Abstract:This paper presents the variations of the rate of change of Total Electron Content (TEC) index (ROTI), characterizing the occurrence of ionospheric plasma irregularities over Vietnam and neighboring countries in the Southeast Asian region using the continuous GPS data during the 2008-2018 period. The results showed that the occurrence of strong ROTI in all stations is maximum in equinox months March/April and September/October and depends on solar activity. The ROTI is weak during periods of low solar activity… Show more
“…The keograms based on CMONOC in 2014 showed that the irregularities had the highest monthly occurrence rate in March of almost 100%, then 80% in September, 48% in December and 27% in June. The high occurrence in both equinoxes and low occurrence in two solstices are consistent with previous results (Su et al 2008;Thanh et al 2021). The seasonal characteristics of occurrence rate showed good correspondence with the vertical drift velocities of the ionospheric plasma (Vyas and Dayanandan 2011;Su et al 2008).…”
Section: Discussionsupporting
confidence: 91%
“…Their results for 2014 showed that only at CUSV (13.74 °N, 100.53 °E) station the occurrence rate in December is higher than that in June. At MTEV (22.39 °N,102.81 °E) and SMAV (21.06 °N, 103.75 °E), the occurrence in June are larger than that in December (Thanh et al 2021). Some researchers found that the occurrence rate of VHF scintillation or spread F in the low-latitude of Indian sector peaked in the equinoxes and winter during the high solar activity period; and during the low solar activity period the occurrence peaked in equinoxes and summer (Sushil and Gwal 2000;Singh et al 2004;Vyas and Dayanandan 2011;Sahithi et al 2019;Raghunath and Ratnam 2015).…”
Ionospheric irregularities have been studied since ~ 70 years ago. With the development of Global Navigation Satellite system (GNSS), networks of GNSS receivers have been used to obtain the characteristics of the irregularities, including the drift velocity, the structure, and the evolution. In this paper, keograms based on the Crustal Movement Observation Network of China (CMONOC) were used to characterize the irregularities over the area from longitude 85 to 125 °E and latitude 11 to 35 °N in 2014. Keograms were obtained for the rate of TEC index (ROTI) for every 0.5 degree longitude and 30 min universal time pixel. The results showed that the occurrence rate of irregularities in 2014 was high in the equinox months and December, and lowest in June. In equinox months the irregularities often appeared after sunset. In March the irregularities usually had long lifetime of ~ 5–7 h and ~ 5 degrees apparent longitudinal width. The long lifetime usually was accompanied by obvious eastward drift of ~ 100 m/s and large vertical ROTI (vROTI). In September the irregularities had weaker ROTI and shorter lifetime than those in March. The irregularities in the 2 equinox months should be related to the equatorial plasma bubbles (EPBs). In June, they appeared ~ 2–3 h later than those in equinoxes and drifted westward. The summer irregularities had weakest ROTI and their latitude was ~ 30 °N, much higher than those in equinoxes. In December, the irregularities were discrete patches with a longitudinal width of ~ 2 degrees and short lifetime of ~ 2 h. Unlike the equatorial irregularities in equinox months which are part of equatorial plasma bubbles, the solstice irregularities mainly appear to be a local phenomenon.
Graphical Abstract
“…The keograms based on CMONOC in 2014 showed that the irregularities had the highest monthly occurrence rate in March of almost 100%, then 80% in September, 48% in December and 27% in June. The high occurrence in both equinoxes and low occurrence in two solstices are consistent with previous results (Su et al 2008;Thanh et al 2021). The seasonal characteristics of occurrence rate showed good correspondence with the vertical drift velocities of the ionospheric plasma (Vyas and Dayanandan 2011;Su et al 2008).…”
Section: Discussionsupporting
confidence: 91%
“…Their results for 2014 showed that only at CUSV (13.74 °N, 100.53 °E) station the occurrence rate in December is higher than that in June. At MTEV (22.39 °N,102.81 °E) and SMAV (21.06 °N, 103.75 °E), the occurrence in June are larger than that in December (Thanh et al 2021). Some researchers found that the occurrence rate of VHF scintillation or spread F in the low-latitude of Indian sector peaked in the equinoxes and winter during the high solar activity period; and during the low solar activity period the occurrence peaked in equinoxes and summer (Sushil and Gwal 2000;Singh et al 2004;Vyas and Dayanandan 2011;Sahithi et al 2019;Raghunath and Ratnam 2015).…”
Ionospheric irregularities have been studied since ~ 70 years ago. With the development of Global Navigation Satellite system (GNSS), networks of GNSS receivers have been used to obtain the characteristics of the irregularities, including the drift velocity, the structure, and the evolution. In this paper, keograms based on the Crustal Movement Observation Network of China (CMONOC) were used to characterize the irregularities over the area from longitude 85 to 125 °E and latitude 11 to 35 °N in 2014. Keograms were obtained for the rate of TEC index (ROTI) for every 0.5 degree longitude and 30 min universal time pixel. The results showed that the occurrence rate of irregularities in 2014 was high in the equinox months and December, and lowest in June. In equinox months the irregularities often appeared after sunset. In March the irregularities usually had long lifetime of ~ 5–7 h and ~ 5 degrees apparent longitudinal width. The long lifetime usually was accompanied by obvious eastward drift of ~ 100 m/s and large vertical ROTI (vROTI). In September the irregularities had weaker ROTI and shorter lifetime than those in March. The irregularities in the 2 equinox months should be related to the equatorial plasma bubbles (EPBs). In June, they appeared ~ 2–3 h later than those in equinoxes and drifted westward. The summer irregularities had weakest ROTI and their latitude was ~ 30 °N, much higher than those in equinoxes. In December, the irregularities were discrete patches with a longitudinal width of ~ 2 degrees and short lifetime of ~ 2 h. Unlike the equatorial irregularities in equinox months which are part of equatorial plasma bubbles, the solstice irregularities mainly appear to be a local phenomenon.
Graphical Abstract
“…[11] Similarly, Nguyen Thi Lan Huong (2013) documented that nitrate level in Ipomoea aquatica, Brassica juncea, and Brassica integrifolia after 9 days of fertilized were 613.09, 587.08, and 580.73 mg/kg of fresh mass, respectively. [12] Table 3 * 1 Each value represents the mean ± SD of six replicates. * 2 The safe limit value set by the VMARD [13] In three leafy vegetables in this study (Brassica juncea, Brassica integrifolia, Ipomoea aquatica) were significantly higher than safe limit value set by the VMARD.…”
Section: Content Of the Nitrate Form In Leafy Vegetablesmentioning
Lead, nitrate, and nitrite are among the major contaminants of vegetables. These concentrations appraise the quality characteristic of vegetables. Governments and regulators has control the level of nitrate, nitrite, and lead in vegetables to protect the human health. The present study was initiated to investigate the levels of these contaminants in five leafy vegetables in local market (Brassica juncea, Brassica integrifolia, Lactuca sativa, Ipomoea aquatica, and Nasturtium officinale). The vegetable species can be listed by decreasing nitrate content as follows: Lactuca sativa > Nasturtium officinale > Ipomoea aquatica > Brassica integrifolia > Brassica juncea. The nitrite content in leafy vegetables was significantly lower than nitrate content. Among observed vegetables, highest concentration of lead is in Ipomoea aquatica (0.200±0.011 mg/L), whereas lead content in Lactuca sativa and Nasturtium officinale were not detected. In addition, the Pb levels in the leafy vegetables were not correlated with nitrate concentration. Based on the results of our investigation, the approximate daily intake (DI) of NO3–, NO2– and Provisional Tolerable Weekly Intake (PTWI) of lead were assessed to human health in consuming the observed leafy vegetables.
“…The occurrence characteristics of high values of ROTI at low latitudes in Africa have been discussed by Abe et al [10], by finding the longitudinal differences of such occurrences. On the other hand, Thanh et al [11] have analysed the behaviour of ROTI over low latitudes in Southeast Asia, in order to characterize ionosphere irregularities.…”
Studies on the irregularities of the ionosphere during disturbed geomagnetic conditions are fundamental to understanding the complex dynamics taking place in the upper atmosphere. In this work, different data sources are used to study the ionosphere effects of two moderate geomagnetic storms, 26–27 February 2014 and 17–18 September 2021, over the Iberian Peninsula. Data are obtained from digital ionosondes in Spain, Italy and Greece; the Global Navigation Satellite System (GNSS) derived Total Electron Content (TEC) and Rate Of TEC Index (ROTI) from several receiver stations in Spain, Portugal and Morocco; and the UPC Quarter-of-an-hour time resolution Rapid GIM (UQRG), vertical TEC global ionosphere maps (GIMs), produced at 15 min intervals by the Universitat Politecnica de Catalunya (UPC, Spain). This analysis showed that, during the two moderate storms, spread-F and high values of ROTI, indicating the presence of irregularities, are found in a very localized area (Southern Iberian Peninsula and northwest Africa) and local times (night-time). However, no irregularities are found eastwards and northwards of the location indicated. We propose some possible explanations for these observations for both the storms, one of them related to the position of the Equatorial Ionosphere Anomaly (EIA) and the other one attributed to the Perkins’ instabilities.
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