- Open Access
Monitoring the ionospheric total electron content variations over the Korean Peninsula using a GPS network during geomagnetic storms
© The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences; TERRAPUB. 2011
- Received: 10 December 2010
- Accepted: 9 March 2011
- Published: 7 September 2011
We have established a regional ionospheric model (RIM) for investigating changes in the total electron content (TEC) over South Korea using 38 Korean GPS reference stations. The inverse distance weighted (IDW) interpolation method was applied to create a two-dimensional ionospheric map of vertical TEC units (TECU) based on a grid. To examine the diurnal patterns of ionospheric TEC over South Korea, we first processed the GPS data from a geomagnetically quiet period of 10 days. In a second step, we compared the estimated GPS-TEC variations with the changes in geomagnetic activity indices (the Kp and Dst indices) and the auroral electrojet index (AE) as a function of universal time (UT) on 4 and 20 November, 2003. The GPS-TEC responses for those storm events were proportional to the geomagnetic activity at this mid-latitude location. The sudden increases in ionospheric TEC (SITEC) caused by the geomagnetic storms were detected. The variations in GPS-TEC may help reveal the processes of ionospheric disturbances caused by geomagnetic storms.
- Regional ionospheric model
- total electron content
- inverse distance weighted interpolation
- geomagnetic storm
The Global Positioning System (GPS) has been used as a valuable tool to monitor and estimate ionospheric total electron contents (TECs) (Lanyi and Roth, 1988; Mannucci et al., 1993; Sardon et al., 1994; Davis and Hartmann, 1997; Hernandez-Pajares et al., 1999). The TEC in the ionosphere is measured using two of the L band carrier frequencies, L1 at 1575.42 MHz and L2 at 1227.60 MHz, because GPS signals are easily affected by the dispersive nature of the ionosphere. The propagation time of a signal is directly proportional to the integrated electron density along the signal path. By processing the data from a dual frequency GPS receiver, it is possible to calculate the number of free electrons that were encountered by the signal path from the satellite to the receiver. The magnitude of the TEC in the ionosphere is variable and depends on several factors such as season, geographical position, local time, the solar activity cycle, and geomagnetic storm occurrences (Fedrizzi et al., 2005; Jakowski et al., 2002; Immel et al., 2003; Tsurutani et al., 2004; Mannucci et al., 2005).
The responses of the ionosphere during storm events have been studied for several decades using numerous instruments, such as incoherent scatter radars (ISR) and ionosondes (Lei et al., 2004). However, ISRs are limited by their local coverage, and ionosondes can only observe the bottom part of the ionosphere, whereas ground-based GPS measurements enable the ionosphere to be well monitored without several geometric limitations. Data from GPS networks enable us to measure the TEC of the ionosphere.
Many researchers have developed ionospheric models to derive GPS-TECs (Sardon et al., 1994). Recently, some researchers have used GPS network data to study ionospheric irregularities (Otsuka et al., 2002; Jin et al., 2004). Jakowski et al. (2002) suggested that TEC monitoring by GPS networks can contribute to research on space weather. Wan et al. (2005) investigated the sudden increase in total electron content (SITEC) caused by a very intensive solar flare by using the observations from a worldwide GPS network. Zhao et al. (2005) investigated the response of the Equatorial Ionization Anomaly (EIA) to the superstorms of October–November 2003 using GPS data measured over a regional area. Tsugawa et al. (2006) also investigated medium-scale ionospheric disturbances that generally induce perturbations in ionospheric TECs by using the GPS Earth Observation Network (GEONET). The ground-based GPS networks available both globally and in regional areas also enable the assessment of variations in ionospheric TECs during both quiet and disturbed periods possible. The TEC derived from a GPS network is very useful in helping to understand upper atmosphere phenomena. When data from a ground-based GPS network is used, a map of the TEC over that region can be produced.
Early ionospheric modeling methods were mostly based on function-fitting techniques such as those for spherical harmonics (Schaer, 1999), the broadcasting ionosphere model (Klobuchar, 1987) and polynomial functions. Grid-based ionospheric modeling has been extensively used for global and regional ionosphere recovery (Skone, 1998; Liao, 2000).
One of the largest solar X-ray flares occurred on 4 November 2003. The largest geomagnetic storm of solar cycle 23 occurred on 20 November 2003 due to a coronal mass ejection (CME). Extreme solar flares can result in various ionospheric phenomena: for example, a sudden increase of TEC (SITEC), storm-enhanced density (SED) and equatorial plasma bubbles (EPBs). The 28 and 29 October and 4 November, 2003, flares caused a TEC enhancement of about 30 percent (Tsurutani et al., 2006).
This paper presents a method for high-precision ionospheric TEC modeling using a local GPS network and an attempt to monitor the variation of the ionospheric TEC over the Korean Peninsula by using Korean GPS Network (KGN) data for 4 and 20 November, 2003. The vertical TEC maps obtained from densely-located local GPS receivers enable for a precise detection of the TEC response of the ionosphere. This ionospheric model is based on a two-dimensional grid. The inverse distance weighted (IDW) interpolation method is applied to generate the two-dimensional ionospheric map of the vertical TECU. In order to monitor the TEC response over South Korea during storm periods, diurnal TEC patterns at any point for 10 quiet days are determined and the median TEC variation over the 10 days is also calculated. This data is used to monitor ionospheric TEC enhancements during storm periods. In addition, we have investigated the correlation between TEC responses and geomagnetic activity at mid-latitudes. We have also studied the GPS-TEC variation at the time of sudden storm commencement (SSC). The aim of this paper is to show and discuss some effects on the ionosphere TEC at mid-latitudes of the geomagnetic storms that occurred in November 2003.
The KGN has 80 permanent GPS sites that were established in 2000. Several governmental agencies including the Korea Astronomy and Space Science Institute (KASI) in the Ministry of Education, Science and Technology (MEST), the National Geographic Information Institute (NGI) in the Ministry of Land, Transport and Maritime Affairs (MLTM), the Ministry of Public Administration and Security (MOPAS), and other institutes have operated the GPS network and related facilities. Each reference station of the KGN is equipped with a geodetic dual frequency GPS receiver. The aims of the KGN are specified as the monitoring of local and regional crustal deformation, earth sciences research, cadastral surveys, providing geographic information, and transmitting Differential GPS (DGPS) corrections for a national service through some specific reference stations.
true geometric range from satellite to receiver (m)
satellite clock error (s)
receiver clock error (s)
satellite hardware bias (s)
receiver hardware bias (s)
speed of light in a vacuum (m/s)
ionospheric delay (m)
tropospheric delay (m)
wavelength of frequency (m)
carrier phase integer ambiguity (cycle)
measurement noise (m)
Where P (t i ) and F(t i ) are the pseudo-range and carrier phase observables: respectively. The term ω i is the smoothing weight factor with an initial value of 1 and varying from 0 to 1. The term P(t i )sm is the smoothed code.
Where and Br = b2r–b1r represent the differential code biases (DCBs). When estimating the ionospheric TEC using GPS data, the GPS-DCBs have to be taken into account. If the DCBs are not removed from the TEC value, the “absolute” TEC value cannot be determined. Moreover, GPS receiver DCBs can be as much as a few tens of nanoseconds (ns). The DCBs for all GPS satellites and ground stations are computed daily as constants. In our approach, the estimation of the receiver DCB needs one particular value as reference in the GPS network. We also used a zero-mean condition for the separation of the receiver-dependent part of the bias. The DCB needs to be removed from the original TEC as it results in a decrease of reliability of the ionospheric TEC.
Where Z0 is the value of an interpolated grid point; Z i is a known value, d i is the distance between a point being estimated and a samplied point, k is an exponent parameter, and S is the total number of known points. We applied the IDW method to establish a GPS grid-based ionospheric model over South Korea. The ionospheric TEC maps were produced using a 0.1° grid spacing. To reduce the effects of ray-path bending of GPS signals, the receiver’s elevation mask was set to 15 degrees.
4.1 A typical diurnal pattern of TEC variation in November 2003
The temporal variation of TEC at any point for the 10 quiet days represents the general trends. The diurnal pattern of vertical TEC exhibits a gradual increase from about early morning (UT ~ 0 h) to an afternoon maximum (UT = 5 ~ 6 h) and then decreases sharply until about sunset (UT ~ 11 h). The daily peak occurred around 6:00 UT (UT = LT – 09:00). These patterns of TEC variation help appreciate its day-to-day variability. The median diurnal TEC variation for this period is determined for the purpose of making a comparison with TEC variations monitored during storm times.
4.2 Ionospheric TEC responses to geomagnetic storms
Two large geomagnetic events occurred on 4 and 20 November 2003. We investigated the ionospheric TEC responses at each point of the mid-latitude network during these events.
4.2.1 4 November, 2003
To investigate the characteristics of the ionospheric TEC responses during this period, the ionospheric TEC was derived from the GPS data collected from the KGN in South Korea. The two-dimensional TEC maps of the KASI-RIM have a 0.1° grid spacing and a very high time resolution of 30 seconds.
4.2.2 20 November, 2003
Overall, the analyses showed that the geomagnetic activity indices and the GPS-TEC responses obtained from the KGN were in good agreement at the SSCs that occurred on 4 and 20 November 2003. However, the TEC increments for all the events that occurred at these mid-latitudes were not always proportional to the geomagnetic activity indices. Also, unfortunately, we could not present results for a comparison of GPS-derived TEC and ionosonde TEC due to the loss of some of the ionosonde data at the Anyang station (37.39° N, 126.95°E).
The ionosphere is easily affected by environmental factors. Variations in ionospheric TEC can be detected by local observation data. This paper has examined the ionospheric response over South Korea during the geomagnetic storms on 4 and 20 November 2003 using the permanent Korean GPS network. This study has investigated the similarities between the geomagnetic storms and the local TEC responses observed by a GPS ionospheric model.
In this paper, the grid-based TEC values with high temporal and spatial resolutions were obtained using an inverse distance weighted (IDW) interpolation method. This enables observations of a fast TEC response to variations in conditions, due to the high temporal resolution of 30 seconds. To clearly identify the ionospheric TEC changes that occur during storm periods, we have presented the diurnal pattern of TEC variation over the Korean Peninsula for quiet conditions as well.
We have investigated the GPS-TEC variations of the ionosphere on 4 November and 20 November 2003. The sudden changes in GPS-TEC observed during these storm periods were remarkable. An enhancement of GPS-TEC occurred almost simultaneously with the timing of the sudden storm commencements (SSCs). It has been shown that the small-scale TEC responses derived from this GPS network were closely related with geomagnetic activities. However, the GPS-TEC responses for all of the storm events were not proportional to the geomagnetic activity. The study of the correlation between the TEC response and the geomagnetic activity at mid-latitudes requires further investigation.
Our approach, using high temporal and spatial resolution measurements of TEC, will contribute to the monitoring of ionospheric TEC at mid-latitudes and the study of geomagnetic storms. As a result, GPS can be used as a comprehensive tool for the study of geomagnetic storms and verification of other measurements. Therefore, we believe that the changes in ionospheric composition generated by such storms are the cause of VTEC enhancements observed in the mid-latitudes.
The authors appreciate the referee’s comments which were helpful in improving our manuscript. The authors also would like to thank the data centers, the National Geographic Information Institute (NGI) in the Ministry of Land, Transport and Maritime Affairs (MLTM), the Ministry of Public Administration and Security (MOPAS) and the Data Analysis Center for Geomagnetism and Space Magnetism Graduate School of Science, Kyoto University for providing us with the GPS data and the geomagnetic indices data. This work was supported by the KASI’s basic core technology.
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