GPS TEC Fluctuations in the Low and High Latitudes During the 2015 St. Patrick`s Day Storm

As a part of collaborative efforts to understand ionospheric irregularities, the Korea ionospheric scintillation sites (KISS) network has been built based on global positioning system (GPS) receivers with sampling rates higher than 1 Hz. We produce the rate of TEC index (ROTI) to represent GPS TEC f...

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Main Authors: Jong-Kyun Chung, Junseok Hong, Sung-Moon Yoo, Jeong-Han Kim, Geonhwa Jee, Valery V. Hegai
Format: Article
Language:English
Published: The Korean Space Science Society 2017-12-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2017/v34n4/OJOOBS_2017_v34n4_245.pdf
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author Jong-Kyun Chung
Junseok Hong
Sung-Moon Yoo
Jeong-Han Kim
Geonhwa Jee
Valery V. Hegai
author_facet Jong-Kyun Chung
Junseok Hong
Sung-Moon Yoo
Jeong-Han Kim
Geonhwa Jee
Valery V. Hegai
author_sort Jong-Kyun Chung
collection DOAJ
description As a part of collaborative efforts to understand ionospheric irregularities, the Korea ionospheric scintillation sites (KISS) network has been built based on global positioning system (GPS) receivers with sampling rates higher than 1 Hz. We produce the rate of TEC index (ROTI) to represent GPS TEC fluctuations related to ionospheric irregularities. In the KISS network, two ground-based GPS sites at Kiruna (marker: KIRN; geographic: 67.9° N, 21.4° E; geomagnetic: 65.2° N) and Chuuk (marker: CHUK; geographic: 7.5° N, 151.9° E; geomagnetic: 0.4° N) were selected to evaluate the ROTI value for ionospheric irregularities during the occurrence of the 2015 St. Patrick’s Day storm. The KIRN ROTI values in the aurora region appear to be generally much higher than the CHUK ROTI values in the EIA region. The CHUK ROTI values increased to ~0.5 TECU/min around UT=13:00 (LT=23:00) on March 16 in the quiet geomagnetic condition. On March 17, 2015, CHUK ROTI values more than 1.0 TECU/min were measured between UT=9:00 and 12:00 (LT=19:00 and 22:00) during the first main phase of the St. Patrick’s Day storm. This may be due to ionospheric irregularities by increased pre-reversal enhancement (PRE) after sunset during the geomagnetic storm. Post-midnight, the CHUK ROTI showed two peaks of ~0.5 TECU/min and ~0.3 TECU/min near UT=15:00 (LT=01:00) and UT=18:00 (LT=04:00) at the second main phase. The KIRN site showed significant peaks of ROTI around geomagnetic latitude=63.3° N and MLT=15:40 on the same day. These can be explained by enhanced ionospheric irregularities in the auroral oval at the maximum of AE index
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spelling doaj.art-6f45c10f91b448ce88f3086e9e02486a2024-02-02T21:05:37ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092017-12-0134424525010.5140/JASS.2017.34.4.245GPS TEC Fluctuations in the Low and High Latitudes During the 2015 St. Patrick`s Day StormJong-Kyun Chung0Junseok Hong1Sung-Moon Yoo2Jeong-Han Kim3Geonhwa Jee4Valery V. Hegai5Korea Astronomy & Space Science Institute, Daejeon 34055, KoreaKorea Astronomy & Space Science Institute, Daejeon 34055, KoreaKorea Astronomy & Space Science Institute, Daejeon 34055, KoreaKorea Polar Research Institute, Incheon 21990, KoreaKorea Polar Research Institute, Incheon 21990, KoreaPushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Russian Academy of Sciences (IZMIRAN), Moscow, Troitsk 142190, Russia As a part of collaborative efforts to understand ionospheric irregularities, the Korea ionospheric scintillation sites (KISS) network has been built based on global positioning system (GPS) receivers with sampling rates higher than 1 Hz. We produce the rate of TEC index (ROTI) to represent GPS TEC fluctuations related to ionospheric irregularities. In the KISS network, two ground-based GPS sites at Kiruna (marker: KIRN; geographic: 67.9° N, 21.4° E; geomagnetic: 65.2° N) and Chuuk (marker: CHUK; geographic: 7.5° N, 151.9° E; geomagnetic: 0.4° N) were selected to evaluate the ROTI value for ionospheric irregularities during the occurrence of the 2015 St. Patrick’s Day storm. The KIRN ROTI values in the aurora region appear to be generally much higher than the CHUK ROTI values in the EIA region. The CHUK ROTI values increased to ~0.5 TECU/min around UT=13:00 (LT=23:00) on March 16 in the quiet geomagnetic condition. On March 17, 2015, CHUK ROTI values more than 1.0 TECU/min were measured between UT=9:00 and 12:00 (LT=19:00 and 22:00) during the first main phase of the St. Patrick’s Day storm. This may be due to ionospheric irregularities by increased pre-reversal enhancement (PRE) after sunset during the geomagnetic storm. Post-midnight, the CHUK ROTI showed two peaks of ~0.5 TECU/min and ~0.3 TECU/min near UT=15:00 (LT=01:00) and UT=18:00 (LT=04:00) at the second main phase. The KIRN site showed significant peaks of ROTI around geomagnetic latitude=63.3° N and MLT=15:40 on the same day. These can be explained by enhanced ionospheric irregularities in the auroral oval at the maximum of AE indexhttp://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2017/v34n4/OJOOBS_2017_v34n4_245.pdfGPS TEC fluctuationrate of TEC indexionospheric irregularitylow and high latitudes
spellingShingle Jong-Kyun Chung
Junseok Hong
Sung-Moon Yoo
Jeong-Han Kim
Geonhwa Jee
Valery V. Hegai
GPS TEC Fluctuations in the Low and High Latitudes During the 2015 St. Patrick`s Day Storm
Journal of Astronomy and Space Sciences
GPS TEC fluctuation
rate of TEC index
ionospheric irregularity
low and high latitudes
title GPS TEC Fluctuations in the Low and High Latitudes During the 2015 St. Patrick`s Day Storm
title_full GPS TEC Fluctuations in the Low and High Latitudes During the 2015 St. Patrick`s Day Storm
title_fullStr GPS TEC Fluctuations in the Low and High Latitudes During the 2015 St. Patrick`s Day Storm
title_full_unstemmed GPS TEC Fluctuations in the Low and High Latitudes During the 2015 St. Patrick`s Day Storm
title_short GPS TEC Fluctuations in the Low and High Latitudes During the 2015 St. Patrick`s Day Storm
title_sort gps tec fluctuations in the low and high latitudes during the 2015 st patrick s day storm
topic GPS TEC fluctuation
rate of TEC index
ionospheric irregularity
low and high latitudes
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2017/v34n4/OJOOBS_2017_v34n4_245.pdf
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