中纬度地区下午E区等离子体密度不规则性的首次报告

IF 0.6 Q4 ASTRONOMY & ASTROPHYSICS
Tae-Yong Yang, Y. Kwak, Jaewook Lee, Jaeheung Park, Seonghwan Choi
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引用次数: 2

摘要

本文首次报道了2009年12月29日以来,在韩国大田(36.18°N, 127.14°E, 26.7°N倾角)连续工作的甚高频(VHF)相干后向散射雷达对中纬度北部E区场向不规则(FAIs)的观测结果。基于连续雷达观测资料,给出了中纬度e区下午FAIs的统计特征。发现e区下午fai的回波信噪比(SNR)高达35 dB,主要发生在100-135 km高度附近。下午回波的频谱宽度大部分接近于零,表明下午时间的不规则性与湍流等离子体运动无关。下午e区域FAI的发生具有显著的季节变化,夏季最大,冬季最小。此外,为了研究下午E区fai -散发E (Es)的关系,fai还与Es参数进行了比较,这是基于位于大田以北100 km的利川(37.14°N, 127.54°E, 27.7°N)的电离层探空仪的观测结果。Es的虚拟高度主要在105 ~ 110 km之间,比FAI底部高5 ~ 10 km。FAI信噪比与最高频率(fte)(或覆盖频率(fbEs))之间没有关系。然而,发现fai的信噪比与(fte - fbes)密切相关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The First Report on the Afternoon E -Region Plasma Density Irregularities in Middle Latitude
We report, for the first time, the afternoon (i.e., from noon to sunset time) observations of the northern mid-latitude E-region field-aligned irregularities (FAIs) made by the very high frequency (VHF) coherent backscatter radar operated continuously since 29 December 2009 at Daejeon (36.18°N, 127.14°E, 26.7°N dip latitude) in South Korea. We present the statistical characteristics of the mid-latitude afternoon E-region FAIs based on the continuous radar observations. Echo signal-to-noise ratio (SNR) of the afternoon E-region FAIs is found to be as high as 35 dB, mostly occurring around 100–135 km altitudes. Most spectral widths of the afternoon echoes are close to zero, indicating that the irregularities during the afternoon time are not related to turbulent plasma motions. The occurrence of afternoon E-regional FAI is observed with significant seasonal variation, with a maximum in summer and a minimum in winter. Furthermore, to investigate the afternoon E-region FAIs- Sporadic E (Es) relationship, the FAIs have also been compared with Es parameters based on observations made from an ionosonde located at Icheon (37.14°N, 127.54°E, 27.7°N dip latitude), which is 100 km north of Daejeon. The virtual height of Es (h’Es) is mainly in the height range of 105 km to 110 km, which is 5 km to 10 km greater than the bottom of the FAI. There is no relationship between the FAI SNR and the highest frequencies (ftEs) (or blanket frequencies (fbEs)). SNR of FAIs, however, is found to be related well with (ftEs–fbEs).
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来源期刊
Journal of Astronomy and Space Sciences
Journal of Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
1.30
自引率
20.00%
发文量
0
审稿时长
12 weeks
期刊介绍: JASS aims for the promotion of global awareness and understanding of space science and related applications. Unlike other journals that focus either on space science or on space technologies, it intends to bridge the two communities of space science and technologies, by providing opportunities to exchange ideas and viewpoints in a single journal. Topics suitable for publication in JASS include researches in the following fields: space astronomy, solar physics, magnetospheric and ionospheric physics, cosmic ray, space weather, and planetary sciences; space instrumentation, satellite dynamics, geodesy, spacecraft control, and spacecraft navigation. However, the topics covered by JASS are not restricted to those mentioned above as the journal also encourages submission of research results in all other branches related to space science and technologies. Even though JASS was established on the heritage and achievements of the Korean space science community, it is now open to the worldwide community, while maintaining a high standard as a leading international journal. Hence, it solicits papers from the international community with a vision of global collaboration in the fields of space science and technologies.
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