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Workflows, Web services, DCIs and GUIs - What is behind the HELIOGate Portal. Dr. Gabriele Pierantoni Dr. David Perez Suarez. What is HELIOGate for ?. Study the interactions between the Sun and t he other bodies of the Solar System. What is behind HELIOGate ?. Workflows APIs
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Workflows, Web services, DCIs and GUIs - What is behind the HELIOGate Portal Dr. Gabriele Pierantoni Dr. David Perez Suarez
What is HELIOGate for ? Study the interactions between the Sun and the other bodies of the Solar System.
What is behind HELIOGate ? Workflows APIs Web Services Applications
HELIOGate The HELIO Gate portal offers to the Heliophysics community an easy and intuitive way of performing repetitive and time-consuming actions.
Heliophysics • In heliophysics, we are interested in how an event on or near the solar surface can propagate through the heliosphere and affect a planetary environment • Searches should identify interesting time intervals based on a combination of event, features, etc. metadata • There are concerns about the quality and integrity of the metadata and whether it is adequate to support the searches we would like to undertake
Heliophysics, nowadays WEB Services API Code Resources Workflows Data GUI Catalogues
Heliophysics, workflows HELIOGate WS-Pgrade WEB Services Resources Taverna Data HELIOGate SHIWA Catalogues
Heliophysicists, workflows Repository Portal
Propagation Model A propagation model is used to help determine which observations, where and when may be of interest in order to satisfy the user's search criteria.
Advanced Propagation Model Origin Target t t P = Pmax ETA Range E P = POK Period of interest E P = Pmin E
Advanced Propagation Model – Release 1 Portlet WEB Services Catalogues GUSE WF Resources WEB Services Catalogues
Advanced Propagation Model – Release 2 Portlet GUSE WF Catalogues WF Resources WF Catalogues
Fastest CMEs Propagation This workflow is used to investigate one of the most relevant events in HELIOphysics; Coronal Mass Ejections. The propagation of these events is studied throughout the Solar System by the means of the execution of the SHEBA propagation model on the HELIO Processing Service.
Interfaces Time Ranges, Catalogues Events Parameters Time Ranges Time Ranges, Position Catalogues Ranks
LO-FAR Data Processing WS-PGRADE Resources