SWIF Model

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  <!--
       First report some required elements from ISO standard for Observation
  -->
  <om:phenomenonTime/><!-- DO NOT USE, we report phenomenon time only in Catalogs -->
  <om:resultTime/>    <!-- DO NOT USE, we report result time only in Catalogs -->
  <om:procedure xlink:href="https://metadata.pithia.eu/resources/2.2/process/noa/CompositeProcess_EIS_SWIF_Model"/>

  <om:observedProperty/>

  <om:featureOfInterest>
    <FeatureOfInterest>
      <namedRegion xlink:href="https://metadata.pithia.eu/ontology/2.2/featureOfInterest/Earth_Ionosphere"/>
    </FeatureOfInterest>
  </om:featureOfInterest>
  <om:result/> <!-- DO NOT USE, we use the CollectionResults below to specify URLs to provider) -->
  <!--
       Now our Data Collection elements next
  -->
  <identifier>
    <PITHIA_Identifier>
      <localID>DataCollection_EIS_SWIF_Model</localID>
      <namespace>noa</namespace>
      <version>1</version>
      <creationDate>2023-05-22T09:55:00Z</creationDate>
      <lastModificationDate>2024-07-22T14:47:00Z</lastModificationDate>
    </PITHIA_Identifier>
  </identifier>
  <name>SWIF Model</name>
  <!-- Type is not allowed here. Comes from procedure ? -->
  <!-- <type xlink:href="https://metadata.pithia.eu/ontology/2.2/instrumentType/IncoherentScatterRadar"/>  -->
  <description>
The SWIF ionospheric forecasting algorithm provides alerts and warnings for upcoming ionospheric storm disturbances and ionospheric forecasts over Europe. 
SWIF combines historical and real-time ionospheric observations with solar wind parameters obtained in real time at L1 point through the cooperation of an 
autoregression forecasting algorithm, namely TSAR that provides real-time ionospheric forecasts up to 24 hours ahead during all possible conditions with an 
empirical method, namely STIM, that formulates the ionospheric storm-time response triggered by solar wind disturbances. 
  </description>
  <type xlink:href="https://metadata.pithia.eu/ontology/2.2/computationType/Model"/>
  <project xlink:href="https://metadata.pithia.eu/resources/2.2/project/noa/Project_NOA_EIS"/>
  <relatedParty>
    <ResponsiblePartyInfo>
      <role xlink:href="https://metadata.pithia.eu/ontology/2.2/relatedPartyRole/PointOfContact"/>
      <party xlink:href="https://metadata.pithia.eu/resources/2.2/individual/noa/Individual_NOA_Belehaki"/>
    </ResponsiblePartyInfo>
  </relatedParty>
  <relatedParty>
    <ResponsiblePartyInfo>
      <role xlink:href="https://metadata.pithia.eu/ontology/2.2/relatedPartyRole/DataProvider"/>
      <party xlink:href="https://metadata.pithia.eu/resources/2.2/organisation/pithia/Organisation_NOA"/>
    </ResponsiblePartyInfo>
  </relatedParty>

  <collectionResults>
    <source>
      <OnlineResource>
        <serviceFunction xlink:href="https://metadata.pithia.eu/ontology/2.2/serviceFunction/Download"/>
        <linkage><gmd:URL>https://swe.ssa.esa.int/dias-federated</gmd:URL></linkage>
        <name>European Ionosonde Service (EIS) Interface</name>
        <protocol>HTTPS</protocol>
        <description>
		The EIS provides a browser-based user interface for data browsing and downloading. 
		Direct data access requires authentication by external organisation (ESA); once user access is authorised the link lands directly at the EIS page. 
		Three products derive from the SWIF Model: (a) foF2 Forecasts Maps, (b) foF2 Forecasts Plots Over Stations and (c) Ionospheric Alerts.  
		</description>
        <dataFormat xlink:href="https://metadata.pithia.eu/ontology/2.2/resultDataFormat/text-plain"/>
		<dataFormat xlink:href="https://metadata.pithia.eu/ontology/2.2/resultDataFormat/image-png"/>
      </OnlineResource>
    </source> 
    <source>
      <OnlineResource>
        <serviceFunction xlink:href="https://metadata.pithia.eu/ontology/2.2/serviceFunction/Application"/>
        <linkage><gmd:URL>https://electron.space.noa.gr/swif/api/v2/docs#/idb</gmd:URL></linkage>
        <name>SWIF API</name>
        <protocol>HTTPS</protocol>
        <description>
		The SWIF API provides a browser-based user interface for data browsing and downloading.
		API parameters: (I) Endpoint /swifdb/stations: Active stations over a given interval. 
		(II) Endpoint /swifdb/tsar/covstats: Info on the number of the available data per year/month/day per station over a given interval.
		Parameter stations: select the station of interest. 
		(III) Endpoint /swifdb/tsar/rangestats: Info on the data temporal availabilty per station.
		Parameter stations: select the station of interest. 
		(IV) Endpoint /swifdb/forecasts: Forecast foF2 values for the next 24 hours over each Digisonde station.
		Parameter stations: select the station of interest. 
		(V) Endpoint /swifdb/forecasts/pager: Forecast foF2 values for the next 24 hours over each Digisonde station.
		Parameter stations: select the station of interest. 
		By using this endpoint (pager) you divide a large dataset into smaller pages without temporal restrictions.
		(VI) Endpoint /swifdb/forecasts_df: Forecast foF2 values for the next 24 hours over each Digisonde station. 
		Apache Arrow - Pandas DataFrame compatible columnar data structure.
		Parameter stations: select the station of interest. Parameter attributes: requested column names.
		(VII) Endpoint /swifdb/forecasts_sync_df: Forecast foF2 values for the next 24 hours over each Digisonde station.
		Forecasts as Dataframe (complex sync request: ForecastsCov sync)
		(VIII) Endpoint /swifdb/solardb/magdata: DSCOVR mission Magdata records (Bmag, Bx, By, Bz).
		(IX) Endpoint /swifdb/solardb/magdata/pager: DSCOVR mission Magdata records (Bmag, Bx, By, Bz).
		By using this endpoint (pager) you divide a large dataset into smaller pages without temporal restrictions.
		(X) Endpoint /swifdb/solardb/magdata_df: DSCOVR mission Magdata records (Bmag, Bx, By, Bz).
		Apache Arrow - Pandas DataFrame compatible columnar data structure.
		(XI) Endpoint /swifdb/stim/storms: Interplanetary storms detected.
		Parameter local: [false] if you want info about the interplanetary storm only or [true] if you want to get info about the local (at the Digisonde stations) stroms as well.
		Each storm has a UUID "id" that can be used in the /swifdb/stim/storm/{pubid} or/and /swifdb/stim/istorm/{pubid} endpoint for retrieving the relevant info.
		(XII) Endpoint /swifdb/stim/storm/{pubid}: Interplanetary storms detected.
		Parameter pubid: the UUID "id" of a distinct interplanetary storm.
		(XIII) Endpoint /swifdb/stim/istorms: Local storms detected.
		Parameter stations: select the station(s) of interest.
		Parameter parent: [false] if you want info about the local (at the Digisonde station) storm only or [true] if you want to get info about the interplanetary storm as well.
		Each storm has a UUID "id" that can be used in the /swifdb/stim/storm/{pubid} or/and /swifdb/stim/istorm/{pubid} endpoint for retrieving the relevant info.
		(XIV) Endpoint /swifdb/stim/istorm/{pubid}: Local storms detected.
		Parameter pubid: the UUID "id" of a distinct local storm.
		(XV) Endpoint /swifdb/tsar/stormstats: Temporal statistics.
		Number of interplanetary storms detected over a given interval.
		</description>
        <dataFormat xlink:href="https://metadata.pithia.eu/ontology/2.2/resultDataFormat/application-json"/>
      </OnlineResource>
    </source> 
  </collectionResults>

  <dataLevel xlink:href="https://metadata.pithia.eu/ontology/2.2/dataLevel/L4"/>
  <qualityAssessment>
    <dataQualityFlag xlink:href="https://metadata.pithia.eu/ontology/2.2/dataQualityFlag/DQ4"/>
  </qualityAssessment>
  <permission xlink:href="https://metadata.pithia.eu/ontology/2.2/licence/CCBY"/>
</DataCollection>