The Morphology of Poleward Moving Auroral Forms

We investigated the morphology of poleward moving auroral forms (PMAFs) qualitatively by visual inspection of all-sky camera (ASC) images and quantitatively using the arciness index. The PMAFs in this study were initially identified with a meridian scanning photometer (MSP) located at the Kjell Henr...

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Main Authors: Goertz, Anton Oscar, Partamies, Noora, Whiter, Daniel, Baddeley, Lisa
Format: Text
Language:English
Published: 2023
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2022-296
https://egusphere.copernicus.org/preprints/2022/egusphere-2022-296/
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spelling ftcopernicus:oai:publications.copernicus.org:egusphere102949 2023-05-15T17:48:28+02:00 The Morphology of Poleward Moving Auroral Forms Goertz, Anton Oscar Partamies, Noora Whiter, Daniel Baddeley, Lisa 2023-03-21 application/pdf https://doi.org/10.5194/egusphere-2022-296 https://egusphere.copernicus.org/preprints/2022/egusphere-2022-296/ eng eng doi:10.5194/egusphere-2022-296 https://egusphere.copernicus.org/preprints/2022/egusphere-2022-296/ eISSN: Text 2023 ftcopernicus https://doi.org/10.5194/egusphere-2022-296 2023-03-27T16:23:13Z We investigated the morphology of poleward moving auroral forms (PMAFs) qualitatively by visual inspection of all-sky camera (ASC) images and quantitatively using the arciness index. The PMAFs in this study were initially identified with a meridian scanning photometer (MSP) located at the Kjell Henriksen Observatory (KHO), Svalbard, and analyzed using ASC images taken by cameras at the KHO and in Ny-Ålesund, Svalbard. We present a detailed six-step evolution of PMAF morphology in two dimensions. This evolution includes (1) an equatorward expansion of the auroral oval and an intensification of auroral brightness at the open–closed boundary (OCB), (2) the appearance of an arc-like structure in the oval, (3) poleward and possible west/eastward propagation, (4) azimuthal expansion events, (5) re-brightening of the PMAF and eventual (6) fading away. This is the first work dedicated to the morphological evolution of PMAFs and it includes more detailed discussion and novel aspects, such as the observation of initial merging of 557.7 nm auroral patches to form a PMAF. Moreover, the morphology of PMAFs is quantified using the arciness index, which is a number describing how arc-like auroral forms appear in ASC images. This allows an unbiased statistical investigation of auroral morphology. We present the results of a superposed epoch analysis of arciness in relation to PMAF occurrence. This analysis uncovered that arciness increases suddenly during the onset of a PMAF event and decreases over the PMAF lifetime to return to its baseline value once the event has concluded. This behavior may be understood based on changes in the morphology of PMAFs and validates our understanding of PMAF morphology. Furthermore, our findings relating to arciness may enable automatic identification of PMAFs, which has been found to be notoriously difficult. Text Ny Ålesund Ny-Ålesund Svalbard Copernicus Publications: E-Journals Ny-Ålesund Svalbard
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description We investigated the morphology of poleward moving auroral forms (PMAFs) qualitatively by visual inspection of all-sky camera (ASC) images and quantitatively using the arciness index. The PMAFs in this study were initially identified with a meridian scanning photometer (MSP) located at the Kjell Henriksen Observatory (KHO), Svalbard, and analyzed using ASC images taken by cameras at the KHO and in Ny-Ålesund, Svalbard. We present a detailed six-step evolution of PMAF morphology in two dimensions. This evolution includes (1) an equatorward expansion of the auroral oval and an intensification of auroral brightness at the open–closed boundary (OCB), (2) the appearance of an arc-like structure in the oval, (3) poleward and possible west/eastward propagation, (4) azimuthal expansion events, (5) re-brightening of the PMAF and eventual (6) fading away. This is the first work dedicated to the morphological evolution of PMAFs and it includes more detailed discussion and novel aspects, such as the observation of initial merging of 557.7 nm auroral patches to form a PMAF. Moreover, the morphology of PMAFs is quantified using the arciness index, which is a number describing how arc-like auroral forms appear in ASC images. This allows an unbiased statistical investigation of auroral morphology. We present the results of a superposed epoch analysis of arciness in relation to PMAF occurrence. This analysis uncovered that arciness increases suddenly during the onset of a PMAF event and decreases over the PMAF lifetime to return to its baseline value once the event has concluded. This behavior may be understood based on changes in the morphology of PMAFs and validates our understanding of PMAF morphology. Furthermore, our findings relating to arciness may enable automatic identification of PMAFs, which has been found to be notoriously difficult.
format Text
author Goertz, Anton Oscar
Partamies, Noora
Whiter, Daniel
Baddeley, Lisa
spellingShingle Goertz, Anton Oscar
Partamies, Noora
Whiter, Daniel
Baddeley, Lisa
The Morphology of Poleward Moving Auroral Forms
author_facet Goertz, Anton Oscar
Partamies, Noora
Whiter, Daniel
Baddeley, Lisa
author_sort Goertz, Anton Oscar
title The Morphology of Poleward Moving Auroral Forms
title_short The Morphology of Poleward Moving Auroral Forms
title_full The Morphology of Poleward Moving Auroral Forms
title_fullStr The Morphology of Poleward Moving Auroral Forms
title_full_unstemmed The Morphology of Poleward Moving Auroral Forms
title_sort morphology of poleward moving auroral forms
publishDate 2023
url https://doi.org/10.5194/egusphere-2022-296
https://egusphere.copernicus.org/preprints/2022/egusphere-2022-296/
geographic Ny-Ålesund
Svalbard
geographic_facet Ny-Ålesund
Svalbard
genre Ny Ålesund
Ny-Ålesund
Svalbard
genre_facet Ny Ålesund
Ny-Ålesund
Svalbard
op_source eISSN:
op_relation doi:10.5194/egusphere-2022-296
https://egusphere.copernicus.org/preprints/2022/egusphere-2022-296/
op_doi https://doi.org/10.5194/egusphere-2022-296
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