M2020 Derived Imaging Data Archive Peer Review
Dec 21, 2020 — Feb 15, 2021
Review Comments Due Jan 29, 2021
Reminder: M2020 Landing Day is February 18, 2021
For the Mars 2020 Perseverance Rover Mission (M2020), almost all of the instruments acquire imaging data for either primary or secondary/context purposes — M2020 is festooned with imagers. The data from which will be processed through the JPL Instrument Data System (IDS) pipeline to create operational image products for each of the instrument teams which, in turn, also produce their own derived data. This peer review (the RDR PR) will therefore be an all-encompassing look at the entire scope and scale of derived products generated from these operational imaging data.
This is a lot of data.
Prior to this RDR PR, a raw data peer review (the EDR PR) uncovered issues to be addressed. Therefore, this RDR PR has had changes implemented to address most of those issues. Updated versions of the raw products are included and may be re-reviewed.
As M2020 is still on approach to Mars, the test data used for this review will portray imagery acquired from testbed/laboratory environments and, as such, may be irrelevant in any scientific sense. Nevertheless, the main goal of this review is to ensure that the data ultimately submitted for archival will be meet several important objectives:
Not all review members will be expected to comment with respect to all the above objectives. The group, as a whole, will accomplish this.
Ultimately, your review of these archives will consist of a written set of comments, clarifications and discrepancies that, if implemented and/or corrected, would improve the archive. These written statements need to be provided to the Review Coordinator by the “Comments Due” date in the Schedule (below).
Though this peer review covers a lot of data, there is a methodical path through it. The first, and most important, thing to look at is probably the camera SIS, found here:
The SIS itself is huge, you are probably better off skimming it and honing in on sections of interest rather than trying to read the whole thing. Note that it has been completely reorganized and largely rewritten since the EDR PR, so if you participated in that review you should revisit the document.
Of particular note are the label tables described in Appendix B, they describe in detail all of the label items. Start with this one:
(There’s also a PDF version, but the hyperlinks likely work better in the above HTML.)
Then it’s a matter of looking for the data you’re most interested in. Pick a camera type, choose the right bundle from the list below, go to the directory starting with “data”, and drill down through the sol numbers to find the data of interest. The XML label can be viewed directly in most Web browsers. Cross-reference interesting items against the label table.
The browse directory contains viewable images. However, Marsviewer (described below) is recommended to access the bulk of the image data.
Reviewers are welcome to provide comments in any preferred format via email to the Review Coordinators. The below Google Sheet is available for use, but ultimately not required. Each reviewer has a named tab within this Sheet for their own use.
https://docs.google.com/spreadsheets/d/1zlOmca83Ft_RGmQwuPVBOrWCoo9Cej5Ie7mh2FZjwNo/edit?usp=sharing
This sheet will ultimately be used to adjudicate reviewer comments and convey the Data Provider’s response to each of these comments. So, however review comments are delivered to the Review Coordinators, they will be distilled and tracked here.
There are 5 image archive “bundles” being reviewed here (see the Bundle SIS). They are:
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/mars2020_ecam
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/mars2020_mastcamz
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/mars2020_helicam
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/mars2020_imgops
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/mars2020_meda
As described in the Bundle SIS, the first four will ultimately be archived at the Imaging Node, with mars2020_imgops data being included by reference at the Geosciences Node within the specific instrument bundles. The last is archived at the Atmospheres Node, and is a partial bundle containing only the SkyCam; it will be combined with the rest of the MEDA non-imaging data in a single, unified bundle prior to release.
There is one additional bundle that is important to this review:
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/mars2020_mission
which will be maintained at the Geosciences Node. A portion of this bundle is included with this review, containing the files that are relevant to the camera data and are a primary, critical part of this review. However, the bundle itself is not complete - feel free to point out issues but keep that in mind during the review.
The data being reviewed here is largely from Operational Readiness Test (ORT) 11, from mid-November, 2020. This was a “surface nominal” test, which exercised most of the capabilities of the rover (except mobility) and most of the instruments. It consists of sols 00113-00118. This is a lot of data, on the order of 500 GB. But as this rover generates a lot of data, especially a lot of derived data, we felt it was important to present an example of the scope and scale of data users should expect, and to exercise the generation tools. We certainly do not expect anyone to look at all of the data; pick and choose what makes sense to you and your interests.
Note that due to some last-minute fixes, terrain meshes are only included for sol 00114, even though they were in more sols for the actual ORT.
In addition to the ORT-11 data, updated EDRs from the EDR Peer Review are included for instruments or modes that were not represented in the ORT. The EDR data files are the same as for the EDR PR, but the labels have been regenerated. There are no derived products generated from these EDRs. The sols with this EDR-only data, and the reason for inclusion, are:
See the liens list for caveats regarding this non-ORT-11 data.
Finally, there are a few extra example files here: extra_examples which contains examples of files that illustrate issues in the liens list that are fixed in software but could not be applied to the entire data set. They are proper products with labels, but are not in any bundle or directory structures.
All, however, are appropriate for your review. They can respectively be found in:
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/support/LDD/
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/support/context/
Marsviewer is an interactive, Java-based tool that understands the relationships between the various data products, their organization within the archive, and how to present the data in a visual manner. Most importantly, it provides visualization for the non-image data types, such as XYZs and surface normals, that are stored in image format. To get started, simply perform the following:
Download the executable from the Peer Review site here:
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/support/marsviewer/marsviewer-install.zip
Once downloaded, double-click the .zip file to reveal the marsviewer-install.exe installation executable.
Run the installation wizard, specifying the location to which the application suite will be installed on your computer. The default installation location is %PROGFILES%\JPL\Marsviewer\. (where %PROGFILES% should be replaced with the suitable ‘Program Files’ directory of your system).
After installation, you should see a ‘Marsviewer’ icon on your Windows Desktop. Double-click the application icon to launch the tool.
Download the DMG image from the Peer Review site here:
https://pds-imaging.jpl.nasa.gov/reviews/mars2020/support/marsviewer/Marsviewer.dmg
Once downloaded, the DMG file should be expanded. If not, then double-click on the file to expand it
Select and drop the Marsviewer (for search and display) and Jadeviewer (image viewer only) apps into your Applications folder. Marsviewer is used for browsing Mars images that reside on PDS servers. Jadeviewer is used for looking at a specific image data product on your computer.
Double-click the application to launch it. If you get a security violation when doing that, try ctrl-click on the icon and then select Open. It should present you with a dialog asking if you really want to open it. Say yes. This should only be needed once; a simple double-click should be sufficient for future invocations.
When Marsviewer starts, it presents you with a dialog box from which to select a “File Finder”. There are preset values for each of the instrument groups, which should be straightforward The one confusing one is ECAM. Select “PDS M2020 ECAM - PR” for most uses. This gives you access to the reassembled FDR and RDR products. Selecting “PDS M2020 ECAM Tiles - PR” will give you access to the original tiles, but not the reassembled products.
File/New File Finder will allow you to change the file finder preset to a different type.
The server hosting this data for the PR is slow, so be patient during loading - especially with very large ECAM images.
For each of the file finders, data is available on the following sols:
ECAM | 11, 22, 71, 74, 114, 115, 116, 117, 118, 157, 2865 |
Mastcam-Z | 114, 115, 116, 117, 118, 194 |
Heli | 0 |
SHERLOC-ACI | 116 |
SHERLOC-WATSON | 115, 116, 118, 231 |
PIXL MCC | 118 |
SuperCam RMI | 116 |
MEDA SkyCam | 115 |
ECAM Tiles | 11, 22, 71, 74, 114, 115, 116, 117, 118, 157, 2865 |
The Mars2020 image processing system is still under development; not everything is finished yet. There are thus aspects of the archives submitted for this review that are incomplete, incorrect, or missing. The known issues are listed below:
Example products with these labels present are available in extra_examples. They are outside the bundle structure because the fixes were made too late to rerun all the data. Nevertheless, the examples show what the above items should look like for the rest of the data set.
An example of this behavior can be seen with img:active_flag. Its two XPaths in the table are:
/Product_Observational/Observation_Area/Discipline_Area/Imaging/Radiometric_Correction/active_flag
/Product_Observational/Observation_Area/Discipline_Area/Imaging/Flat_Field_Correction/active_flag
Note that the active_flag key has two different parents: Radiometric_Correction and Flag_Field_Correction. The corresponding VICAR keys are:
Radiometric_Correction.img.active_flag -> DERIVED_IMAGE_PARMS.RADIOMETRIC_CORRECTION_TYPE
Flat_Field_Correction.img.active_flag -> OBSERVATION_REQUEST_PARMS.FLAT_FIELD_CORRECTION_FLAG
Yet the VICAR keys displayed are:
Shutter_Subtraction.img.shutter_subtraction_mode -> INSTRUMENT_STATE_PARMS.SHUTTER_CORRECTION_MODE
Shutter_Subtraction.img.active_flag -> OBSERVATION_REQUEST_PARMS.SHUTTER_CORRECTION_MODE
This bug will be fixed in the next release of the table generation software.
Some additional liens which apply ONLY to the non-ORT-11 data (outside sols 113-118):
Date Range | Moniker | Duration | Event |
Dec 21 — Jan 3 | Team Assembles/ Holidays | 2 weeks | Allow participants to introduce themselves to the archives. |
Jan 4 — Jan 29 | Review | 4 weeks | Reviewers to review and make comments about the archives |
Feb 1 | Comments Due | 1 day | All comments should be delivered to Review Coordinators (M. Le/ M. McAuley) |
Feb 2 — Feb 3 | Comments Published to Provider | 2 days | Compiled comments to be sent to data provider and posted by Coordinator |
Feb 4 — Feb 12 | Provider Response | 1+ week | Provider responses to compiled comments due to Coordinator |
Feb 13 — Feb 18 | Response Published | 1 week | Reviewers acceptance/comment of Provider’s response |
Name | Affiliation |
Richard Chen | PDS, Engineering Node |
Kimberly Murray | Arizona State University |
Kevin Lewis | Johns Hopkins University |
Timothy J. Parker | JPL, Planetary Geosciences |
Jon Proton | OpsCode, LLC (Mastcam-Z) |
Susan Slavney | PDS, Geosciences Node |
Tom Stein | PDS, Analyst’s Notebook |