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Fig.
14.3
) that are now being executed in HELIOGate are the processing of fre-
quency data produced by the LOFAR new generation radio interferometric array
and the processing of images from the Crisp Imaging Spectro-Polarimeter (CRISP),
located at the Swedish Solar Telescope (SST).
Unfortunately, the very large variety of data processing applications makes it
very dif
cult to cover them all under prede
ned workflows and portlets. To tackle
this dif
culty, HELIOGate tries to offer easy-to-con
gure tools at three main levels
as described in Fig.
14.3
:
Generic workflows for data processing that can be adapted in an ef
cient and
reusable way, and,
A generic data processing code framework written in Java to minimize the effort
required to develop data processing code.
User views to execute workflows that hide from the users all the parameters that
are not strictly necessary.
Fig. 14.3 Data processing in HELIOGate
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