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Comparison between SuperDARN flow vectors and equivalent ionospheric currents from ground magnetometer arrays

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Comparison between SuperDARN flow vectors and equivalent ionospheric currents from ground magnetometer arrays. / Weygand, J. M.; Amm, O.; Angelopoulos, V. et al.
In: Journal of Geophysical Research, Vol. 117, No. A5, A05325, 25.05.2012.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Weygand, JM, Amm, O, Angelopoulos, V, Milan, SE, Grocott, A, Gleisner, H & Stolle, C 2012, 'Comparison between SuperDARN flow vectors and equivalent ionospheric currents from ground magnetometer arrays', Journal of Geophysical Research, vol. 117, no. A5, A05325. https://doi.org/10.1029/2011JA017407

APA

Weygand, J. M., Amm, O., Angelopoulos, V., Milan, S. E., Grocott, A., Gleisner, H., & Stolle, C. (2012). Comparison between SuperDARN flow vectors and equivalent ionospheric currents from ground magnetometer arrays. Journal of Geophysical Research, 117(A5), Article A05325. https://doi.org/10.1029/2011JA017407

Vancouver

Weygand JM, Amm O, Angelopoulos V, Milan SE, Grocott A, Gleisner H et al. Comparison between SuperDARN flow vectors and equivalent ionospheric currents from ground magnetometer arrays. Journal of Geophysical Research. 2012 May 25;117(A5):A05325. doi: 10.1029/2011JA017407

Author

Weygand, J. M. ; Amm, O. ; Angelopoulos, V. et al. / Comparison between SuperDARN flow vectors and equivalent ionospheric currents from ground magnetometer arrays. In: Journal of Geophysical Research. 2012 ; Vol. 117, No. A5.

Bibtex

@article{986b4742df3a410596404d79eb3ae83c,
title = "Comparison between SuperDARN flow vectors and equivalent ionospheric currents from ground magnetometer arrays",
abstract = " Equivalent ionospheric currents obtained with the spherical elementary current systems (SECS) method and derived from nearly 100 ground magnetometers spread over North America and Greenland are compared with ionospheric flow vectors measured by the SuperDARN radars during both the summer and winter seasons. This comparison is done over a range of spatial separations, magnetic latitudes, magnetic local times, and auroral electrojet activity to investigate under what conditions the vectors are anti-parallel to one another. Our results show that in general the equivalent ionospheric currents are anti-parallel to the flows and the best results are achieved within the auroral oval during active geomagnetic conditions in the dawn, dusk and noon sectors in the northern hemisphere summer. These results indicate the best anti-parallel alignment occurs when the currents and flows are large and well defined. Factors that may influence the alignment include ionospheric conductivity gradients and quiet time backgrounds. Our results can be used to approximate the macroscopic (∼1000 km) ionospheric convection patterns. The SECS maps represent a value-added product from the raw magnetometer database and can be used for contextual interpretation; they can help with our understanding of magnetosphere-ionosphere coupling mechanisms using ground arrays and the magnetospheric spacecraft data, and they can be used as input for other techniques.",
keywords = "SuperDARN, auroral region , equivalent ionospheric currents , ionospheric convection , spherical elementary current systems",
author = "Weygand, {J. M.} and O. Amm and V. Angelopoulos and Milan, {S. E.} and A. Grocott and H. Gleisner and C. Stolle",
note = "Copyright 2012 by the American Geophysical Union",
year = "2012",
month = may,
day = "25",
doi = "10.1029/2011JA017407",
language = "English",
volume = "117",
journal = "Journal of Geophysical Research",
issn = "0148-0227",
publisher = "American Geophysical Union",
number = "A5",

}

RIS

TY - JOUR

T1 - Comparison between SuperDARN flow vectors and equivalent ionospheric currents from ground magnetometer arrays

AU - Weygand, J. M.

AU - Amm, O.

AU - Angelopoulos, V.

AU - Milan, S. E.

AU - Grocott, A.

AU - Gleisner, H.

AU - Stolle, C.

N1 - Copyright 2012 by the American Geophysical Union

PY - 2012/5/25

Y1 - 2012/5/25

N2 - Equivalent ionospheric currents obtained with the spherical elementary current systems (SECS) method and derived from nearly 100 ground magnetometers spread over North America and Greenland are compared with ionospheric flow vectors measured by the SuperDARN radars during both the summer and winter seasons. This comparison is done over a range of spatial separations, magnetic latitudes, magnetic local times, and auroral electrojet activity to investigate under what conditions the vectors are anti-parallel to one another. Our results show that in general the equivalent ionospheric currents are anti-parallel to the flows and the best results are achieved within the auroral oval during active geomagnetic conditions in the dawn, dusk and noon sectors in the northern hemisphere summer. These results indicate the best anti-parallel alignment occurs when the currents and flows are large and well defined. Factors that may influence the alignment include ionospheric conductivity gradients and quiet time backgrounds. Our results can be used to approximate the macroscopic (∼1000 km) ionospheric convection patterns. The SECS maps represent a value-added product from the raw magnetometer database and can be used for contextual interpretation; they can help with our understanding of magnetosphere-ionosphere coupling mechanisms using ground arrays and the magnetospheric spacecraft data, and they can be used as input for other techniques.

AB - Equivalent ionospheric currents obtained with the spherical elementary current systems (SECS) method and derived from nearly 100 ground magnetometers spread over North America and Greenland are compared with ionospheric flow vectors measured by the SuperDARN radars during both the summer and winter seasons. This comparison is done over a range of spatial separations, magnetic latitudes, magnetic local times, and auroral electrojet activity to investigate under what conditions the vectors are anti-parallel to one another. Our results show that in general the equivalent ionospheric currents are anti-parallel to the flows and the best results are achieved within the auroral oval during active geomagnetic conditions in the dawn, dusk and noon sectors in the northern hemisphere summer. These results indicate the best anti-parallel alignment occurs when the currents and flows are large and well defined. Factors that may influence the alignment include ionospheric conductivity gradients and quiet time backgrounds. Our results can be used to approximate the macroscopic (∼1000 km) ionospheric convection patterns. The SECS maps represent a value-added product from the raw magnetometer database and can be used for contextual interpretation; they can help with our understanding of magnetosphere-ionosphere coupling mechanisms using ground arrays and the magnetospheric spacecraft data, and they can be used as input for other techniques.

KW - SuperDARN

KW - auroral region

KW - equivalent ionospheric currents

KW - ionospheric convection

KW - spherical elementary current systems

U2 - 10.1029/2011JA017407

DO - 10.1029/2011JA017407

M3 - Journal article

VL - 117

JO - Journal of Geophysical Research

JF - Journal of Geophysical Research

SN - 0148-0227

IS - A5

M1 - A05325

ER -