<?xml-model href='http://www.tei-c.org/release/xml/tei/custom/schema/relaxng/tei_all.rng' schematypens='http://relaxng.org/ns/structure/1.0'?><TEI xmlns="http://www.tei-c.org/ns/1.0">
	<teiHeader>
		<fileDesc>
			<titleStmt><title level='a'>MAGFILO: Manually Annotated GONG Filaments in H-Alpha Observations</title></titleStmt>
			<publicationStmt>
				<publisher>Harvard Dataverse</publisher>
				<date>01/01/2024</date>
			</publicationStmt>
			<sourceDesc>
				<bibl> 
					<idno type="par_id">10538884</idno>
					<idno type="doi">10.7910/DVN/J6JNVK</idno>
					
					<author>Azim Ahmadzadeh</author><author>Rohan Adhyapak</author><author>Kartik Chaurasiya</author><author>Laxmi Alekhya Nagubandi</author><author>V Aparna</author><author>Petrus C Martens</author><author>Alexei Pevtsov</author><author>Luca Bertello</author><author>Alexander Pevtsov</author><author>Naomi Douglas</author><author>Samuel McDonald</author><author>Apaar Bawa</author><author>Eugene Kang</author><author>Riley Wu</author><author>Dustin J Kempton</author><author>Aya Abdelkarem</author><author>Patrick M Copeland</author><author>Sri Harsha Seelamneni</author><author>Azim Ahmadzadeh</author>
				</bibl>
			</sourceDesc>
		</fileDesc>
		<profileDesc>
			<abstract><ab><![CDATA[MAGFiLO is a dataset of manually annotated solar filaments from H-Alpha observations captured by the Global Oscillation Network Group (GONG). This dataset includes over ten thousand annotated filaments, spanning the years 2011 through 2022. Each annotation details one filament&#39;s segmentation, minimum bounding box, spine, and magnetic field chirality. MAGFiLO is the first dataset of its size, enabling advanced deep learning models to identify filaments and their features with unprecedented precision. It also provides a testbed for solar physicists interested in large-scale analysis of filaments.]]></ab></abstract>
		</profileDesc>
	</teiHeader>
	<text><body><div/></body></text>
</TEI>
