TitleClimatology of equatorial plasma bubble observed by MyRTKnet over the years 2008–2013
Publication TypeConference Paper
Year of Publication2015
AuthorsBuhari, SM, Abdullah, M, Yokoyama, T, Hasbi, AM, Otsuka, Y, Nishioka, M, Bahari, SA, Tsugawa, T
Conference Name2015 International Conference on Space Science and Communication (IconSpace)2015 International Conference on Space Science and Communication (IconSpace)
Date Published08/2015
PublisherIEEE
Conference LocationLangkawi, Malaysia
Abstract

Malaysia Real-Time Kinematics GNSS Network (MyRTKnet) which consists of 78 GPS receivers was used to investigate the occurrence of equatorial plasma bubble (EPB) along 96°E-120°E longitude. In this study, we present the monthly occurrence rate of EPB along the geographical longitudes of 96°E-120°E for a half of solar cycle period (2008-2013). A 2D map of rate of TEC change index (ROTI) projected at 300 km altitude was derived from the signal paths between GPS satellites and the receivers. A ROTI keogram for one day period was obtained from the east-west cross section of the 2D ROTI maps at 4°N for every 5 min. The occurrence day of EPB was determined from the keogram by the existence of ROTI larger than 0.1 TECU/min within the 96°E-120°E longitude. The results show that the occurrence of EPB along the 96°E-120°E has maximum during equinoctial months and is consistent with previous studies. The occurrence rate of EPB during equinoctial months shows similar characteristics in low and high solar activity due to the broad observational coverage of the MyRTKnet. In contrast, the occurrence rate of EPB during solstice months shows significant relation with solar activity. Solstice months recorded high occurrence rate of EPB in high solar activity that might be attributed to post-midnight irregularities.

URLhttp://ieeexplore.ieee.org/lpdocs/epic03/wrapper.htm?arnumber=7283752http://xplorestaging.ieee.org/ielx7/7269215/7283733/07283752.pdf?arnumber=7283752
DOI10.1109/IconSpace.2015.7283752


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