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Welcome to the project website!
From 1969 to 1995, Big Bear Solar Observatory (BBSO)
staff recorded all of their observations on 35 mm film
before switching to digital imaging after 1995. These film data include
full-disk observations from BBSO's 8 inch
telescope and high-resolution observations from the 10 and 26 inch
telescopes, with the cadence of observations
ranging from 10 seconds to 1 minute. BBSO has an excellent clear sky
fraction. These film data sets cover two and
one-half solar cycles, include thousands of flares, and span the entire operational service of several space missions, including SMM, CGRO, and Yohkoh.
Wide public access to these BBSO data films is impractical and their
scientific capability has never been fully explored.
This project aims to digitize these films using specialized commercial
digitizing equipment and archive them in the public domain. The BBSO
data to be digitized includes full-disk and high-resolution H-alpha
images, as well as He I images. The entire set of full-disk data will be
converted to create a synoptic data base. High resolution film data will
be digitized according to events selected by the full-disk data. All
observed solar flares and filament eruptions will be automatically
detected and cataloged using artificial intelligence methods that have
been developed and implemented at the
Space Weather Research
Laboratory of the New
Jersey Institute of Technology.
Despite some limitations of the film data
format, the long-term coverage and high quality of the BBSO data will
have very broad applications for many statistical studies. For example,
the study of a large number of archived events will improve the
forecasting of future solar eruptive events, and thus
assist operational space weather prediction.
Targeted research on the filaments and flares will be carried out with
the digitized data.
We are happy to hear from you. Please address questions/concerns to
Haimin Wang.
Staffs actively working on the project include
Chang Liu,
Rui Liu,
together with three undergraduate students.

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