A unified model of cusp spot, High Latitude Dayside aurora (HiLDA)/(Space Hurricane), and 15MLT-PCA

Cusp spot, High Latitude Dayside aurora (HiLDA), ‘space hurricane’, and 15MLT-PCA (Polar Cap Arc observed around 15:00 Magnetic Local Time) are mesoscale auroral structures observed in the polar cap region. They share many common properties and, at the same time, have notable differences. A 15MLT-PC...

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Main Authors: DeSheng Han, YaTing Xiong, Run Shi, HuiXuan Qiu, HuiTing Feng
Format: Article
Language:English
Published: Science Press 2023-07-01
Series:Earth and Planetary Physics
Subjects:
Online Access:http://www.eppcgs.org/article/doi/10.26464/epp2023046?pageType=en
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author DeSheng Han
YaTing Xiong
Run Shi
HuiXuan Qiu
HuiTing Feng
author_facet DeSheng Han
YaTing Xiong
Run Shi
HuiXuan Qiu
HuiTing Feng
author_sort DeSheng Han
collection DOAJ
description Cusp spot, High Latitude Dayside aurora (HiLDA), ‘space hurricane’, and 15MLT-PCA (Polar Cap Arc observed around 15:00 Magnetic Local Time) are mesoscale auroral structures observed in the polar cap region. They share many common properties and, at the same time, have notable differences. A 15MLT-PCA is a polar cap arc connected to the auroral oval, but the others are auroral spots detached from the oval. A cusp spot differs from a HiLDA in local time location. A space hurricane differs from a HiLDA in having spiral-arm structures. Until now, relationships among these auroras have not been depicted clearly. Here we propose a unified model, based on lobe reconnection, that encompasses their similarities and differences. We then provide critical supporting evidence for the model. The model suggests that different reconnection sites under different IMF conditions result in these differently-appearing auroral forms. The model explains all the characteristic features of these auroras and has implications for understanding the dawn/dusk and inter-hemispheric asymmetries observed in their occurrence patterns. We anticipate confirmation of the model by observations to be made during the Solar wind-Magnetosphere-Ionosphere Link Explorer (SMILE) mission. Moreover, since the model indicates that these auroras appear on the footprint of the poleward cusp boundary, we expect data from the SMILE mission to make it possible to estimate the approximate shape of the cusp.
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spelling doaj.art-a8d955982df64bbb8b7cfc3e64a8f0172023-07-03T01:41:43ZengScience PressEarth and Planetary Physics2096-39552023-07-017451351910.26464/epp2023046PE386-handesheng-FA unified model of cusp spot, High Latitude Dayside aurora (HiLDA)/(Space Hurricane), and 15MLT-PCADeSheng Han0YaTing Xiong1Run Shi2HuiXuan Qiu3HuiTing Feng4State Key Laboratory of Marine Geology, School of Ocean and Earth Science, Tongji University, Shanghai 200092, ChinaState Key Laboratory of Marine Geology, School of Ocean and Earth Science, Tongji University, Shanghai 200092, ChinaState Key Laboratory of Marine Geology, School of Ocean and Earth Science, Tongji University, Shanghai 200092, ChinaState Key Laboratory of Marine Geology, School of Ocean and Earth Science, Tongji University, Shanghai 200092, ChinaState Key Laboratory of Marine Geology, School of Ocean and Earth Science, Tongji University, Shanghai 200092, ChinaCusp spot, High Latitude Dayside aurora (HiLDA), ‘space hurricane’, and 15MLT-PCA (Polar Cap Arc observed around 15:00 Magnetic Local Time) are mesoscale auroral structures observed in the polar cap region. They share many common properties and, at the same time, have notable differences. A 15MLT-PCA is a polar cap arc connected to the auroral oval, but the others are auroral spots detached from the oval. A cusp spot differs from a HiLDA in local time location. A space hurricane differs from a HiLDA in having spiral-arm structures. Until now, relationships among these auroras have not been depicted clearly. Here we propose a unified model, based on lobe reconnection, that encompasses their similarities and differences. We then provide critical supporting evidence for the model. The model suggests that different reconnection sites under different IMF conditions result in these differently-appearing auroral forms. The model explains all the characteristic features of these auroras and has implications for understanding the dawn/dusk and inter-hemispheric asymmetries observed in their occurrence patterns. We anticipate confirmation of the model by observations to be made during the Solar wind-Magnetosphere-Ionosphere Link Explorer (SMILE) mission. Moreover, since the model indicates that these auroras appear on the footprint of the poleward cusp boundary, we expect data from the SMILE mission to make it possible to estimate the approximate shape of the cusp.http://www.eppcgs.org/article/doi/10.26464/epp2023046?pageType=enpolar cap aurora15mlt-pcahildacusp spot
spellingShingle DeSheng Han
YaTing Xiong
Run Shi
HuiXuan Qiu
HuiTing Feng
A unified model of cusp spot, High Latitude Dayside aurora (HiLDA)/(Space Hurricane), and 15MLT-PCA
Earth and Planetary Physics
polar cap aurora
15mlt-pca
hilda
cusp spot
title A unified model of cusp spot, High Latitude Dayside aurora (HiLDA)/(Space Hurricane), and 15MLT-PCA
title_full A unified model of cusp spot, High Latitude Dayside aurora (HiLDA)/(Space Hurricane), and 15MLT-PCA
title_fullStr A unified model of cusp spot, High Latitude Dayside aurora (HiLDA)/(Space Hurricane), and 15MLT-PCA
title_full_unstemmed A unified model of cusp spot, High Latitude Dayside aurora (HiLDA)/(Space Hurricane), and 15MLT-PCA
title_short A unified model of cusp spot, High Latitude Dayside aurora (HiLDA)/(Space Hurricane), and 15MLT-PCA
title_sort unified model of cusp spot high latitude dayside aurora hilda space hurricane and 15mlt pca
topic polar cap aurora
15mlt-pca
hilda
cusp spot
url http://www.eppcgs.org/article/doi/10.26464/epp2023046?pageType=en
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