SPASE Metadata Validator

Enter the URL or local path to the SPASE description, then click "Validate".
You can also select the version of the data model to use and whether to check external references like Resource IDs and URLs.

URL: 
-or-
File: 
   
SPASE Data Model Version:  In XML  2.7.0  2.6.1  2.6.0  2.5.0  2.4.1  2.4.0  2.3.2  2.3.1  2.3.0  2.2.9  2.2.8  2.2.6  2.2.4  2.2.3  2.2.2  2.2.1  2.2.0  2.1.0  2.0.3  2.0.2  2.0.1  2.0.0  1.2.2  1.2.0  1.1.0  sim-1.0.0
Check References: Resource ID URL

Using schema: https://spase-group.org/data/schema/spase-1_1_0.xsd
Using URL: https://spase-group.org/data/schema/spase-1_1_0.xsd Error: schema_reference.4: Failed to read schema document 'https://spase-group.org/data/schema/spase-1_1_0.xsd', because 1) could not find the document; 2) the document could not be read; 3) the root element of the document is not . Validating null:
http://spase-validator.heliocloud.org/examples/WindWavesTNR-2.xml

Line -1 schema_reference.4: Failed to read schema document 'https://spase-group.org/data/schema/spase-1_1_0.xsd', because 1) could not find the document; 2) the document could not be read; 3) the root element of the document is not .

1<?xml version="1.0" encoding="UTF-8"?>
2<Spase xmlns="http://www.spase-group.org/data/schema">
3<Version>1.1.0</Version>
4<Instrument>
5    <ResourceID>spase://example/instrument</ResourceID>
6    <ResourceHeader>
7        <ResourceName>Wind Waves Thermal Noise Receiver</ResourceName>
8         <AlternateName>Thermal Noise Receiver</AlternateName>
9         <ReleaseDate>2004-10-01T00:00:00</ReleaseDate>
10        <Description>The Thermal Noise Receiver (TNR) on the WIND
11            spacecraft is an instrument of a new generation, which is
12            flown for the first time. It utilizes a digital spectrum
13            analysis technique similar to a wavelet transform analysis.
14            This permits a high time resolution, associated to a high
15            frequency resolution. It was essentially designed to measure
16            the thermal noise at a high rate. The interest of this
17            receiver also covers other events, both in situ (plasma
18            waves, ion acoustic waves) and remotely detected (solar and
19            magnetospheric radio bursts). However, this receiver uses a
20            compression technique which limits the study of high
21            intensity events. Namely, the digital dynamic range is about
22            45 dB, added to an AGC range of more than 60 dB, the AGC
23            acting as a sensitivity adjustment. (e.g. an 80 dB event
24            will not saturate the receiver, but the computed spectrum
25            will only cover its upper 45 dB.)</Description>
26        <Contact>
27            <PersonID>CDPP:PR:IssautierIsabelle</PersonID>
28            <Role>CoInvestigator</Role>
29        </Contact>
30    </ResourceHeader>
31    <InstrumentType>SpectralPowerReceiver</InstrumentType>
32    <InvestigationName/>
33    <ObservatoryID>spase://test/observatory</ObservatoryID>
34    <Caveats/>
35</Instrument>
36</Spase>