A LOFAR observation of ionospheric scintillation from two simultaneous travelling ionospheric disturbances
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Published:2020
Issue:
Volume:10
Page:10
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ISSN:2115-7251
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Container-title:Journal of Space Weather and Space Climate
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language:
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Short-container-title:J. Space Weather Space Clim.
Author:
Fallows Richard A.ORCID, Forte Biagio, Astin Ivan, Allbrook Tom, Arnold AlexORCID, Wood AlanORCID, Dorrian GarethORCID, Mevius MaaijkeORCID, Rothkaehl Hanna, Matyjasiak BarbaraORCID, Krankowski AndrzejORCID, Anderson James M., Asgekar AshishORCID, Avruch I. MaxORCID, Bentum MarkORCID, Bisi Mario M., Butcher Harvey R., Ciardi BenedettaORCID, Dabrowski BartoszORCID, Damstra Sieds, de Gasperin FrancescoORCID, Duscha Sven, Eislöffel JochenORCID, Franzen Thomas M.O.ORCID, Garrett Michael A.ORCID, Grießmeier Jean-MatthiasORCID, Gunst André W., Hoeft Matthias, Hörandel Jörg R., Iacobelli MarcoORCID, Intema Huib T.ORCID, Koopmans Leon V.E., Maat Peter, Mann Gottfried, Nelles AnnaORCID, Paas Harm, Pandey Vishambhar N., Reich WolfgangORCID, Rowlinson AntoniaORCID, Ruiter Mark, Schwarz Dominik J.ORCID, Serylak MaciejORCID, Shulevski AleksanderORCID, Smirnov Oleg M.ORCID, Soida MarianORCID, Steinmetz MatthiasORCID, Thoudam SatyendraORCID, Toribio M. CarmenORCID, van Ardenne Arnold, van Bemmel Ilse M.ORCID, van der Wiel Matthijs H.D.ORCID, van Haarlem Michiel P., Vermeulen René C., Vocks ChristianORCID, Wijers Ralph A.M.J., Wucknitz OlafORCID, Zarka PhilippeORCID, Zucca PietroORCID
Abstract
This paper presents the results from one of the first observations of ionospheric scintillation taken using the Low-Frequency Array (LOFAR). The observation was of the strong natural radio source Cassiopeia A, taken overnight on 18–19 August 2013, and exhibited moderately strong scattering effects in dynamic spectra of intensity received across an observing bandwidth of 10–80 MHz. Delay-Doppler spectra (the 2-D FFT of the dynamic spectrum) from the first hour of observation showed two discrete parabolic arcs, one with a steep curvature and the other shallow, which can be used to provide estimates of the distance to, and velocity of, the scattering plasma. A cross-correlation analysis of data received by the dense array of stations in the LOFAR “core” reveals two different velocities in the scintillation pattern: a primary velocity of ~20–40 ms−1 with a north-west to south-east direction, associated with the steep parabolic arc and a scattering altitude in the F-region or higher, and a secondary velocity of ~110 ms−1 with a north-east to south-west direction, associated with the shallow arc and a scattering altitude in the D-region. Geomagnetic activity was low in the mid-latitudes at the time, but a weak sub-storm at high latitudes reached its peak at the start of the observation. An analysis of Global Navigation Satellite Systems (GNSS) and ionosonde data from the time reveals a larger-scale travelling ionospheric disturbance (TID), possibly the result of the high-latitude activity, travelling in the north-west to south-east direction, and, simultaneously, a smaller-scale TID travelling in a north-east to south-west direction, which could be associated with atmospheric gravity wave activity. The LOFAR observation shows scattering from both TIDs, at different altitudes and propagating in different directions. To the best of our knowledge this is the first time that such a phenomenon has been reported.
Funder
Natural Environment Research Council European Space Agency Horizon 2020
Subject
Space and Planetary Science,Atmospheric Science
Cited by
23 articles.
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