Created: 2014-08-11 15:17:18

The workflow concept is below. Current workflow is proof of concept and works for default event.

1. The initial query is to the stereo_hi_sw_transient list in a particular time range. From this catalogue we extract the longitude of the source of the transient, the longitude error, the start time (launch time of the transient) and the estimated time of arrival. The time of the event is then passed to the HELIO Instrument Location Service (ILS) to extract the Heliocentric Earth Equatorial longitudes of all available instruments.

2. If the longitude of the spacecraft matches the launch longitude of the solar wind transient, the spacecraft is checked for the possible in-situ detection of a CME or CIR (all available in-situ catalogues above are checked).

3. If a CME or CIR is detected in-situ, both the in-situ data and the imaging data are saved for manual analysis. The procedure is repeated for all detections in the stereo_hi_sw_transient list.

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