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; Tibor Durgonics; K. Oksavik; Y. Zhang; E. Spanswick; V. Sreeja; M. Aquino; P. J. Cilliers; Gaoyuan Li; B. Ning; C. N. Mitchell; L. Spogli; M. Terkildsen; A. T. Weatherwax

doi:10.23919/URSIGASS.2017.8105125

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, Tibor Durgonics, K. Oksavik, Y. Zhang, E. Spanswick, V. Sreeja, M. Aquino, P. J. Cilliers, Gaoyuan LiB. Ning, C. N. Mitchell, L. Spogli, M. Terkildsen, A. T. Weatherwax

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

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 language	English
Title of host publication	General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017 XXXIInd
Number of pages	4
Publisher	IEEE
Publication date	2017
Pages	4
DOIs	https://doi.org/10.23919/URSIGASS.2017.8105125
Publication status	Published - 2017
Event	XXXII General Assembly and Scientific Symposium of the International Union of Radio Science - Palais des congrés, Montréal, Canada Duration: 19 Aug 2017 → 26 Aug 2017 Conference number: 32

Conference

Conference	XXXII General Assembly and Scientific Symposium of the International Union of Radio Science
Number	32
Location	Palais des congrés
Country/Territory	Canada
City	Montréal
Period	19/08/2017 → 26/08/2017

Access to Document

10.23919/URSIGASS.2017.8105125

OpenUrl availability

Full text

Cite this

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., ... Weatherwax, A. T. (2017). GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015. In General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017 XXXIInd (pp. 4). IEEE. https://doi.org/10.23919/URSIGASS.2017.8105125

@inproceedings{d3cdf7bcf3fb474bbc67d627c8ea673d,

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 Tibor Durgonics and K. Oksavik and Y. Zhang and E. Spanswick and V. Sreeja and M. Aquino and Cilliers, {P. J.} and Gaoyuan Li and B. Ning and Mitchell, {C. N.} and L. Spogli and M. Terkildsen and Weatherwax, {A. T.}",

year = "2017",

doi = "10.23919/URSIGASS.2017.8105125",

language = "English",

pages = "4",

booktitle = "General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017 XXXIInd",

publisher = "IEEE",

address = "United States",

note = "XXXII General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2017 ; Conference date: 19-08-2017 Through 26-08-2017",

}

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 General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017 XXXIInd. IEEE, pp. 4, XXXII General Assembly and Scientific Symposium of the International Union of Radio Science, Montréal, Quebec, Canada, 19/08/2017. 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. et al.
General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 2017 XXXIInd. IEEE, 2017. p. 4.

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

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, Tibor

AU - Oksavik, K.

AU - Zhang, Y.

AU - Spanswick, E.

AU - Sreeja, V.

AU - Aquino, M.

AU - Cilliers, P. J.

AU - Li, Gaoyuan

AU - Ning, B.

AU - Mitchell, C. N.

AU - Spogli, L.

AU - Terkildsen, M.

AU - Weatherwax, A. T.

N1 - Conference code: 32

PY - 2017

Y1 - 2017

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.

U2 - 10.23919/URSIGASS.2017.8105125

DO - 10.23919/URSIGASS.2017.8105125

M3 - Article in proceedings

SP - 4

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

PB - IEEE

T2 - XXXII General Assembly and Scientific Symposium of the International Union of Radio Science

Y2 - 19 August 2017 through 26 August 2017

ER -

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

Abstract

Conference

Access to Document

OpenUrl availability

Fingerprint

Cite this