Gass, Daniel Data and Code for Thesis - An Examination of Observed Coronal Structures Through Automated Techniques Across Solar Cycle 24. [DataSet]

Description

Collection of coronal structure widths and locations by wavelength (171, 193, 211 and 304 Angstroms) for active region and plume structures in Solar Cycle 24 using Solar Dynamics Observatory (SDO) Atmospheric Imaging Assembly (AIA) data, and local coronal brightenings in Solar Cycle 23 using the Solar and Heliospheric Observatory (SOHO) Extreme-ultraviolet Imaging Telescope (EIT). Also contained is the COronal Structure Detection and Analysis (COSDA) software developed to extract these features from raw image data, written in Python 3.

Research / Data Type:	Collection - various types
DOI:	10.17030/uclan.data.00000377
Research Institutes:	Jeremiah Horrocks Institute > The Sun and the Heliosphere
Depositing User:	Daniel Gordon Gass
Date Deposited:	16 May 2023 09:01
Revision:	12
URI:	https://uclandata.uclan.ac.uk/id/eprint/377
Additional details Additional details Creators: Creators Email ORCID Gass, Daniel danielgass192@gmail.com https://orcid.org/0009-0004-7998-4635 Research Groups: Solar Physics Collection period: From To 1 October 2018 15 December 2022 Contact email address: rdmsupport@uclan.ac.uk Last Modified: 16 May 2023 09:20

Available Files

Full Archive

ThesisCode-main.zip ThesisCode-main.zip ThesisCode-main.zip Visible to: Anyone Document Type : Full Archive File Description: An archive containing the results of investigations into widths and positions of coronal structures at limb for Cycle 24 with AIA, and Cycle 23 with EIT alongside code used for each of the three stages. Metadata Revision: 3 Mime-Type: application/zip Language: English License: Creative Commons: Attribution-No Derivative Works 3.0 File size: 15MB