Multi-instrument detection in Europe of ionospheric disturbances caused by the 15 January 2022 eruption of the Hunga volcano

被引:16
|
作者
Verhulst, Tobias G. W. [1 ,2 ]
Altadill, David [3 ]
Barta, Veronika [4 ]
Belehaki, Anna [5 ]
Buresova, Dalia [6 ]
Cesaroni, Claudio [7 ]
Galkin, Ivan [8 ,9 ]
Guerra, Marco [10 ]
Ippolito, Alessandro [7 ]
Herekakis, Themistocles [5 ]
Kouba, Daniel [6 ]
Mielich, Jens [11 ]
Segarra, Antoni [3 ]
Spogli, Luca [7 ,10 ]
Tsagouri, Ioanna [5 ]
机构
[1] Royal Meteorol Inst Belgium, Ringlaan 3, B-1180 Brussels, Belgium
[2] Solar Terr Ctr Excellence, Ringlaan 3, B-1180 Brussels, Belgium
[3] Univ Ramon Llull, Observ Ebre, CSIC, C Observ 3-A, Roquetes 43520, Spain
[4] Inst Earth Phys & Space Sci, Csatkai E U 6-8, H-9400 Sopron, Hungary
[5] IAASARS, Natl Observ Athens, Athens 15236, Greece
[6] Czech Acad Sci, Inst Atmospher Phys, Bocni II 1401, Prague 14131, Czech Republic
[7] Ist Nazl Geofis & Vulcanol, Via Vigna Murata 605, I-00143 Rome, Italy
[8] Borealis Global Designs Ltd, 24 Marie Louise Blvd,Entrance A,Suite 1, Varna 9000, Bulgaria
[9] Univ Massachusetts Lowell, Space Sci Lab, 600 Suffolk St,3rd Floor, Lowell, MA 01854 USA
[10] SpacEarth Technol, Via Vigna Murata 605, I-00143 Rome, Italy
[11] Leibniz Inst Atmospher Phys, Schlossstr 6, D-18225 Kuhlungsborn, Germany
基金
欧盟地平线“2020”;
关键词
Travelling ionospheric disturbances; volcanic eruption impact on the ionosphere; medium-scale TIDs; ACOUSTIC-GRAVITY WAVES; UPPER-ATMOSPHERE; NETWORK; HAAPAI; SWARM;
D O I
10.1051/swsc/2022032
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The 15 January 2022 eruption of the Hunga volcano provides a unique opportunity to study the reaction of the ionosphere to large explosive events. In particular, this event allows us to study the global propagation of travelling ionospheric disturbances (TIDs) using various instruments. We focus on detecting the ionospheric disturbances caused by this eruption over Europe, where dense networks of both ionosondes and GNSS receivers are available. This event took place on the day of a geomagnetic storm. We show how data from different instruments and observatories can be combined to distinguish the TIDs produced by the eruption from those caused by concurrent geomagnetic activity. The Lamb wavefront was detected as the strongest disturbance in the ionosphere, travelling between 300 and 340 m/s, consistent with the disturbances in the lower atmosphere. By comparing observations obtained from multiple types of instruments, we also show that TIDs produced by various mechanisms are present simultaneously, with different types of waves affecting different physical quantities. This illustrates the importance of analysing data from multiple independent instruments in order to obtain a full picture of an event like this one, as relying on only a single data source might result in some effects going unobserved.
引用
收藏
页码:1039 / 1053
页数:20
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