Commit e0a27e032b4e63c80446072cd818166e1e2849a6

Authored by Elena.Budnik
1 parent 3a733206

morch, cain models

NumericalData/AMDA/ACE/MFI/ace-mag-real.xml
... ... @@ -53,7 +53,7 @@
53 53 <TemporalDescription>
54 54 <TimeSpan>
55 55 <StartDate>2014-01-06T00:00:00Z</StartDate>
56   - <StopDate>2017-02-28T00:59:59Z</StopDate>
  56 + <StopDate>2017-03-01T00:59:59Z</StopDate>
57 57 </TimeSpan>
58 58 <Cadence>PT60S</Cadence>
59 59 </TemporalDescription>
... ...
NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml
... ... @@ -48,7 +48,7 @@
48 48 <TemporalDescription>
49 49 <TimeSpan>
50 50 <StartDate>2014-01-06T00:00:00Z</StartDate>
51   - <StopDate>2017-02-28T00:59:59Z</StopDate>
  51 + <StopDate>2017-03-01T00:59:59Z</StopDate>
52 52 </TimeSpan>
53 53 <Cadence>PT60S</Cadence>
54 54 </TemporalDescription>
... ...
NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml
... ... @@ -49,7 +49,7 @@
49 49 <TemporalDescription>
50 50 <TimeSpan>
51 51 <StartDate>2014-06-01T00:00:00Z</StartDate>
52   - <StopDate>2017-02-14T19:12:00Z</StopDate>
  52 + <StopDate>2017-02-21T19:42:00Z</StopDate>
53 53 </TimeSpan>
54 54 <Cadence>PT1M</Cadence>
55 55 </TemporalDescription>
... ...
NumericalData/AMDA/MAVEN/SEP/mvn-sep1-clb.xml
... ... @@ -44,7 +44,7 @@
44 44 <TemporalDescription>
45 45 <TimeSpan>
46 46 <StartDate>2014-09-22T19:34:31Z</StartDate>
47   - <StopDate>2016-08-15T00:00:12Z</StopDate>
  47 + <StopDate>2016-11-15T00:00:09Z</StopDate>
48 48 </TimeSpan>
49 49 <Cadence_Min>PT2S</Cadence_Min>
50 50 <Cadence_Max>PT32S</Cadence_Max>
... ...
NumericalData/AMDA/MAVEN/SEP/mvn-sep2-clb.xml
... ... @@ -44,7 +44,7 @@
44 44 <TemporalDescription>
45 45 <TimeSpan>
46 46 <StartDate>2014-09-22T19:34:33Z</StartDate>
47   - <StopDate>2016-08-15T00:00:12Z</StopDate>
  47 + <StopDate>2016-11-15T00:00:09Z</StopDate>
48 48 </TimeSpan>
49 49 <Cadence_Min>PT2S</Cadence_Min>
50 50 <Cadence_Max>PT32S</Cadence_Max>
... ...
NumericalData/AMDA/MAVEN/SWEA/mavpds-swea-svyspec.xml
... ... @@ -46,7 +46,7 @@
46 46 <TemporalDescription>
47 47 <TimeSpan>
48 48 <StartDate>2014-03-19T14:15:52Z</StartDate>
49   - <StopDate>2016-08-14T23:59:59Z</StopDate>
  49 + <StopDate>2016-11-15T00:00:00Z</StopDate>
50 50 </TimeSpan>
51 51 <Cadence>PT4S</Cadence></TemporalDescription>
52 52 <ObservedRegion>Mars</ObservedRegion>
... ...
NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-momboard.xml
... ... @@ -48,7 +48,7 @@
48 48 <TemporalDescription>
49 49 <TimeSpan>
50 50 <StartDate>2014-03-19T14:19:43Z</StartDate>
51   - <StopDate>2016-08-15T00:01:00Z</StopDate>
  51 + <StopDate>2016-11-15T00:00:13Z</StopDate>
52 52 </TimeSpan>
53 53 <Cadence>PT4S</Cadence></TemporalDescription>
54 54 <ObservedRegion>Mars</ObservedRegion>
... ...
NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-specboard.xml
... ... @@ -45,7 +45,7 @@
45 45 <TemporalDescription>
46 46 <TimeSpan>
47 47 <StartDate>2014-03-19T14:20:43Z</StartDate>
48   - <StopDate>2016-08-15T00:00:56Z</StopDate>
  48 + <StopDate>2016-11-15T00:00:05Z</StopDate>
49 49 </TimeSpan>
50 50 <Cadence>PT4S</Cadence></TemporalDescription>
51 51 <ObservedRegion>Mars</ObservedRegion>
... ...
NumericalOutput/AMDA/CAIN/b_cain.xml
... ... @@ -9,15 +9,19 @@
9 9 <Description>Cain model martian crustal magnetic field along s/c orbit is being real-time calculated.
10 10 S/c and sampling time should be defined by user.
11 11 </Description>
12   - <Acknowledgement>TBD</Acknowledgement>
  12 + <Acknowledgement/>
  13 + <Contact>
  14 + <PersonID>spase://CDPP/Person/Joseph.C.Cain</PersonID>
  15 + <Role>PrincipalInvestigator</Role>
  16 + </Contact>
13 17 <Contact>
14   - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
  18 + <PersonID>spase://CDPP/Person/Elena.Budnik</PersonID>
15 19 <Role>TechnicalContact</Role>
16 20 </Contact>
17 21 <InformationURL>
18   - <Name>Rules of use, and caveats</Name>
19   - <URL>TBD</URL>
20   - <Description>TBD</Description>
  22 + <Name>Model description</Name>
  23 + <URL>http://onlinelibrary.wiley.com/doi/10.1029/2000JE001487/full</URL>
  24 + <Description/>
21 25 </InformationURL>
22 26 </ResourceHeader>
23 27 <AccessInformation>
... ... @@ -31,7 +35,7 @@
31 35 </URL>
32 36 </AccessURL>
33 37 <Format>Text.ASCII</Format>
34   - <Acknowledgement>TBD</Acknowledgement>
  38 + <Acknowledgement/>
35 39 </AccessInformation>
36 40 <SimulationRunID>spase://CDPP/SimulationRun/AMDA/CAIN/CainRun</SimulationRunID>
37 41 <MeasurementType>MagneticField</MeasurementType>
... ... @@ -40,27 +44,23 @@
40 44 <StartDate>1970-01-01T00:00:00Z</StartDate>
41 45 <StopDate>1970-01-01T00:00:00Z</StopDate>
42 46 </TimeSpan>
43   - <Cadence>UserDefined</Cadence>
  47 + <Cadence>PTUserDefined</Cadence>
44 48 </TemporalDescription>
45 49 <SimulatedRegion>Mars</SimulatedRegion>
46   - <Caveats>
47   - TBD
48   - </Caveats>
  50 + <Caveats/>
49 51 <InputResourceID/>
50 52 <Parameter>
51 53 <Name>b mso</Name>
52 54 <ParameterKey>bcain_mso</ParameterKey>
53 55 <Description/>
54   - <Caveats>
55   - TBD
56   - </Caveats>
  56 + <Caveats/>
57 57 <Units>nT</Units>
58 58 <Structure>
59 59 <Size>3</Size>
60 60 <Element>
61 61 <Name>bx</Name>
62 62 <Qualifier>Component.I</Qualifier>
63   - <Index/>
  63 + <Index>1</Index>
64 64 <ParameterKey>bcain_mso(0)</ParameterKey>
65 65 <ValidMin/>
66 66 <ValidMax/>
... ... @@ -69,7 +69,7 @@
69 69 <Element>
70 70 <Name>by</Name>
71 71 <Qualifier>Component.J</Qualifier>
72   - <Index/>
  72 + <Index>2</Index>
73 73 <ParameterKey>bcain_mso(1)</ParameterKey>
74 74 <ValidMin/>
75 75 <ValidMax/>
... ... @@ -78,7 +78,7 @@
78 78 <Element>
79 79 <Name>bz</Name>
80 80 <Qualifier>Component.K</Qualifier>
81   - <Index/>
  81 + <Index>3</Index>
82 82 <ParameterKey>bcain_mso(2)</ParameterKey>
83 83 <ValidMin/>
84 84 <ValidMax/>
... ... @@ -93,10 +93,8 @@
93 93 <Parameter>
94 94 <Name>b tot</Name>
95 95 <ParameterKey>bcain_tot</ParameterKey>
96   - <Description> TBD </Description>
97   - <Caveats>
98   - TBD
99   - </Caveats>
  96 + <Description/>
  97 + <Caveats/>
100 98 <Units>nT</Units>
101 99 <FillValue>NaN</FillValue>
102 100 <Field>
... ...
NumericalOutput/AMDA/MORSCHHAUSER/b_morschhauser.xml
... ... @@ -4,20 +4,27 @@
4 4 <NumericalOutput>
5 5 <ResourceID>spase://CDPP/NumericalOutput/AMDA/MORSCHAUSER/b_morschhauser</ResourceID>
6 6 <ResourceHeader>
7   - <ResourceName>Morschhauser B</ResourceName>
8   - <ReleaseDate>2014-07-08T16:49:29Z</ReleaseDate>
9   - <Description>TBD</Description>
10   - <Acknowledgement>TBD</Acknowledgement>
11   - <Contact>
12   - <PersonID>TBD</PersonID>
13   - <Role>PrincipalInvestigator</Role>
14   - </Contact>
  7 + <ResourceName>Morschhauser B along s/c orbit</ResourceName>
  8 + <ReleaseDate>2017-03-08T16:49:29Z</ReleaseDate>
  9 + <Description>Morschhauser model martian crustal magnetic field along s/c orbit is being real-time calculated.
  10 + S/c and sampling time should be defined by user.</Description>
  11 + <Acknowledgement/>
  12 + <Contact>
  13 + <PersonID>spase://CDPP/Person/A.Morschhauser</PersonID>
  14 + <Role>PrincipalInvestigator</Role>
  15 + </Contact>
  16 + <Contact>
  17 + <PersonID>spase://CDPP/Person/A.Beth</PersonID>
  18 + <Role>TechnicalContact</Role>
  19 + </Contact>
  20 + <Contact>
  21 + <PersonID>spase://CDPP/Person/Elena.Budnik</PersonID>
  22 + <Role>TechnicalContact</Role>
  23 + </Contact>
15 24 <InformationURL>
16   - <Name>Rules of use, and caveats</Name>
17   - <URL>
18   - TBD
19   - </URL>
20   - <Description>TBD</Description>
  25 + <Name>Model description</Name>
  26 + <URL>http://onlinelibrary.wiley.com/doi/10.1002/2013JE004555/abstract</URL>
  27 + <Description/>
21 28 </InformationURL>
22 29 </ResourceHeader>
23 30 <AccessInformation>
... ... @@ -31,9 +38,7 @@
31 38 </URL>
32 39 </AccessURL>
33 40 <Format>Text.ASCII</Format>
34   - <Acknowledgement>
35   - TBD
36   - </Acknowledgement>
  41 + <Acknowledgement/>
37 42 </AccessInformation>
38 43 <SimulationRunID>spase://CDPP/SimulationRun/AMDA/MORSCHHAUSER/MorschhauserRun</SimulationRunID>
39 44 <MeasurementType>MagneticField</MeasurementType>
... ... @@ -42,27 +47,22 @@
42 47 <StartDate>1970-01-01T00:00:00Z</StartDate>
43 48 <StopDate>1970-01-01T00:00:00Z</StopDate>
44 49 </TimeSpan>
45   - <Cadence/>
  50 + <Cadence>PTUserDefined</Cadence>
46 51 </TemporalDescription>
47 52 <SimulatedRegion>Mars</SimulatedRegion>
48   - <Caveats>
49   - TBD
50   - </Caveats>
  53 + <Caveats>Field is calculated for the altitudes less than 450 km</Caveats>
51 54 <InputResourceID/>
52 55 <Parameter>
53 56 <Name>b mso</Name>
54 57 <ParameterKey>bmorsch_mso</ParameterKey>
55 58 <Description/>
56   - <Caveats>
57   - TBD
58   - </Caveats>
59 59 <Units>nT</Units>
60 60 <Structure>
61 61 <Size>3</Size>
62 62 <Element>
63 63 <Name>bx</Name>
64   - <Qualifier/>
65   - <Index/>
  64 + <Qualifier>Component.I</Qualifier>
  65 + <Index>1</Index>
66 66 <ParameterKey>bmorsch_mso(0)</ParameterKey>
67 67 <ValidMin/>
68 68 <ValidMax/>
... ... @@ -70,8 +70,8 @@
70 70 </Element>
71 71 <Element>
72 72 <Name>by</Name>
73   - <Qualifier/>
74   - <Index/>
  73 + <Qualifier>Component.J</Qualifier>
  74 + <Index>2</Index>
75 75 <ParameterKey>bmorsch_mso(1)</ParameterKey>
76 76 <ValidMin/>
77 77 <ValidMax/>
... ... @@ -79,25 +79,28 @@
79 79 </Element>
80 80 <Element>
81 81 <Name>bz</Name>
82   - <Qualifier/>
83   - <Index/>
  82 + <Qualifier>Component.K</Qualifier>
  83 + <Index>3</Index>
84 84 <ParameterKey>bmorsch_mso(2)</ParameterKey>
85 85 <ValidMin/>
86 86 <ValidMax/>
87 87 <FillValue/>
88 88 </Element>
89 89 </Structure>
90   - <FillValue>NaN</FillValue>
  90 + <FillValue>NaN</FillValue>
  91 + <Field>
  92 + <FieldQuantity>Magnetic</FieldQuantity>
  93 + </Field>
91 94 </Parameter>
92 95 <Parameter>
93 96 <Name>b_tot</Name>
94 97 <ParameterKey>bmorsch_tot</ParameterKey>
95   - <Description> TBD </Description>
96   - <Caveats>
97   - TBD
98   - </Caveats>
  98 + <Description/>
99 99 <Units>nT</Units>
100   - <FillValue>NaN</FillValue>
  100 + <FillValue>NaN</FillValue>
  101 + <Field>
  102 + <FieldQuantity>Magnetic</FieldQuantity>
  103 + </Field>
101 104 </Parameter>
102 105 </NumericalOutput>
103 106 </Spase>
... ...
NumericalOutput/AMDA/TAO/Jupiter/tao-jup-swrt.xml
... ... @@ -43,7 +43,7 @@
43 43 <TemporalDescription>
44 44 <TimeSpan>
45 45 <StartDate>2017-01-06T00:00:00Z</StartDate>
46   - <StopDate>2017-02-28T00:00:00Z</StopDate>
  46 + <StopDate>2017-03-01T00:00:00Z</StopDate>
47 47 </TimeSpan>
48 48 <Cadence>PT1H</Cadence>
49 49 </TemporalDescription>
... ...
NumericalOutput/AMDA/TAO/Mars/tao-mars-swrt.xml
... ... @@ -43,7 +43,7 @@
43 43 <TemporalDescription>
44 44 <TimeSpan>
45 45 <StartDate>2017-01-06T00:00:00Z</StartDate>
46   - <StopDate>2017-02-28T00:00:00Z</StopDate>
  46 + <StopDate>2017-03-01T00:00:00Z</StopDate>
47 47 </TimeSpan>
48 48 <Cadence>PT1H</Cadence>
49 49 </TemporalDescription>
... ...
NumericalOutput/AMDA/TAO/Saturn/tao-sat-sw.xml
... ... @@ -43,7 +43,7 @@
43 43 <TemporalDescription>
44 44 <TimeSpan>
45 45 <StartDate>1990-01-01T01:30:00Z</StartDate>
46   - <StopDate>2017-01-01T00:00:00Z</StopDate>
  46 + <StopDate>2017-01-21T00:00:00Z</StopDate>
47 47 </TimeSpan>
48 48 <Cadence>PT1H</Cadence>
49 49 </TemporalDescription>
... ...
Observatory/AMDA/STEREO.xml
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>STEREO</ResourceName>
8 8 <AlternateName>Solar Terrestrial Relations Observatory; NASA</AlternateName>
9   - <ReleaseDate>2010-09-25T03:09:48Z</ReleaseDate>
  9 + <ReleaseDate>2017-02-25T03:09:48Z</ReleaseDate>
10 10 <Description>The Solar-Terrestrial Relations Observatory (STEREO) mission includes two spacecraft respectively lagging (STEREO A) and leading (STEREO B) the Earth in heliocentric orbit around the Sun for remote 3-D imaging and radio observations of coronal mass ejections (CMEs). These events are responsible for large solar energetic particle events in interplanetary space and are the primary cause of major geomagnetic storms at Earth. The two spacecraft are launched to drift slowly away from the Earth in opposite directions at about 10 degrees per year for the lagging spacecraft and 20 degrees per year for the leading one. Optimal longitudinal separation of about sixty degrees is achieved after two years. Afterwards the separation gradually increases beyond the design lifetime of two years with the possibility of extended mission observations at larger angles. Science instruments selected for STEREO include the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) for extreme ultraviolet (EUV), white-light coronographic, and heliospheric imaging, the STEREO/WAVES (SWAVES) interplanetary radio burst tracker, the In situ Measurements of Particles and CME Transients (IMPACT) investigation for in-situ sampling the 3-D distribution and plasma characteristics of solar energetic particles and the interplanetary magnetic field, and the PLAsma and SupraThermal Ion and Composition (PLASTIC) experiment to measure elemental and charge composition of ambient and CME plasma ions. STEREO data recorded and stored onboard each spacecraft will be downlinked through the NASA Deep Space Network on a daily schedule. Real-time space weather data will be continuously transmitted through a separate beacon system to NASA and non-NASA receiving stations.</Description>
11 11 <Contact>
12 12 <!-- Mike Kaiser -->
... ...
Person/A.Beth.xml 0 → 100644
... ... @@ -0,0 +1,10 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_2_0.xsd">
  3 + <Version>2.2.0</Version>
  4 + <Person>
  5 + <ResourceID>spase://CDPP/Person/A.Beth</ResourceID>
  6 + <PersonName>Dr. Arnaud A. Beth</PersonName>
  7 + <OrganizationName>Currently : Imperial College, UK</OrganizationName>
  8 + <Email>a.beth@imperial.ac.uk</Email>
  9 + </Person>
  10 +</Spase>
... ...
Person/A.Morschhauser.xml 0 → 100644
... ... @@ -0,0 +1,10 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_2_0.xsd">
  3 + <Version>2.2.0</Version>
  4 + <Person>
  5 + <ResourceID>spase://CDPP/Person/A.Morschauser</ResourceID>
  6 + <PersonName>Dr. Achim Morschhauser</PersonName>
  7 + <OrganizationName>Department of Planetary Physics, German Aerospace Center, Berlin, Germany</OrganizationName>
  8 + <Email>achim.morschhauser@dlr.de</Email>
  9 + </Person>
  10 +</Spase>
... ...
SimulationModel/AMDA/Cain.xml
... ... @@ -6,10 +6,10 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Cain Model</ResourceName>
8 8 <AlternateName>Cain martian crustal magnetic field model</AlternateName>
9   - <ReleaseDate>2014-07-08T14:48:29Z</ReleaseDate>
  9 + <ReleaseDate>2017-02-08T14:48:29Z</ReleaseDate>
10 10 <Description>Spherical Harmonic</Description>
11 11 <Contact>
12   - <PersonID>TBD</PersonID>
  12 + <PersonID>spase://CDPP/Person/Joseph.C.Cain</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Association>
... ... @@ -18,6 +18,6 @@
18 18 <Note>Magnetic Field Models</Note>
19 19 </Association>
20 20 </ResourceHeader>
21   - <SimulationType>Spherical Harmonic</SimulationType>
  21 + <SimulationType>SphericalHarmonic</SimulationType>
22 22 </SimulationModel>
23 23 </Spase>
... ...
SimulationModel/AMDA/Morschhauser.xml
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Morschhauser Model</ResourceName>
8 8 <AlternateName>Morschhauser Mars Crustal magnetic Field Model</AlternateName>
9   - <ReleaseDate>2014-07-08T14:48:29Z</ReleaseDate>
  9 + <ReleaseDate>2017-01-08T14:48:29Z</ReleaseDate>
10 10 <Description>Spherical Harmonic</Description>
11 11 <Contact>
12 12 <PersonID>Morschhauser</PersonID>
... ... @@ -18,6 +18,6 @@
18 18 <Note>Magnetic Field Models</Note>
19 19 </Association>
20 20 </ResourceHeader>
21   - <SimulationType>Spherical Harmonic</SimulationType>
  21 + <SimulationType>SphericalHarmonic</SimulationType>
22 22 </SimulationModel>
23 23 </Spase>
... ...
SimulationRun/AMDA/CAIN/CainRun.xml
... ... @@ -35,7 +35,7 @@ INhundred nT in components calculated for areodetic altitudes below 200 km.
35 35 <Role>PrincipalInvestigator</Role>
36 36 </Contact>
37 37 <Contact>
38   - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
  38 + <PersonID>spase://CDPP/Person/Elena.Budnik</PersonID>
39 39 <Role>TechnicalContact</Role>
40 40 </Contact>
41 41 </ResourceHeader>
... ...
SimulationRun/AMDA/MORSCHHAUSER/MorschhauserRun.xml
... ... @@ -4,14 +4,18 @@
4 4 <SimulationRun>
5 5 <ResourceID>spase://CDPP/SimulationRun/AMDA/MORSCHAUSER/MorschhauserRun</ResourceID>
6 6 <ResourceHeader>
7   - <ResourceName>Morschauser Model</ResourceName>
8   - <AlternateName>Mars Model B Field alog s/c orbit</AlternateName>
9   - <ReleaseDate>2014-07-08T14:48:29Z</ReleaseDate>
10   - <Description></Description>
  7 + <ResourceName>Morschhauser Model</ResourceName>
  8 + <AlternateName>Morschhauser Model model of martian crustal magnetic field</AlternateName>
  9 + <ReleaseDate>2017-03-08T14:48:29Z</ReleaseDate>
  10 + <Description>Model of the lithospheric magnetic field of Mars is based on Mars Global Surveyor orbiting satellite data and represented by an expansion of spherical harmonic (SH) functions up to degree and order 110. Several techniques were applied in order to obtain a reliable and well-resolved model of the Martian lithospheric magnetic field: A modified Huber-Norm was used to properly treat data outliers, the mapping phase orbit data was weighted based on an a priori analysis of the data, and static external fields were treated by a joint inversion of external and internal fields. Further, temporal variabilities in the data which lead to unrealistically strong anomalies were considered as noise and handled by additionally minimizing a measure of the horizontal gradient of the vertically down internal field component at surface altitude. Here we use an iteratively reweighted least squares algorithm to approach an absolute measure (L1 norm), allowing for a better representation of strong localized magnetic anomalies as compared to the conventional least squares measure (L2 norm). The resulting model reproduces all known characteristics of the Martian lithospheric field and shows a rich level of detail. It is characterized by a low level of noise and robust when downward continued to the surface. We show how these properties can help to improve the knowledge of the Martian past and present magnetic field by investigating magnetic signatures associated with impacts and volcanoes. Additionally, we present some previously undescribed isolated anomalies, which can be used to determine paleopole positions and magnetization strengths.</Description>
11 11 <Contact>
12   - <PersonID></PersonID>
  12 + <PersonID>spase://CDPP/Person/A.Morschhauser</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CDPP/Person/A.Beth</PersonID>
  17 + <Role>TechnicalContact</Role>
  18 + </Contact>
15 19 </ResourceHeader>
16 20 <Model>
17 21 <ModelID>spase://CDPP/SimulationModel/AMDA/Morschhauser</ModelID>
... ... @@ -26,7 +30,10 @@
26 30 <Units></Units>
27 31 </SimulationDomain>
28 32 <InputParameter>
29   - <Name>Orbit</Name>
  33 + <Name>Orbit</Name>
  34 + <Property>
  35 + <PropertyQuantity>Ephemeris</PropertyQuantity>
  36 + </Property>
30 37 </InputParameter>
31 38 </SimulationRun>
32 39 </Spase>
... ...