GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015

P. Prikryl, R. Ghoddousi-Fard, A. Viljanen, J. M. Weygand, B. S.R. Kunduri, E. G. Thomas, J. M. Ruohoniemi, M. Connors, D. W. Danskin, P. T. Jayachandran, K. S. Jacobsen, Y. L. Andalsvik, T. Durgonics, K. Oksavik, Y. Zhang, E. Spanswick, V. Sreeja, M. Aquino, P. J. Cilliers, G. Li & 5 others B. Ning, C. N. Mitchell, L. Spogli, M. Terkildsen, A. T. Weatherwax

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

Abstract

Interplanetary coronal mass ejections (ICMEs) compounded by high-speed plasma streams from coronal holes caused two intense geomagnetic storms on March 17-18, 2013 and 2015 during the current solar cycle. Ionospheric responses to the storms in the northern and southern hemispheres are compared in the context of solar wind coupling to the magnetosphere-ionosphere system. Phase scintillation is observed at high latitudes by arrays of high-rate GNSS Ionospheric Scintillation and TEC Monitors (GISTMs) and geodetic-quality GPS receivers sampling at 1 Hz. The high-rate GPS receivers are distributed in the northern and in the southern high latitudes with sparser coverage. In addition to GPS receivers, the high-latitude ionosphere dynamics is studied using arrays of ground-based instruments including HF radars, ionosondes, riometers, magnetometers, optical imagers as well as particle detectors and ultraviolet scanning imagers onboard the DMSP satellites.

Original languageEnglish
Title of host publication32nd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017
PublisherIEEE
Pages1-4
Number of pages4
ISBN (Electronic)9789082598704
DOIs
Publication statusPublished - 10 Nov 2017
Event32nd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2017 - Montreal, Canada
Duration: 19 Aug 201726 Aug 2017

Conference

Conference32nd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2017
CountryCanada
CityMontreal
Period19/08/1726/08/17

Fingerprint

auroral electrojets
electrojets
magnetic storms
Scintillation
polar regions
scintillation
Global positioning system
receivers
Ionosphere
Image sensors
ionospherics
ionospheres
riometers
DMSP satellites
Particle detectors
Magnetosphere
ionosondes
Solar wind
coronal holes
radiation counters

ASJC Scopus subject areas

  • Computer Networks and Communications
  • Instrumentation
  • Radiation

Cite this

Prikryl, P., Ghoddousi-Fard, R., Viljanen, A., Weygand, J. M., Kunduri, B. S. R., Thomas, E. G., ... Weatherwax, A. T. (2017). GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015. In 32nd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017 (pp. 1-4). IEEE. https://doi.org/10.23919/URSIGASS.2017.8105125

GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015. / Prikryl, P.; Ghoddousi-Fard, R.; Viljanen, A.; Weygand, J. M.; Kunduri, B. S.R.; Thomas, E. G.; Ruohoniemi, J. M.; Connors, M.; Danskin, D. W.; Jayachandran, P. T.; Jacobsen, K. S.; Andalsvik, Y. L.; Durgonics, T.; Oksavik, K.; Zhang, Y.; Spanswick, E.; Sreeja, V.; Aquino, M.; Cilliers, P. J.; Li, G.; Ning, B.; Mitchell, C. N.; Spogli, L.; Terkildsen, M.; Weatherwax, A. T.

32nd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017. IEEE, 2017. p. 1-4.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Prikryl, P, Ghoddousi-Fard, R, Viljanen, A, Weygand, JM, Kunduri, BSR, Thomas, EG, Ruohoniemi, JM, Connors, M, Danskin, DW, Jayachandran, PT, Jacobsen, KS, Andalsvik, YL, Durgonics, T, Oksavik, K, Zhang, Y, Spanswick, E, Sreeja, V, Aquino, M, Cilliers, PJ, Li, G, Ning, B, Mitchell, CN, Spogli, L, Terkildsen, M & Weatherwax, AT 2017, GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015. in 32nd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017. IEEE, pp. 1-4, 32nd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2017, Montreal, Canada, 19/08/17. https://doi.org/10.23919/URSIGASS.2017.8105125
Prikryl P, Ghoddousi-Fard R, Viljanen A, Weygand JM, Kunduri BSR, Thomas EG et al. GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015. In 32nd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017. IEEE. 2017. p. 1-4 https://doi.org/10.23919/URSIGASS.2017.8105125
Prikryl, P. ; Ghoddousi-Fard, R. ; Viljanen, A. ; Weygand, J. M. ; Kunduri, B. S.R. ; Thomas, E. G. ; Ruohoniemi, J. M. ; Connors, M. ; Danskin, D. W. ; Jayachandran, P. T. ; Jacobsen, K. S. ; Andalsvik, Y. L. ; Durgonics, T. ; Oksavik, K. ; Zhang, Y. ; Spanswick, E. ; Sreeja, V. ; Aquino, M. ; Cilliers, P. J. ; Li, G. ; Ning, B. ; Mitchell, C. N. ; Spogli, L. ; Terkildsen, M. ; Weatherwax, A. T. / GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015. 32nd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017. IEEE, 2017. pp. 1-4
@inproceedings{8f3d2009d991468082e98009ff4b1c5a,
title = "GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015",
abstract = "Interplanetary coronal mass ejections (ICMEs) compounded by high-speed plasma streams from coronal holes caused two intense geomagnetic storms on March 17-18, 2013 and 2015 during the current solar cycle. Ionospheric responses to the storms in the northern and southern hemispheres are compared in the context of solar wind coupling to the magnetosphere-ionosphere system. Phase scintillation is observed at high latitudes by arrays of high-rate GNSS Ionospheric Scintillation and TEC Monitors (GISTMs) and geodetic-quality GPS receivers sampling at 1 Hz. The high-rate GPS receivers are distributed in the northern and in the southern high latitudes with sparser coverage. In addition to GPS receivers, the high-latitude ionosphere dynamics is studied using arrays of ground-based instruments including HF radars, ionosondes, riometers, magnetometers, optical imagers as well as particle detectors and ultraviolet scanning imagers onboard the DMSP satellites.",
author = "P. Prikryl and R. Ghoddousi-Fard and A. Viljanen and Weygand, {J. M.} and Kunduri, {B. S.R.} and Thomas, {E. G.} and Ruohoniemi, {J. M.} and M. Connors and Danskin, {D. W.} and Jayachandran, {P. T.} and Jacobsen, {K. S.} and Andalsvik, {Y. L.} and T. Durgonics and K. Oksavik and Y. Zhang and E. Spanswick and V. Sreeja and M. Aquino and Cilliers, {P. J.} and G. Li and B. Ning and Mitchell, {C. N.} and L. Spogli and M. Terkildsen and Weatherwax, {A. T.}",
year = "2017",
month = "11",
day = "10",
doi = "10.23919/URSIGASS.2017.8105125",
language = "English",
pages = "1--4",
booktitle = "32nd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017",
publisher = "IEEE",
address = "USA United States",

}

TY - GEN

T1 - GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015

AU - Prikryl, P.

AU - Ghoddousi-Fard, R.

AU - Viljanen, A.

AU - Weygand, J. M.

AU - Kunduri, B. S.R.

AU - Thomas, E. G.

AU - Ruohoniemi, J. M.

AU - Connors, M.

AU - Danskin, D. W.

AU - Jayachandran, P. T.

AU - Jacobsen, K. S.

AU - Andalsvik, Y. L.

AU - Durgonics, T.

AU - Oksavik, K.

AU - Zhang, Y.

AU - Spanswick, E.

AU - Sreeja, V.

AU - Aquino, M.

AU - Cilliers, P. J.

AU - Li, G.

AU - Ning, B.

AU - Mitchell, C. N.

AU - Spogli, L.

AU - Terkildsen, M.

AU - Weatherwax, A. T.

PY - 2017/11/10

Y1 - 2017/11/10

N2 - Interplanetary coronal mass ejections (ICMEs) compounded by high-speed plasma streams from coronal holes caused two intense geomagnetic storms on March 17-18, 2013 and 2015 during the current solar cycle. Ionospheric responses to the storms in the northern and southern hemispheres are compared in the context of solar wind coupling to the magnetosphere-ionosphere system. Phase scintillation is observed at high latitudes by arrays of high-rate GNSS Ionospheric Scintillation and TEC Monitors (GISTMs) and geodetic-quality GPS receivers sampling at 1 Hz. The high-rate GPS receivers are distributed in the northern and in the southern high latitudes with sparser coverage. In addition to GPS receivers, the high-latitude ionosphere dynamics is studied using arrays of ground-based instruments including HF radars, ionosondes, riometers, magnetometers, optical imagers as well as particle detectors and ultraviolet scanning imagers onboard the DMSP satellites.

AB - Interplanetary coronal mass ejections (ICMEs) compounded by high-speed plasma streams from coronal holes caused two intense geomagnetic storms on March 17-18, 2013 and 2015 during the current solar cycle. Ionospheric responses to the storms in the northern and southern hemispheres are compared in the context of solar wind coupling to the magnetosphere-ionosphere system. Phase scintillation is observed at high latitudes by arrays of high-rate GNSS Ionospheric Scintillation and TEC Monitors (GISTMs) and geodetic-quality GPS receivers sampling at 1 Hz. The high-rate GPS receivers are distributed in the northern and in the southern high latitudes with sparser coverage. In addition to GPS receivers, the high-latitude ionosphere dynamics is studied using arrays of ground-based instruments including HF radars, ionosondes, riometers, magnetometers, optical imagers as well as particle detectors and ultraviolet scanning imagers onboard the DMSP satellites.

UR - http://www.scopus.com/inward/record.url?scp=85046138591&partnerID=8YFLogxK

U2 - 10.23919/URSIGASS.2017.8105125

DO - 10.23919/URSIGASS.2017.8105125

M3 - Conference contribution

SP - 1

EP - 4

BT - 32nd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017

PB - IEEE

ER -