Paper

Published: 2020/1/15

Geomagnetic Field Observation for Deeper Understanding of Space and Ground Phenomena

Nurul Shazana Abdul Hamid, Khairul Adib Yusof, Mardina Abdullah (Universiti Kebangsaan Malaysia-The National University of Malaysia)

Assessment of signal processing methods for geomagnetic precursor of the 2012 M6.9 Visayas, Philippines earthquake
Acta Geophysica, 67, 1297-1306, doi:10.1007/s11600-019-00319-w, 2019

Investigation of Unusual Solar Flare Effect on the Global Ionospheric Current System
J. Geophysical Res., 123, 8599-8609, doi:10.1029/2018JA025601, 2018

  Geomagnetic field data have been widely used by scientists to gain deeper insight of Earth’s interior's activities and the surrounding space environment. We have been utilizing ground-based magnetometer data provided by Magnetic Data Acquisition System (MAGDAS) of Kyushu University in exploring earthquake and solar flare phenomena.


  Earthquake forecasting by observing anomalous geomagnetic emission were mostly accomplished by utilizing either one of these signal processing methods: polarization ratio analysis (PRA) and diurnal variation ratio (DVR). In order to objectively compare their performances, the M6.9 Visayas, Philipines earthquake on 6th February 2012 was selected as a case study. Geomagnetic field data from two MAGDAS stations located in close proximity to the epicentre (i.e. Cebu and Legazpi stations) were acquired and processed. A precursory anomaly was found using the PRA method, which appeared 2 weeks before the earthquake. In contrast, the DVR method did not reveal any prominent anomaly to be considered as precursor. The difference between the performances of the two methods may be attributed to the studied earthquake having a low magnitude, which possibly emitted weaker geomagnetic emission during the pre-earthquake phase. Nevertheless, the PRA method was shown to be effective in detecting possible precursor of upcoming earthquake, thus have bigger potential to be utilized in real-time prediction.

[Top photo] Dr. Shazana (rightmost) was having a discussion with Assoc. Prof. Dr. Akimasa Yoshikawa (PI of MAGDAS Project) at Kyushu University. [Left bottom photo] Prof. Ir Dr. Mardina (leftmost) and Dr. Shazana (rightmost) with Assoc. Prof. Dr. Akimasa during a public talk at UKM. [Right bottom photo] Mr. Khairul (center) was undergoing training at BMKG Indonesia.

The most recent MAGDAS magnetometer installation in Penang, Malaysia in September 2019, which is the 7th such instrument in the country.

  The application of geomagnetic data in space weather research is deemed promising due to the high volume of ground observatories around the globe. Together with data from other networks, we investigated geomagnetic crochets following the X-class solar flare events occurred during geomagnetically quiet days, which were 9 August 2011 (X6.9) and 24 September 2011 (X1.4). The ionospheric current responses during these two events were significantly different as reductions of the eastward equatorial electrojet were observed in all daytime stations during the former event while enhancements were observed in the latter event. By applying spherical harmonic analysis on the data from a number of ground stations, we revealed that the equivalent current system of the geomagnetic crochets for the 24 September 2011 event exhibit a similar pattern with the background Sq current system. On the other hand, the crochet current system for the 9 August 2011 event revealed a different pattern from the background Sq current system in both Northern and Southern Hemispheres.