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, 12...

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Main Authors: Tae-Yong Yang, Young-Sil Kwak, Jaeheung Park, Seonghwan Choi, Jaewook Lee
Format: Article
Language:English
Published: The Korean Space Science Society 2021-06-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://koreascience.or.kr/article/JAKO202118248972703.page
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author Tae-Yong Yang
Young-Sil Kwak
Jaeheung Park
Seonghwan Choi
Jaewook Lee
author_facet Tae-Yong Yang
Young-Sil Kwak
Jaeheung Park
Seonghwan Choi
Jaewook Lee
author_sort Tae-Yong Yang
collection DOAJ
description 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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spelling doaj.art-24d88d67c4694b9bb6f50cf1bd8942c22024-02-03T02:10:51ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092021-06-0138213514310.5140/JASS.2021.38.2.135The First Report on the Afternoon E -Region Plasma Density Irregularities in Middle LatitudeTae-Yong Yang0https://orcid.org/0000-0002-5725-9828Young-Sil Kwak1https://orcid.org/0000-0003-3375-8574Jaeheung Park2https://orcid.org/0000-0002-1272-508XSeonghwan Choi3https://orcid.org/0000-0002-1946-7327Jaewook Lee4https://orcid.org/0000-0002-5284-4841Korea Astronomy and Space Science Institute, Daejeon 34055, KoreaKorea Astronomy and Space Science Institute, Daejeon 34055, KoreaKorea Astronomy and Space Science Institute, Daejeon 34055, KoreaKorea Astronomy and Space Science Institute, Daejeon 34055, KoreaKorea Astronomy and Space Science Institute, Daejeon 34055, KoreaWe 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).http://koreascience.or.kr/article/JAKO202118248972703.pagevery high frequency (vhf) coherent backscatter radarafternoon e-region irregularities
spellingShingle Tae-Yong Yang
Young-Sil Kwak
Jaeheung Park
Seonghwan Choi
Jaewook Lee
The First Report on the Afternoon E -Region Plasma Density Irregularities in Middle Latitude
Journal of Astronomy and Space Sciences
very high frequency (vhf) coherent backscatter radar
afternoon e-region irregularities
title The First Report on the Afternoon E -Region Plasma Density Irregularities in Middle Latitude
title_full The First Report on the Afternoon E -Region Plasma Density Irregularities in Middle Latitude
title_fullStr The First Report on the Afternoon E -Region Plasma Density Irregularities in Middle Latitude
title_full_unstemmed The First Report on the Afternoon E -Region Plasma Density Irregularities in Middle Latitude
title_short The First Report on the Afternoon E -Region Plasma Density Irregularities in Middle Latitude
title_sort first report on the afternoon e region plasma density irregularities in middle latitude
topic very high frequency (vhf) coherent backscatter radar
afternoon e-region irregularities
url http://koreascience.or.kr/article/JAKO202118248972703.page
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