2024-03-29T02:02:25Zhttps://eprints.lib.hokudai.ac.jp/dspace-oai/requestoai:eprints.lib.hokudai.ac.jp:2115/810402022-11-17T02:08:08Zhdl_2115_20039hdl_2115_116Investigation of Ionospheric Response to June 2009 Sarychev Peak Volcano EruptionShestakov, NikolayOrlyakovskiy, AlexanderPerevalova, NataliaTitkov, NikolayChebrov, DanilaOhzono, Mako1000030301930Takahashi, Hiroakimetadata only accessCreative Commons Attribution 4.0 Internationalvolcanic eruptionexplosionGNSS ionosphere soundingcovolcanic ionospheric disturbances453Global Navigation Satellite Systems have been extensively used to investigate the ionosphere response to various natural and man-made phenomena for the last three decades. However, ionospheric reaction to volcano eruptions is still insufficiently studied and understood. In this work we analyzed the ionospheric response to the 11-16 June 2009 VEI class 4 Sarychev Peak volcano eruption by using surrounding Russian and Japanese GPS networks. Prominent covolcanictotal electron content (TEC)ionospheric disturbances (CVIDs) with amplitudes and periods ranged between 0.03-0.15 TECU and 2.5-4.5 min were discovered for the three eruptive events occurred at 18:51 UT, 14 June; at 01:15 and 09:18 UT, 15 June 2009. The estimates of apparent CVIDs velocities vary within 700-1000 m/s in the far-field zone (300-900 km to the southwest from the volcano) and 1300-1800 m/s in close proximity toSarychev Peak. The characteristics of the observed TEC variations allow us to attribute them to acoustic mode. The south-southwestward direction is preferred for CVIDs propagation. We concluded that the ionospheric response to a volcano eruption is mainly determined by a ratio between explosion strength and background ionization level. Some evidence of secondary (F2-layer) CVIDs' source eccentric location were obtained.MDPI2021-02engjournal articleNAhttp://hdl.handle.net/2115/81040https://doi.org/10.3390/rs13040638Remote Sensing134638