MSL data in the PDS and the Analyst's Notebook, Working with the archived science & engineering data |
MSL data in the PDS and the Analyst's Notebook, Working with the archived science & engineering data |
Feb 27 2013, 07:22 PM
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Solar System Cartographer Group: Members Posts: 10229 Joined: 5-April 05 From: Canada Member No.: 227 |
"February 27, 2013. MSL Release 1, part 1, Sols 0-89.
The first release of MSL data takes place in two parts. Part 1, February 27, 2013, includes raw data products (EDRs) acquired on Sols 0 through 89, August 6 through November 5, 2012, for these instruments: APXS, ChemCam, DAN, Hazcam, Navcam, and REMS, along with SPICE data. Part 2, March 20, 2013, will include the derived data products (RDRs) for Sols 0 though 89 for the APXS, ChemCam, DAN, Hazcam, Navcam, and REMS instruments, along with both the EDRs and RDRs for the CheMin and RAD instruments, and the RDRs for the SAM instrument. Release 1 does not include data from the MAHLI, MARDI, or Mastcam instruments. These instrument teams have not yet delivered data products to PDS. Some documents in the MSL archives are awaiting clearance by JPL Document Review and/or the JPL Import/Export Control Office. They will be posted online as soon as clearance has been received, and announced on this web site." Phil -------------------- ... because the Solar System ain't gonna map itself.
Also to be found posting similar content on https://mastodon.social/@PhilStooke Maps for download (free PDF: https://upload.wikimedia.org/wikipedia/comm...Cartography.pdf NOTE: everything created by me which I post on UMSF is considered to be in the public domain (NOT CC, public domain) |
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Apr 16 2013, 03:00 PM
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Senior Member Group: Members Posts: 2346 Joined: 7-December 12 Member No.: 6780 |
The official statement regarding the noise of thermopiles B and C according to the PDS file REMS RDR Data Set Reference Information is
QUOTE Data from thermopiles B and C of the Ground Temperature Sensor are included but are too noisy to be considered useful. I'm not yet quite at that point, because the noise seems to be structured; it might be possible - besides appropriate averaging - to exploit this structure by analysing a sufficiently large set of data. Examples: 1. The double peak of the Brightness Temperature B noise distribution seems to indicate temperatures below 200K. Dividing the areas of the two peaks may lead to a temperature estimate. 2. Standard deviation and skewness of the noise distribution seem to be correlated to temperature. For all REMS RDR data: QUOTE These data are not corrected from several factors such as external heat sources or shadows, so confidence level codes shall be revised carefully before using them.
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