TY - JOUR
T1 - Multi-instrument detection in Europe of ionospheric disturbances caused by the 15 January 2022 eruption of the Hunga volcano
AU - Verhulst, Tobias G.W.
AU - Altadill, David
AU - Barta, Veronika
AU - Belehaki, Anna
AU - Burešová, Dalia
AU - Cesaroni, Claudio
AU - Galkin, Ivan
AU - Guerra, Marco
AU - Ippolito, Alessandro
AU - Herekakis, Themistocles
AU - Kouba, Daniel
AU - Mielich, Jens
AU - Segarra, Antoni
AU - Spogli, Luca
AU - Tsagouri, Ioanna
N1 - Funding Information:
The study is partially funded by the PITHIA-NRF Horizon 2020 Grant Agreement 101007599 of the European Commission and uses resources deployed in the frames of the TechTIDE Horizon 2020 Grant Agreement 776011.
Funding Information:
A. Belehaki acknowledges the financial support provided by the AFRL grant award FA9550-19-17019. The Swarm IPIR data can be obtained through the official Swarm website ftp://swarm-diss.eo.esa.int and through the Swarm IPIR web page http://tid.uio.no/plasma/swarm/IPIR_cdf/ .
Funding Information:
The study is partially funded by the PITHIA-NRF Horizon 2020 Grant Agreement 101007599 of the European Commission and uses resources deployed in the frames of the Tech- TIDE Horizon 2020 Grant Agreement 776011.
Publisher Copyright:
© T.G.W. Verhulst et al., Published by EDP Sciences 2022.
PY - 2022
Y1 - 2022
N2 - 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.
AB - 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.
KW - Medium-scale TIDs
KW - Travelling ionospheric disturbances
KW - Volcanic eruption impact on the ionosphere
UR - http://www.scopus.com/inward/record.url?scp=85137106731&partnerID=8YFLogxK
U2 - 10.1051/swsc/2022032
DO - 10.1051/swsc/2022032
M3 - Article
AN - SCOPUS:85137106731
SN - 2115-7251
VL - 12
SP - 1039
EP - 1053
JO - Journal of Space Weather and Space Climate
JF - Journal of Space Weather and Space Climate
IS - 3
ER -