<?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_Corona</localID>
<namespace>kul</namespace>
<version>1</version>
<creationDate>2022-10-19T09:55:00Z</creationDate>
<lastModificationDate>2023-04-25T11:27:00Z</lastModificationDate>
</PITHIA_Identifier>
</identifier>
<name>EUHFORIA: Solar wind boundary conditions</name>
<description>
Calculates characteristics of the solar wind boundary at 0.1 AU.
</description>
<!--
A list of the "capabilities" of the procedure: a description (dimensionality, units) for each observed property that this process can evaluate.
The dimensionalityInstance describes the data domain of the single instance of the measured observed property (1D.point, 1D.Profile, 2D.Map, 2D.image..).
The dimensionalityTimeline describes the timeline of the measured observed property (e.g. Timeseries, Animation,...).
-->
<capabilities>
<processCapability>
<name>Solar wind speed at 0.1 AU</name>
<observedProperty xlink:href="https://metadata.pithia.eu/ontology/2.2/observedProperty/ElectronVelocity_Heliosphere"/>
<dimensionalityInstance xlink:href="https://metadata.pithia.eu/ontology/2.2/dimensionalityInstance/2DMap"/>
<vectorRepresentation xlink:href="https://metadata.pithia.eu/ontology/2.2/component/radial"/>
<coordinateSystem xlink:href="https://metadata.pithia.eu/ontology/2.2/scs/Stonyhurst"/>
<units xlink:href="https://metadata.pithia.eu/ontology/2.2/unit/ms-1"/>
</processCapability>
<processCapability>
<name>Plasma number density at 0.1 AU</name>
<observedProperty xlink:href="https://metadata.pithia.eu/ontology/2.2/observedProperty/ElectronDensity"/>
<dimensionalityInstance xlink:href="https://metadata.pithia.eu/ontology/2.2/dimensionalityInstance/2DMap"/>
<units xlink:href="https://metadata.pithia.eu/ontology/2.2/unit/m-3"/>
</processCapability>
<processCapability>
<name>Plasma temperature at 0.1 AU</name>
<observedProperty xlink:href="https://metadata.pithia.eu/ontology/2.2/observedProperty/PlasmaTemperature_MHD"/>
<dimensionalityInstance xlink:href="https://metadata.pithia.eu/ontology/2.2/dimensionalityInstance/2DMap"/>
<units xlink:href="https://metadata.pithia.eu/ontology/2.2/unit/K"/>
</processCapability>
<processCapability>
<name>Magnetic field at 0.1 AU</name>
<observedProperty xlink:href="https://metadata.pithia.eu/ontology/2.2/observedProperty/MagneticField"/>
<dimensionalityInstance xlink:href="https://metadata.pithia.eu/ontology/2.2/dimensionalityInstance/2DMap"/>
<vectorRepresentation xlink:href="https://metadata.pithia.eu/ontology/2.2/component/radial"/>
<coordinateSystem xlink:href="https://metadata.pithia.eu/ontology/2.2/scs/Stonyhurst"/>
<units xlink:href="https://metadata.pithia.eu/ontology/2.2/unit/T"/>
</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/>
<!-- Use ESPAS-inspired design of processingInput and InputOutput types to specify all required input parameters for this computation -->
<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>GONG or GONG-ADAPT solar photospheriic magnetogram</name>
<description>
<mrl:LE_Source>
<mrl:description><gco:CharacterString>
The solar wind speed is calculated as a function of the flux tube expansion
factor and the distance of the foot-point of the flux tube to the nearest coronal
hole boundary. The radial component of the magnetic field and the plasma density are
computed as a function of the wind speed. The plasma temperature is determined as a
function of the plasma density.
</gco:CharacterString></mrl:description>
</mrl:LE_Source>
</description>
</InputOutput>
</processingInput>
<processingInput>
</processingInput>
<algorithm/>
</ComputationCapabilities>
