<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2022-10-10T09:40:00Z" status="active" updated="2026-04-15T14:56:07Z" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:DataService"><title>ROB SPoCA coronal hole datalink service</title><identifier>ivo://ksb-orb.dc/rob_spoca_ch/q/dl</identifier><curation><publisher>SIDC: Solar Influences Data analysis Center</publisher><creator><name>Benjamin Mampaey</name></creator><date role="updated">2026-04-09T09:04:36Z</date><contact><name>Veronique Delouille</name><address>Royal Observatory of Belgium, Avenue circulaire 3, 1180 Bruxelles,
BELGIQUE</address><email>sidc-support@oma.be</email></contact></curation><content><subject>the-sun</subject><subject>solar-atmosphere</subject><subject>solar-physics</subject><subject>solar-system-astronomy</subject><description> *** SPoCA Coronal Hole *** This service provides a catalog of Coronal
Holes obtained with the Spatial Possibilitistic Clustering Algorithm
(SPoCA). Level 2 AIA 19.3nm images (calibrated and corrected for
degradation) are used, at a cadence of one AIA image every 6 hours.
Only coronal holes older than three days are being reported. Bounding
box and characteristics such as areas and pixel intensity statistics,
on AIA 19.3nm and HMI magnetogram images are provided.</description><referenceURL>https://vo-tap.oma.be/rob_spoca_ch/q/dl/info</referenceURL><contentLevel>General</contentLevel><contentLevel>University</contentLevel><contentLevel>Research</contentLevel></content><rights>This research has been made at the Royal Observatory of Belgium</rights></ri:Resource>