) climatic and hydrological station network and in a number of other European countries. From 1986 to 1993, the accuracy and performance of this gauge were evaluated during the WMO Solid Precipitation Measurement Intercomparison at 11 stations in Canada, the USA, Russia, Germany, Finland, Romania and Croatia. The double fence intercomparison reference (DFIR) was the reference standard used at all the Intercomparison stations in the Intercomparison. The Intercomparison data collected at the different sites are compatible with respect to the catch ratio (measured/DFIR) for the same gauge, when compared using mean wind speed at the height of the gauge orifice during the observation period. The Intercomparison data for the Tretyakov gauge were compiled from measurements made at these WMO intercomparison sites. These data represent a variety of climates, terrains and exposures. The effects of environmental factors, such as wind speed, wind direction, type of precipitation and temperature, on gauge catch ratios were investigated. Wind speed was found to be the most important factor determining the gauge catch and air temperature had a secondary effect when precipitation was classified into snow, mixed and rain. The results of the analysis of gauge catch ratio versus wind speed and temperature on a daily time step are presented for various types of precipitation. Independent checks of the correction equations against the DFIR have been conducted at those Intercomparison stations and a good agreement (difference less than 10%) has been obtained. The use of such adjustment procedures should significantly improve the accuracy and homogeneity of gauge-measured precipitation data over large regions of the former USSR and central Europe.     

Internal shocks in a relativistic wind as a source for gamma-ray bursts?

We investigate the recent proposal made by Rees and Mészáros (1994) that GRBs result from internal shocks in the relativistic wind emerging from two coalesced neutron stars. Using a simple model of that wind, where a large number of layers with different Lorentz factors interact through a series of mildly relativistic shocks we compute the efficiency of the process and the time profile of the resulting burst. We show that a great variety of profiles can be obtained using plausible initial distributions of Lorentz factors in the wind. However, the rather low overall efficiency (< 10%) of the process and limits imposed on the burst duration can be used to put severe constraints on the nature of the energy source.     

PRESENT SITUATION，FEATURE AND DEVELOPMENTAL IDEAS OF BORDER OPENING IN XINJIANG

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Polar Coronal Holes During Solar Cycles 22 and 23

Data from the Solar Wind Ion Composition Spectrometer (SWICS) on Ulysses and synoptic maps from Kitt Peak are used to analyze the polar coronal holes of solar activity cycles 22 and 23 (from 1990 to end of 2003). In the beginning of the declining phase of solar cycles 22 and 23, the north polar coronal holes (PCHs) appear about one year earlier than the ones in the south polar region. The solar wind velocity and the solar wind ionic charge composition exhibit a characteristic dependence on the solar wind source position within a PCH. From the center toward the boundary of a young PCH, the solar wind velocity decreases, coinciding with a shift of the ionic charge composition toward higher charge states. However, for an old PCH, the ionic charge composition does not show any obvious change, although the latitude evolution of the velocity is similar to that of a young PCH.     

The dynamics of velocity fluctuations in the solar wind – I. Coronal mass ejections

In this paper we present a simple, analytic model for the dynamical evolution of supersonic velocity fluctuations at the base of the ambient solar wind. These fluctuations result in the formation of dense working surfaces that travel down the wind. It is shown how the initial parameters of the fluctuations (velocity, density and duration) are related to the characteristics of the working surfaces far from the Sun (for instance at the Earth). We apply the model to the evolution of the coronal mass ejections in the IP medium, finding that the model is in good agreement with satellite observations of these phenomena, thus providing physical insight into their dynamical evolution. Our model may contribute to future 'space weather forecasting' on the Earth, based on detailed satellite monitoring of the solar corona.