-
Notifications
You must be signed in to change notification settings - Fork 5
Commit
This commit does not belong to any branch on this repository, and may belong to a fork outside of the repository.
- Loading branch information
1 parent
535fba7
commit d9b3e9b
Showing
1 changed file
with
30 additions
and
29 deletions.
There are no files selected for viewing
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -1,31 +1,32 @@ | ||
| <?xml version="1.0" encoding="UTF-8"?> | ||
| <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"> | ||
| <Version>2.2.0</Version> | ||
| <Instrument> | ||
| <ResourceID>spase://SMWG/Instrument/SDO/AIA</ResourceID> | ||
| <ResourceHeader> | ||
| <ResourceName>AIA</ResourceName> | ||
| <ReleaseDate>2010-10-04T20:54:57Z</ReleaseDate> | ||
| <Description>The SDO (Solar Dynamics Observatory) AIA | ||
| (Atmospheric Imaging Assembly) is a battery of four telescopes | ||
| designed to image the dynamic solar atmosphere in multiple | ||
| different wavelengths to link changes in the surface to those | ||
| in the interior. Data will include images of the Sun that span | ||
| at least 1.3 solar diameters in 10 wavelengths (7 EUV and | ||
| 3 UV-visible channels) nearly simultaneously, at a resolution | ||
| of about 1 arcsec and at a cadence of 10 seconds or better | ||
| </Description> | ||
| <Contact> | ||
| <PersonID>spase://SMWG/Person/Alan.M.Title</PersonID> | ||
| <Role>PrincipalInvestigator</Role> | ||
| </Contact> | ||
| <InformationURL> | ||
| <Name>AIA web site at Lockheed</Name> | ||
| <URL>http://aia.lmsal.com/</URL> | ||
| </InformationURL> | ||
| </ResourceHeader> | ||
| <InstrumentType>Imager</InstrumentType> | ||
| <InvestigationName>AIA</InvestigationName> | ||
| <ObservatoryID>spase://SMWG/Observatory/SDO</ObservatoryID> | ||
| </Instrument> | ||
| <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> | ||
| <Instrument> | ||
| <ResourceID>spase://SMWG/Instrument/SDO/AIA</ResourceID> | ||
| <ResourceHeader> | ||
| <ResourceName>Atmospheric Imaging Assembly (AIA)</ResourceName> | ||
| <ReleaseDate>2010-10-04T20:54:57Z</ReleaseDate> | ||
| <Description>The SDO (Solar Dynamics Observatory) AIA (Atmospheric Imaging Assembly) is a battery of four telescopes | ||
| designed to image the dynamic solar atmosphere in multiple different wavelengths to link changes in the surface to those in the interior. Data will include images of the Sun that span at least 1.3 solar diameters in 10 wavelengths (7 EUV and 3 UV-visible channels) nearly simultaneously, at a resolution of about 1 arcsec and at a cadence of 10 seconds or better.</Description> | ||
| <Contact> | ||
| <PersonID>spase://SMWG/Person/Alan.M.Title</PersonID> | ||
| <Role>FormerPI</Role> | ||
| </Contact> | ||
| <Contact> | ||
| <PersonID>spase://SMWG/Person/Mark.C.M.Cheung</PersonID> | ||
| <Role>PrincipalInvestigator</Role> | ||
| </Contact> | ||
| <InformationURL> | ||
| <Name>AIA web site at Lockheed</Name> | ||
| <URL>http://aia.lmsal.com/</URL> | ||
| </InformationURL> | ||
| <InformationURL> | ||
| <Name>The SDO/AIA Instrument paper</Name> | ||
| <URL>https://doi.org/10.1007/s11207-011-9776-8</URL> | ||
| </InformationURL> | ||
| </ResourceHeader> | ||
| <InstrumentType>Imager</InstrumentType> | ||
| <InvestigationName>AIA</InvestigationName> | ||
| <ObservatoryID>spase://SMWG/Observatory/SDO</ObservatoryID> | ||
| </Instrument> | ||
| </Spase> |