Solar flux effects on equatorial ionization anomaly and total electron content over Brazil: Observational results versus IRI representations

The F layer critical frequency (foF2) as measured by Digisondes in the equatorial and low latitude locations in Brazil is analyzed to investigate the seasonal and solar flux controls of the intensity of the equatorial ionization anomaly (EIA) in the equinoctial month of March. The analysis also included the total electron content (TEC) as measured by a GPS receiver operated at the EIA crest location. The foF2 data set covered a period of large solar flux variation from 1996 to 2003, while the GPS TEC data was for a period in 2002–2003 when the solar flux parameter F10.7 underwent large variations, permitting in both cases an examination of the solar flux effects on these parameters. The seasonal variation pattern in TEC shows a maximum in equinoctial months and a minimum in June solstice, with similar variations for foF2. The solar flux dependence of the TEC is a maximum during equinoxes, especially for post-sunset TEC values at times when the latitudinal distribution is controlled by the equatorial evening plasma fountain processes. Significant variations with local time are found in the degree of solar flux dependence for both the TEC and EIA. The EIA intensity shows large dependence on F10.7 during post-sunset to midnight hours. These results are discussed in comparison with their corresponding IRI representations.     

解决湍流圆/平射流异常现象的数值研究

圆射流/平面射流异常现象是湍流研究领域的一个著名的难题,是验证湍流微分方程模型的试金石。本文用GAO-YONG不可压湍流控制方程对圆射流进行了数值验证,成功地解决了该难题,进一步证明了该方程对真实湍流的适定性和通用性。      

用于飞行器的强电离放电非平衡等离子体隐身方法研究

着重研究了等离子体临界电子密度、电子等离子体频率等参数对电磁波的折射、吸收、反射的影响。在此基础上,采用了强电场电离放电方法,在放电间隙内产生高密度、高能量的电子,它足以电离氮、氧等气体,在飞行器表面形成具有一定梯度的高密度等离子体层,能够吸收、折射电磁波,衰减雷达散射面积达千余倍。该等离子体器件是一个很薄的组合件,仅有百余克重,可贴附在电磁波强散射部位和进气道壁上。此方法具有吸收频带宽、吸收率高等特点,有望成为机载微型等离子体产生器件。     

三轴惯性平台式航空重力仪机载重力测量试验研究

介绍了自主研制的GIPS-1A三轴惯性平台式航空重力仪的组成、工作流程及技术指标,并给出了机载重力测量试验系统的集成方法和数据处理方法.经实际机载航空重力重复线精度测试和试生产测试,重复线内符合精度优于0.6mGal@0.01Hz;与国际上性能优异的GT-2A重力仪相比,重复线符合度好,试生产交叉点总精度相当,且异常形...     

A different view of the ionospheric winter anomaly

The Winter Anomaly (WA) is an ionospheric phenomenon, particularly related to the F2-layer, that is classically defined as the situation in which the ionization level during winter is higher than during summer for a certain location. This situation is anomalous because it contradicts what would be naturally expected with summer’s ionization levels higher than winter ones. This phenomenon has been a matter of study since the early decades of the XX century.This contribution tackles the study of the WA based on long time series (up to two solar cycles) of Total Electron Content (TEC) measurements over a globally distributed network of stations. The work done relies on a threefold strategy including: a classical approach based on the comparison of the winter and summer maximum TEC values, that confirmed the results previously documented; an intermediate approach with maximum TEC values modelled as linear functions of the solar radiation level, that allowed to identify stations where the WA is likely to be observed (and at what solar radiation level) and where is not; a final original approach where the maximum TEC values are modelled using Chapman’s function for the seasonal variations, linear regressions for the solar activity dependence and the introduction of site and month dependent equivalent ionization coefficients for the remaining effects. The main conclusions are that the coefficients for winter months seem to depend mainly on geomagnetic latitude, to increase towards high latitudes and to be asymmetric between hemisphere. In accordance to these findings, the occurrences of WA effects would be regulated by proper combinations of these three effects.     

基于BiGRU-SVDD的ADS-B异常数据检测模型

广播式自动相关监视（ADS-B）作为新一代空管监视技术，由于采用明文方式广播发送数据，因而存在易遭受网络攻击的安全问题。为了准确检测ADS-B数据攻击行为，在充分考虑时间相关性的基础上，提出了针对ADS-B数据的异常数据检测模型。首先利用双向门控循环单元（BiGRU）神经网络预测ADS-B数据，得到了ADS-B数据预测值。再将预测值和实际值作差，将差值放入支持向量数据描述（SVDD）训练，得到了能检测ADS-B异常数据的超球体分类器。并且，选择了合适的滑动窗口，在保证异常检测准确率的同时，缩短BiGRU神经网络的训练时长。实验结果表明，BiGRU-SVDD模型能检测出随机位置偏移攻击、高度偏差攻击、重放攻击、拒绝服务（DOS）等攻击下的ADS-B异常数据。并且，与其他机器学习和深度学习方法相比，BiGRU-SVDD异常检测模型的准确率更佳，适应性更优。     

Practical method to identify orbital anomaly as spacecraft breakup in the geostationary region

Identifying spacecraft breakup events is an essential issue for better understanding of the current orbital debris environment. This paper proposes an observation planning approach to identify an orbital anomaly, which appears as a significant discontinuity in archived orbital history, as a spacecraft breakup. The proposed approach is applicable to orbital anomalies in the geostationary region. The proposed approach selects a spacecraft that experienced an orbital anomaly, and then predicts trajectories of possible fragments of the spacecraft at an observation epoch. This paper theoretically demonstrates that observation planning for the possible fragments can be conducted. To do this, long-term behaviors of the possible fragments are evaluated. It is concluded that intersections of their trajectories will converge into several corresponding regions in the celestial sphere even if the breakup epoch is not specified and it has uncertainty of the order of several weeks.     

受控生态生保系统螺旋藻藻种筛选研究

以目前应用较多的7个螺旋藻品种为研究对象,采用摇床培养的方式,在光照强度为200μmol·m^-2·s^-1,光照周期为24h,培养温度为（30．0±1．0）℃的条件下进行培养,通过比较不同藻种的形态特征、生长速率、碳源利用率、营养组分、光合放氧特性以及耐电离辐射能力等指标,从中筛选出满足受控生态生保技术研究所需的螺旋藻藻种。实验结果表明,6号和7号藻种的各项指标比较突出,尤其是6号藻种,在生长速率、蛋白质等含量、光合放氧活性、以及抗辐射的能力表现更为突出,可作为今后受控生态生保技术研究中进一步研究对象和关键生物部件候选藻种。     

Latitudinal features of Total Electron Content over the African and European longitude sector following the St. Patrick’s day storm of 2015

GNSS TEC values have been obtained from 18 stations distributed from the magnetic equator to nearly 80°N magnetic dip in the African and west-European longitude sector corresponding to the March 17–18, 2015 geomagnetic storm. Significantly depleted ionosphere have been observed at stations north of 50°N geographic on March 18, 2015 following the above storm over a longitude swath 11.9°–21°E covering the Eastern Africa and Western European longitude sector. High ROTI values were noted on March 17^th at locations around 80°N magnetic dip. Two prominent peaks in PCN were noted around 09:00 UT and 14:00 UT on March 17, 2015 and around 15:00 UT on March 18, 2015. Daytime thermospheric (O/N₂) ratio was markedly less on March 18th at latitudes above 60°N geographic which is suggested to be the major driver behind depleted high latitude ionosphere during the recovery phase of the storm on March 18, 2015.     

超声速非平衡电离磁流体流动控制试验和数值模拟

为了开展磁流体(MHD)流动控制原理研究,建立了磁流体技术试验系统,采用电容耦合射频-直流组合放电对Ma=3.5气流进行电离,在磁场作用下产生顺/逆气流方向的洛伦兹力控制流场,采用试验段静压变化来监测磁流体流动控制效果,通过一维模型计算磁流体流动控制过程中流场变化情况,分析磁流体流动控制效果;通过添加电磁源项的Navier-Stokes方程耦合电势泊松方程建立了二维磁流体动力模型,对磁流体流动控制进行数值模拟研究。主要结论如下:在磁场约束下,电容耦合射频-直流组合放电能够在Ma=3.5流场中产生大体积均匀电流,电导率约0.015S/m;在焦耳热和洛伦兹力作用下,磁流体加速时静压升高了130Pa,减速时静压升高了200Pa;磁流体流动控制过程中,仅有不足10%的能量在磁流体通道内发生了作用;数值模拟结果显示,在试验条件下,加速时静压升高了128Pa,减速时静压升高了208Pa,与试验结果基本吻合。