Reversal of monthly East Asian winter air temperature in 2020/21 and its predictability

在全球变暖的背景下,近年来东亚冬季气温存在复杂的季节内变化.本文研究了2020/21年东亚冬季气温的月际转折及可预测性.结果 表明,2020/21年东亚冬季气温前冬(2020年12月-2021年1月中旬)偏冷,后冬(2021年1月中旬-2月)偏暖.西伯利亚高压强度在前冬和后冬也出现转折变化.在前冬,由于2020年9月巴...     

不同GPS掩星电离层剖面产品相关性分析

将在一定时空限定范围内的不同低轨卫星COSMIC、GRACE、CHAMP、FY3C的电离层掩星电子密度剖面定义为一个掩星对来对比分析不同类型掩星电离层产品。结果表明：COSMIC掩星对之间的电子密度剖面整体轮廓符合得很好,电子密度剖面主要在250 km以下和500 km以上存在较大的偏差,250~500 km的电子密度整体偏差较小,统计得到的COSMIC掩星对的电子密度参量NmF2和hmF2的相关系数能分别达到0.99和0.97,具有高度相关性,不同COSMIC卫星之间没有明显的系统误差;COSMIC、GRACE、CHAMP和FY3C不同低轨卫星间的电子密度剖面略有差异,通过统计电子密度参量NmF2和hmF2之间的相关系数,COSMIC和CHAMP的相关系数分别为0.95和0.86,COSMIC和GRACE的相关系数分别为0.98和0.94,COSMIC和FY3C的相关系数分别为0.96和0.92,不同掩星类型之间的电子密度参量之间也具有高度相关性,验证了不同卫星任务GPS掩星电离层剖面的一致性。     

空间电磁环境研究在军事上的应用

由磁层、电离层和高层大气组成的近地空间系统是现代战争和未来战争活动的主要空间领域,地磁场和地球电磁环境与军事通信、遥感侦察、导航定位以及高空核打击等军事行动有着密切的关系.本文根据已经公开发表于学术刊物的材料,对比分析高空核爆炸产生的人工辐射带和天然辐射带的主要特点以及灾害性空间天气事件（如亚暴和磁暴）对空间飞行器的损害,简要介绍电离层骚扰和不均匀性对通信的影响,探讨地磁场在导航定位中的可能应用.     

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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。     

Comparative study of electron density from incoherent scatter measurements at Arecibo with the IRI-95 model during solar maximum

Arecibo (18.4 N, 66.7 W) incoherent scatter (IS) observations of electron density N(h) are compared with the International Reference Ionosphere (IRI-95) during midday (10/14 h), for summer, winter and equinox, at solar maximum (1981). The N(h) profiles below the F2 peak, are normalized to the peak density NmF2 of the F region and are then compared with the IRI-95 model using both the standard B0 (old option) and the Gulyaeva-B0 thickness (new option). The thickness parameter B0 is obtained from the observed electron density profiles and compared with those obtained from the IRI-95 using both the options. Our studies indicate that during summer and equinox, in general, the values of electron densities at all the heights given by the IRI model (new option), are generally larger than those obtained from IS measurements. However, during winter, the agreement between the IRI and the observed values is reasonably good in the bottom part of the F2 layer but IRI underestimates electron density at F1 layer heights. The IRI profiles obtained with the old option gives much better results than those generated with the new option. Compared to the observations, the IRI profiles are found to be much thicker using Gulyaeva-B0 option than using standard B0.     

Ionospheric measurements during the CRISTA/MAHRSI campaign: their implications and comparison with previous campaigns

The CRISTA/MAHRSI experiment on board a space shuttle was accompanied by a broad campaign of rocket, balloon and ground-based measurements. Supporting lower ionospheric ground-based measurements were run in Europe and Eastern Asia between 1 October–30 November, 1994. Results of comparisons with long ionospheric data series together with short-term comparisons inside the interval October-November, 1994, showed that the upper middle atmosphere (h =80–100 km) at middle latitudes of the Northern Hemisphere in the interval of the CRISTA/MAHRSI experiment (4–12 November, 1994) was very close to its expected climatological state. In other words, the average results of the experiment can be used as climatological data, at least for the given area/altitudes. The role of solar/geomagnetic and “meteorological” control of the lower ionosphere is investigated and compared with the results of MAP/WINE, MAC/SINE and DYANA campaigns. The effects of both solar/geomagnetic and global meteorological factors on the lower ionosphere are found to be weak during autumn 1994 compared to those in MAP/WINE and DYANA winters, and they are even slightly weaker than those in MAP/SINE summer. The comparison of the four campaigns suggests the following overall pattern: in winter the lower ionosphere at northern middle latitudes appears to be fairly well “meteorologically” controlled with a very weak solar influence. In summer, solar influence is somewhat stronger and dominates the weak “meteorological” influence, but the overall solar/meteorological control is weaker than in winter. In autumn we find the weakest overall solar/meteorological control, local effects evidently dominate.     

CUTLASS Finland radar observations of the ionospheric signatures of flux transfer events and the resulting plasma flows

The CUTLASS Finland radar has been run in a two-beam special scan mode, which offered excellent temporal and spatial information on the flows in the high-latitude ionosphere. A detailed study of one day of this data revealed a convection reversal boundary (CRB) in the CUTLASS field of view (f.o.v) on the dayside, the direction of plasma flow either side of the boundary being typical of a dawn-cell convection pattern. Poleward of the CRB a number of pulsed transients are observed, seemingly moving away from the radar. These transients are identified here as the ionospheric signature of flux transfer events (FTEs). Equatorward of the CRB continuous backscatter was observed, believed to be due to the return flow on closed field lines. The two-beam scan offered a new and innovative opportunity to determine the size and velocity of the ionospheric signatures associated with flux transfer events and the related plasma flow pattern. The transient signature was found to have an azimuthal extent of 1900 ± 900 km and an poleward extent of 250 km. The motion of the transient features was in a predominantly westward azimuthal direction, at a velocity of 7.5 ± 3 km.     

白垩纪快速气候变化研究新进展——温室世界中的冰川证据

白垩纪被认为是两极无冰的典型温室气候时期,但近年来对于白垩纪存在短暂冰川甚至是极地冰盖的猜想引起了越来越多的关注。根据前人提出的冰川或气候变冷证据,如冰川遗迹、全球海平面快速下降事件以及δ18O正偏事件等,总结了白垩纪可能存在冰川的时期,包括Berriasian Valanginian之间、Valanginian晚期、Barremiana期、Aptian Albian之交、Albian Cenomanian之交、Cenomanian中期和末期、Turonian中期、Coniacian中期、Santonian早期、Campanian晚期、Campanian Maastrichtian之交和Maastrichtian末期等。对这些证据的有效性进行详细的讨论,同时也对白垩纪冰川的可能成因进行探讨。笔者认为,白垩纪即便存在冰川,也是小规模、短暂地存在,因此,精确的年代学约束是进行白垩纪冰川研究的前提;米兰科维奇旋回控制下的气候波动是白垩纪形成短暂冰川的可能成因。