4.6 Article

Contrastive research of ionospheric precursor anomalies between Calbuco volcanic eruption on April 23 and Nepal earthquake on April 25, 2015

Journal

ADVANCES IN SPACE RESEARCH
Volume 57, Issue 10, Pages 2141-2153

Publisher

ELSEVIER SCI LTD
DOI: 10.1016/j.asr.2016.02.014

Keywords

Nepal earthquake; Calbuco volcanic eruption; Ionosphere; TEC anomalies; Solar-terrestrial environment; Sliding interquartile range method

Funding

  1. National Natural Science Foundations of China [41374009]
  2. Basic Science and Technology Project of China [2015FY310200]
  3. Natural Science Foundations of Shandong Province, China [ZR2013DM009]
  4. SDUST Research Fund [2014TDJH101]

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On April 23, 2015, the VEI4 (volcanic explosive index) Calbuco volcano abruptly erupted in Chile and the Mw7.9 Nepal earthquake occurred on April 25. In order to investigate the similarities and differences between total electron content (TEC) anomalies preceding these two types of geophysical activities, the TEC time series over preparation zones before the volcanic eruption and earthquake extracted from global ionosphere map were analyzed. We used sunspot numbers (SSN), B-z, Dst, and Kp indices to represent the solar-terrestrial environment and eliminate the effects of solar and geomagnetic activities on ionosphere by the sliding interquartile range method with the 27-day window. The results indicate that TEC-negative and-positive anomalies appeared in the 14th and 6th day before the eruption, respectively. The anomalies lasted about 4-6 h with a magnitude of 15-20 TECU. The TEC anomalies were also observed on the 14th and 6th day before the Nepal earthquake with a duration of 6-8 h, and the absolute magnitude of TEC anomalies was within 12-20 TECU. These findings indicate that the magnitude of TEC anomalies preceding volcanic eruption was larger, and the duration of TEC anomalies before the earthquake was longer, which may be associated with their particular physical mechanisms. The TEC anomalies before the Nepal earthquake in the Eastern hemisphere occurred in the afternoon local time, but those before the eruption were observed in the night local time. Peak regions of TEC anomalies did not coincide with the epicenters of geophysical activities, and the TEC anomalies also appeared in the magnetic conjugated region. Both the TEC anomalies in the preparation zone and conjugated region were distributed near the boundaries of equatorial anomaly zone and moved along the boundaries. In the moving process, sometimes the extent or magnitude of TEC anomalies in the conjugated region was larger than that in the preparation zone. Many more GPS stations and receivers should be distributed along the boundaries of equatorial anomaly zone, which will be significant in predicting volcanic eruptions and earthquakes in the low-mid-latitudes. (C) 2016 COSPAR. Published by Elsevier Ltd. All rights reserved.

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