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STEREO-B SECCHI HI Level 2 produced by UK Solar System Data Centre

ResourceID
spase://NASA/NumericalData/STEREO-B/SECCHI/HI/L2_RAL

Description

SECCHI HI Level 2 FITS files produced by the UK Solar System Data Centre, calibrated and background subtracted. Images stored in FITS files with filenames such as "20140101_180501_24h1A_br11.fts". The meaning of the different parts of this filename is as follows:

  • 20140101 is the observation date, 2014-01-01;
  • 180501 is the observation time, 18:05:01 UT;
  • 2 represents Level-2;
  • 4 is a code for the data units, where 4=Dn/Sec/Pixel, b=Mean Solar Brightness (MSB), and t=S10. MSB & S10 have the diffuse source correction applied;
  • h1 or h2 for HI-1 or HI-2;
  • A or B for STEREO-A or STEREO-B;
  • br for Buffinton/RAL background subtracted--a full running window where the F-corona is computed as the mean of the lowest quartile of pixels;
  • 11 is the length of the running window in days, usually either 01 or 11 for HI-1, and 03 or 11 for HI-2.

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Details

Version:2.3.1

NumericalData

ResourceID
spase://NASA/NumericalData/STEREO-B/SECCHI/HI/L2_RAL
ResourceHeader
ResourceName
STEREO-B SECCHI HI Level 2 produced by UK Solar System Data Centre
ReleaseDate
2020-07-07 21:15:23Z
Description

SECCHI HI Level 2 FITS files produced by the UK Solar System Data Centre, calibrated and background subtracted. Images stored in FITS files with filenames such as "20140101_180501_24h1A_br11.fts". The meaning of the different parts of this filename is as follows:

  • 20140101 is the observation date, 2014-01-01;
  • 180501 is the observation time, 18:05:01 UT;
  • 2 represents Level-2;
  • 4 is a code for the data units, where 4=Dn/Sec/Pixel, b=Mean Solar Brightness (MSB), and t=S10. MSB & S10 have the diffuse source correction applied;
  • h1 or h2 for HI-1 or HI-2;
  • A or B for STEREO-A or STEREO-B;
  • br for Buffinton/RAL background subtracted--a full running window where the F-corona is computed as the mean of the lowest quartile of pixels;
  • 11 is the length of the running window in days, usually either 01 or 11 for HI-1, and 03 or 11 for HI-2.
Contacts
RolePersonStartDateStopDateNote
1.GeneralContactspase://SMWG/Person/William.T.Thompson
InformationURL
Name
UKSSDC - STEREO HI data processing documentation
URL
PriorIDs
spase://VSPO/NumericalData/STEREO-B/SECCHI/HI/L2_RAL
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
UKSSDC - STEREO Archive data access
URL
Format
Text
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Format
Text
InstrumentIDs
MeasurementType
ImageIntensity
TemporalDescription
TimeSpan
StartDate
2006-10-01 00:00:00Z
RelativeStopDate
-P15D