uring the daylight portion of each orbit, the pointing platform will
point the instrument toward the Sun's center, at which time SOLSTICE will
perform full-wavelength scans. During the night portion of most orbits,
it will be reconfigured to use the stellar entrance and exit slits, and
the platform will be pointed to
one of the selected calibration bright blue
stars. The instrument will be in a fixed-wavelength mode and accumulate
stellar data for approximately 15 minutes.
The process of creating a week's worth of SOLSTICE plans consists of three parts:
Ingesting is the extraction of selected data from the information files
(planning aids) to be inserted into our database. These planning aids are
received from Goddard Space Flight Center (GSFC) and contain information
about the relative motion and position of SOLSTICE and the corresponding
stars available for viewing.
Planning uses the ingested data from GSFC in conjunction with our own planning procedures and scheduling software to create an observation plan for the week. Our automatic scheduler, OASIS_PS (Operations and Science Instrument Support_Planning and Scheduling), decides what to plan and when, but it is the responsibility of the planner to determine the quality and accuracy of the plans, as well as to make "special science" additions.
Creating the data products involves converting the plans into two required formats-text format for the scientists and binary code for the UARS microprocessor. At the end of the day, the data products are electronically sent to GSFC.
he Operations and Science Instrument Support - Planning and Scheduling (OASIS-PS) is a software tool designed for resource-oriented planning and scheduling applications. The OASIS-PS system is written in Ada and has four major software subsystem components.
The OASIS-PS software is designed to support a wide range of planning
and scheduling applications and can easily be tailored via database modifications,
DECwindows updates, and new rule base creation.
Application-specific displays may be added to the user interface in order
to allow complex representation or simulation of planning and/or scheduling
information. This may require code generation by users for their application,
but these displays allow the user greater flexibility and understanding
of very complex planning and scheduling information.
Goals Of OASIS-PS :
side from giving scientists valuable information on the present interaction
of the Sun's radiation with the Earth's atmosphere, future experimentation
will also reveal changes and trends such as the degrading "radiation-filtering"
ability of the atmosphere due to ozone depletion.
SOLSTICE was designed to be a highly variable experiment. The types of experiments performed on the Sun and stars have to be modified due to the changing needs of the scientists and the imperfect science of orbital mechanics. This requires a planning team to coordinate the plans of project managers and scientists within the boundaries of solar and stellar availabilities.
Since OASIS-PS is database driven, experimenters may enter application specific data into generic database tables at any time during the mission. This flexibility allows for new and/or modified experiments to be planned by the automatic planning software (OASIS-PS) by simple updates to the appropriate database tables.