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Dusk-Dawn Asymmetries in SuperDARN Convection Maps

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Dusk-Dawn Asymmetries in SuperDARN Convection Maps. / Walach, Maria; Grocott, Adrian; Thomas, Evan et al.
In: Journal of Geophysical Research: Space Physics, Vol. 127, No. 12, e2022JA030906, 20.12.2022.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Walach, M, Grocott, A, Thomas, E & Staples, F 2022, 'Dusk-Dawn Asymmetries in SuperDARN Convection Maps', Journal of Geophysical Research: Space Physics, vol. 127, no. 12, e2022JA030906. https://doi.org/10.1029/2022ja030906

APA

Walach, M., Grocott, A., Thomas, E., & Staples, F. (2022). Dusk-Dawn Asymmetries in SuperDARN Convection Maps. Journal of Geophysical Research: Space Physics, 127(12), Article e2022JA030906. https://doi.org/10.1029/2022ja030906

Vancouver

Walach M, Grocott A, Thomas E, Staples F. Dusk-Dawn Asymmetries in SuperDARN Convection Maps. Journal of Geophysical Research: Space Physics. 2022 Dec 20;127(12):e2022JA030906. doi: 10.1029/2022ja030906

Author

Walach, Maria ; Grocott, Adrian ; Thomas, Evan et al. / Dusk-Dawn Asymmetries in SuperDARN Convection Maps. In: Journal of Geophysical Research: Space Physics. 2022 ; Vol. 127, No. 12.

Bibtex

@article{bccf7fa6d42d4ec3bee7eca77c5bc3cb,
title = "Dusk-Dawn Asymmetries in SuperDARN Convection Maps",
abstract = "The Super Dual Auroral Radar Network (SuperDARN) is a collection of radars built to study ionospheric convection. We use a 7-year archive of SuperDARN convection maps, processed in 3 different ways, to build a statistical understanding of dusk-dawn asymmetries in the convection patterns. We find that the data set processing alone can introduce a bias which manifests itself in dusk-dawn asymmetries. We find that the solar wind clock angle affects the balance in the strength of the convection cells. We further find that the location of the positive potential foci is most likely observed at latitudes of 78° for long periods (>300 min) of southward interplanetary magnetic field (IMF), as opposed to 74° for short periods (",
author = "Maria Walach and Adrian Grocott and Evan Thomas and Frances Staples",
year = "2022",
month = dec,
day = "20",
doi = "10.1029/2022ja030906",
language = "English",
volume = "127",
journal = "Journal of Geophysical Research: Space Physics",
issn = "2169-9402",
publisher = "Blackwell Publishing Ltd",
number = "12",

}

RIS

TY - JOUR

T1 - Dusk-Dawn Asymmetries in SuperDARN Convection Maps

AU - Walach, Maria

AU - Grocott, Adrian

AU - Thomas, Evan

AU - Staples, Frances

PY - 2022/12/20

Y1 - 2022/12/20

N2 - The Super Dual Auroral Radar Network (SuperDARN) is a collection of radars built to study ionospheric convection. We use a 7-year archive of SuperDARN convection maps, processed in 3 different ways, to build a statistical understanding of dusk-dawn asymmetries in the convection patterns. We find that the data set processing alone can introduce a bias which manifests itself in dusk-dawn asymmetries. We find that the solar wind clock angle affects the balance in the strength of the convection cells. We further find that the location of the positive potential foci is most likely observed at latitudes of 78° for long periods (>300 min) of southward interplanetary magnetic field (IMF), as opposed to 74° for short periods (

AB - The Super Dual Auroral Radar Network (SuperDARN) is a collection of radars built to study ionospheric convection. We use a 7-year archive of SuperDARN convection maps, processed in 3 different ways, to build a statistical understanding of dusk-dawn asymmetries in the convection patterns. We find that the data set processing alone can introduce a bias which manifests itself in dusk-dawn asymmetries. We find that the solar wind clock angle affects the balance in the strength of the convection cells. We further find that the location of the positive potential foci is most likely observed at latitudes of 78° for long periods (>300 min) of southward interplanetary magnetic field (IMF), as opposed to 74° for short periods (

U2 - 10.1029/2022ja030906

DO - 10.1029/2022ja030906

M3 - Journal article

VL - 127

JO - Journal of Geophysical Research: Space Physics

JF - Journal of Geophysical Research: Space Physics

SN - 2169-9402

IS - 12

M1 - e2022JA030906

ER -