The Challenge of Data Reduction for Multiple Instruments on   Stratospheric Observatory For Infrared Astronomy (SOFIA)
  SOFIA presents a number of interesting challenges for the development of a data reduction environment which, at its initial phase, will have to incorporate pipelines from seven different instruments. Therefore, the SOFIA data reduction software must run code which has been developed in a variety of dissimilar environments which will only increase in future generations of instrumentation. We investigated three distinctly different situations for performing pipelined data reduction in SOFIA: automated data reduction after data archival at the end of a mission, re-pipelining of science data with updated calibrations or optimum parameters, and the interactive user-driven local execution and analysis of data reduction by an investigator. These different modes would traditionally result in very different software implementations of algorithms used by each instrument team, in effect tripling the amount of data reduction software that would need to be maintained by SOFIA. We present here a unique approach for enfolding all the instrument-specific data reduction software in the observatory framework and verifies the needs for all three reduction scenarios as well as the standard visualization tools. The SOFIA data reduction structure would host the different algorithms and techniques that the instrument teams develop in their own environment. Ideally, duplication of software is minimized across the system because instrument teams can draw on software solutions and techniques previously delivered to SOFIA by other instruments. With this approach, we minimize the effort for analyzing and developing new software reduction pipelines for future generation instruments. We also explore the potential benefits of this approach in the portability of the software to an ever-broadening science audience, as well as its ability to ease the use of distributed processing for data reduction pipelines. 
M. V. Charcos-Llorens, R. Krzaczek, R. Y. Shuping and L. Lin
astro-ph.IM