Updated the ObservedRegion of the ESA/NumericalData/SOHO/GOLF/MissionLong.xml

Author: seijiyashiro

NumericalData/SOHO/GOLF/SSA_SDAC.xml

@@ -1,6 +1,6 @@
 <?xml version="1.0" encoding="UTF-8"?>
-<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema  http://www.spase-group.org/data/schema/spase-2_6_1.xsd">
-   <Version>2.6.1</Version>
+<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema  http://www.spase-group.org/data/schema/spase-2_7_0.xsd">
+   <Version>2.7.0</Version>
    <NumericalData>
       <ResourceID>spase://ESA/NumericalData/SOHO/GOLF/SSA_SDAC</ResourceID>
       <ResourceHeader>
@@ -11,10 +11,14 @@
                <ReleaseDate>2024-08-14T00:08:46</ReleaseDate>
                <Note>Metadata created by SY</Note>
             </RevisionEvent>
+            <RevisionEvent>
+               <ReleaseDate>2025-09-30T00:08:46</ReleaseDate>
+               <Note>Updated the ObservedRegion</Note>
+            </RevisionEvent>
          </RevisionHistory>
          <Description>The Global Oscillation at Low Frequencies (GOLF) investigation will perform uninterrupted velocity oscillation and magnetic field measurements of the full solar disk, spatially unresolved, with extremely high sensitivity (&lt;1 mm/s and 1 milligauss). To determine the velocity, the Doppler effect is measured by the resonant scattering technique. A resonant cell filled with sodium vapor in a strong magnetic field enables, by the Zeeman effect, the selective absorption of light in the two wings of the solar D lines. A comparison of the intensity on both sides of the line leads to an extremely sensitive determination of the velocity. This information is from the paper SOHO - An Observatory to Study the Solar Interior and the Solar Atmosphere,&#039;&#039; by A. I. Poland and V. Domingo (inObservatories in Earth Orbit and Beyond,&#039;&#039; pp. 277-284, ed. by Y. Kondo, Kluwer Academic Publishers, Dordrecht, 1990).</Description>
          <PublicationInfo>
-            <Authors>The GOLF Consortium: Institut d&#039;Astrophysique Spatiale (France); Département d&#039;Astrophysique, Université de Nice (France); Observatoire de l&#039;Université Bordeaux 1 (France); Instituto de Astrofísica de Canarias (Spain); Service d&#039;Astrophysique (France); Service d&#039;Aéronomie (France); Observatoire de la Côte d&#039;Azur (France); </Authors>
+            <Authors>The GOLF Consortium: Institut d&#039;Astrophysique Spatiale (France); Département d&#039;Astrophysique, Université de Nice (France); Observatoire de l&#039;Université Bordeaux 1 (France); Instituto de Astrofísica de Canarias (Spain); Service d&#039;Astrophysique (France); Service d&#039;Aéronomie (France); Observatoire de la Côte d&#039;Azur (France);</Authors>
             <PublicationDate>1996-01-01T00:00:00</PublicationDate>
             <PublishedBy>SOHO Science Archive at the European Space Astronomy Centre</PublishedBy>
          </PublicationInfo>
@@ -66,6 +70,7 @@
          </TimeSpan>
       </TemporalDescription>
       <ObservedRegion>Sun</ObservedRegion>
+      <ObservedRegion>Sun.Interior</ObservedRegion>
       <ObservedRegion>Sun.Photosphere</ObservedRegion>
    </NumericalData>
 </Spase>