Dst index computation using EUHFORIA Heliosphere model output at L1

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<?xml version="1.0" encoding="UTF-8"?>
<ComputationCapabilities xmlns="https://metadata.pithia.eu/schemas/2.2" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:mrl="http://standards.iso.org/iso/19115/-3/mrl/1.0" xmlns:gco="http://standards.iso.org/iso/19115/-3/gco/1.0" xmlns:xlink="http://www.w3.org/1999/xlink" xsi:schemaLocation="https://metadata.pithia.eu/schemas/2.2 https://metadata.pithia.eu/schemas/2.2/pithia.xsd">
    <!-- 
         For those software tools that may be used by any data provider, use as namespace: pithia 
    -->
    <identifier>
        <PITHIA_Identifier>
            <localID>ComputationCapabilities_KUL_EUHFORIA_Dst</localID>
            <namespace>kul</namespace>
            <version>1</version>
            <creationDate>2022-10-19T09:55:00Z</creationDate>
            <lastModificationDate>2024-03-01T12:00:00Z</lastModificationDate>
        </PITHIA_Identifier>
    </identifier>
    <name>Dst index computation using EUHFORIA Heliosphere model output at L1</name>  
    <description>
	  Calculates Dst time series using O'Brian et al.(2000) algorithm by replacing L1 observation with 
          EUHFORIA synthetic data
    </description>
    <!-- 
        A list of the "capabilities" of the procedure: a description (dimensionality, units) for each observed property that this process can evaluate.
	  Calculates Kp time series using Newell et al. algorithm my replacing L1 observation with EUHFORIA synthetic data
        The dimensionalityTimeline describes the timeline of the measured observed property (e.g. Timeseries, Animation,...).
    -->
    <capabilities>
        <processCapability>
            <name>Dst Index, computed</name>
            <observedProperty xlink:href="https://metadata.pithia.eu/ontology/2.2/observedProperty/MagneticField"/>
            <dimensionalityInstance xlink:href="https://metadata.pithia.eu/ontology/2.2/dimensionalityInstance/0D"/>
            <dimensionalityTimeline xlink:href="https://metadata.pithia.eu/ontology/2.2/dimensionalityTimeline/1DTimeseries"/>
            <cadence unit="minute">10</cadence>
            <units xlink:href="https://metadata.pithia.eu/ontology/2.2/unit/nT"/>
            <qualifier xlink:href="https://metadata.pithia.eu/ontology/2.2/qualifier/Derived"/>
        </processCapability>
    </capabilities>   
    <dataLevel xlink:href="https://metadata.pithia.eu/ontology/2.2/dataLevel/L4"/>
    <type xlink:href="https://metadata.pithia.eu/ontology/2.2/computationType/Model"/>
    <version/>
    <softwareReference/>
    <processingInput>
        <InputOutput>
            <!-- Provide only name and description, no values: this field describes the process, not the observation result. 
            If this processingInput is a parameter that has specific value for the whole collection, use om:parameter field of the DataCollection 
            document to define such NamedValue, point its NamedValue.name to this name below, and use NamedValue.value to set the value -->
            <name>EUHFORIA Heliosphere model computation at L1</name>
            <description>
                <mrl:LE_Source>
                     <mrl:description><gco:CharacterString>
This computation uses O'Brian et al. (2000) technique for Dst evaluation based on the velocity components, 
magnetic field components, and total number density at L1 to obtain Dst based on EUHFORIA model of these parameters
                     </gco:CharacterString></mrl:description>
                </mrl:LE_Source>
            </description>
        </InputOutput>
    </processingInput>
    <algorithm/>
</ComputationCapabilities>