HR: 1330h
AN: C32A-0428    [PDF]
TI: ICESat Science Investigator led Processing System (I-SIPS)
AU: * Bhardwaj, S
EM: suneel.bhardwaj@gsfc.nasa.gov
AF: Raytheon ITSS, NASA/Goddard Space Flight Center, Mail Stop 971, Greenbelt, MD 20771 United States
AU: Bay, J
EM: John.G.Bay.1@gsfc.nasa.gov
AF: Raytheon ITSS, NASA/Goddard Space Flight Center, Mail Stop 971, Greenbelt, MD 20771 United States
AU: Brenner, A
EM: Anita.C.Brenner.1@gsfc.nasa.gov
AF: Raytheon ITSS, NASA/Goddard Space Flight Center, Mail Stop 971, Greenbelt, MD 20771 United States
AU: DiMarzio, J
EM: John.P.Dimarzio.1@gsfc.nasa.gov
AF: Raytheon ITSS, NASA/Goddard Space Flight Center, Mail Stop 971, Greenbelt, MD 20771 United States
AU: Hancock, D
EM: David.W.Hancock@nasa.gov
AF: NASA Goddard Space Flight Center, NASA/Goddard Space Flight Center, Mail Stop 971, Greenbelt, MD 20771 United States
AU: Sherman, M
EM: Robert.M.Sherman.1@gsfc.nasa.gov
AF: Raytheon ITSS, NASA/Goddard Space Flight Center, Mail Stop 971, Greenbelt, MD 20771 United States
AB: The ICESat Science Investigator-led Processing System (I-SIPS) generates the GLAS standard data products. It consists of two main parts the Scheduling and Data Management System (SDMS) and the Geoscience Laser Altimeter System (GLAS) Science Algorithm Software. The system has been operational since the successful launch of ICESat. It ingests data from the GLAS instrument, generates GLAS data products, and distributes them to the GLAS Science Computing Facility (SCF), the Instrument Support Facility (ISF) and the National Snow and Ice Data Center (NSIDC) ECS DAAC. The SDMS is the Planning, Scheduling and Data Management System that runs the GLAS Science Algorithm Software (GSAS). GSAS is based on the Algorithm Theoretical Basis Documents provided by the Science Team and is developed independently of SDMS. The SDMS provides the processing environment to plan jobs based on existing data, control job flow, data distribution, and archiving. The SDMS design is based on a mission-independent architecture that imposes few constraints on the science code thereby facilitating I-SIPS integration. I-SIPS currently works in an autonomous manner to ingest GLAS instrument data, distribute this data to the ISF, run the science processing algorithms to produce the GLAS standard products, reprocess data when new versions of science algorithms are released, and distributes the products to the SCF, ISF, and NSIDC. I-SIPS has a proven performance record, delivering the data to the SCF within hours after the initial instrument activation. The I-SIPS design philosophy gives this system a high potential for reuse in other science missions.
DE: 1827 Glaciology (1863)
SC: Cryosphere [C]
MN: 2003 Fall Meeting