Navigation and Ancillary Information Facility NIF NAIF Node Report Addresses both NAIF Node and SPICE Development PDSMC March 27, 2012 SPICE components.

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Navigation and Ancillary Information Facility NIF NAIF Node Report Addresses both NAIF Node and SPICE Development PDSMC March 27, 2012 SPICE components are not restricted under ITAR

Navigation and Ancillary Information Facility NIF NAIF Funding Sources for FY12 2 The PDS funds: SPICE Development NAIF Node * Advanced Multi-Mission Operations System Percent of Total Available Funds  Flight Projects 42%  NAIF Node 25%  SPICE development 22%  AMMOS* 11%

Navigation and Ancillary Information Facility NIF NAIF Flight Project Funding 3

Navigation and Ancillary Information Facility NIF Archive Status Mars Odyssey Cassini MER Rovers MRO MESSENGER New Horizons Mars Express (ESA) Venus Express (ESA) Rosetta (ESA) LRO EPOXI DAWN MSL Juno GRAIL Phobos-Grunt (RSA) MAVEN OSIRIS-REx Magellan Galileo Phoenix LCROSS LADEE Good shape NAIF can finish this partial, pre-PDS archive; just need to find a bit more time. NAIF can/will finish Galileo at some point. NAIF can make a Phoenix archive. AMES did not complete itsLADEE deliveries; NAIF can patch together enough to complete the job. LADEE says it will deliver a SPICE archive at the end of the mission.

Navigation and Ancillary Information Facility NIF Archive Status – 2 Archive sizes and covered time spans 5

Navigation and Ancillary Information Facility NIF NAIF Node Summary - 1 SPICE data archiving is in pretty good shape –Usually encounter problems with archives not produced at JPL –Occasionally we find a problem of our own –NAIF will shortly transfer the NEAR SPICE archive from SBN Plan to do a major transformation of all archived SPICE data to PDS4 standards when PDS4 is stable and ready for ingest –Will correct a few current issues at the same time User consulting continues to be a big part of NAIF staff daily work 6

Navigation and Ancillary Information Facility NIF NAIF Node Summary - 2 Updates to the SPICE Tutorials were recently completed SPICE Training –The next SPICE training class will be in April, near Madrid »Around 81 students applied; ESA accepted only 42 due to space limitations –The next domestic class will probably be scheduled for later this year –Still need to break the curriculum into at least two chunks: »beginner »advanced 7

Navigation and Ancillary Information Facility NIF SPICE Development Summary - 1 Major recent focus is producing the N65 SPICE Toolkit –Due out in April –Contents: »New “geometry finder” functions »New high-level observation geometry routines »Important augmentations to some utility programs »New SPK and CK data types (one of each) to handle eventual problems with some large archive collections »Additional Icy (IDL) and Mice (MATLAB) routines »Lots of smaller items »Some bug fixes After ~three months hiatus WebGeocalc development has been re-initiated 8

Navigation and Ancillary Information Facility NIF SPICE Development Summary - 2 Other SPICE development work (on hold in recent months) –Java Native Interface (JNI) Toolkit »Alpha-test version is already being used by several groups –New shape models »Digital terrain model »Tessellated plate model Already in use on Hayabusa, DAWN, Rosetta, MEX and PhSRM 9 Phobos Itokawa Vesta

Navigation and Ancillary Information Facility NIF SPICE Development Summary - 3 The Planetary Ephemeris Working Group of IAU Commission IV has proposed to adopt (and adapt) SPICE as its standard, especially to facilitate comparisons of the planet ephemerides produced by NASA (JPL), France (Observatoire de Paris) and Russian (Institute of Applied Astronomy). Details to accommodate this are still being worked out, but it now appears this can be done. –Expect a full “Go or no go” vote quite soon There is already some talk of eventually including satellite, comet and asteroid ephemerides. 10

Navigation and Ancillary Information Facility NIF AMMOS* Summary AMMOS funds two NAIF activities: –“Sustaining” »Funds used to port the Toolkit to new environments, and to accommodate infrastructure changes –“Repair” »Funds used to zap bugs –Much of these funds go unused 11 *Advanced Multi-Mission Operations System

Navigation and Ancillary Information Facility NIF Flight Projects Summary - 1 Ongoing SPICE operations for NASA flight projects are generally going well –Odyssey, MER, MRO, Epoxi, Cassini, Dawn, LRO, Messenger, New Horizons, Juno, MSL, GRAIL Upcoming NASA missions set to use SPICE are: –MAVEN, SMAP (earth science) and OSIRIS-REx LADEE will not use SPICE in ops, but claim they will produce/deliver a SPICE archive Archive production by missions is generally going well 12 NASA Flight Projects (not funded by PDS)

Navigation and Ancillary Information Facility NIF Flight Projects Summary - 2 ESA –MEX, VEX, Rosetta SPICE archives are trickling in –BepiColombo and Solar Orbiter seem very likely to use SPICE –ExoMars and others are TBD ISRO –Said they want more SPICE training, but no recent dialogue RSA –Cooperation on Phobos Sample Return was good –Support for Luna-Resurs (for both RSA and ISRO) will be proposed to NASA, if a SALMON or similar opportunity opens up JAXA –Unclear as to future SPICE use, but some use seems likely given past experience “China” 13 International Flight Projects (A mixed bag of funding)

Navigation and Ancillary Information Facility NIF Question for PDSMC Should PDS (and IPDA) strive to have “all” instrument teams create at least a minimal, quasi- standard set of consistent observation geometry parameters*, to be placed in product labels and extracted into registries? –To be used in PDS4 data searches –To support data analysis when user’s don’t want/need to re- compute observation geometry parameters –Might be accomplished using something like the “geolib”* approach used on MEX and VEX –One big challenge: some parameters have different meaning, or are simply not applicable, depending on the type of instrument or type of mission 14 *geolib computes: orbit number, solar distance, sub-solar point, s/c-sun distance, s/c- target distance, optic axis surface intercept point, slant distance, phase/incidence/ emission angles, local true solar time, pixel scale (size) on surface.