solarflows dr. gabriele pierantoni (tcd)
DESCRIPTION
SolarFlows Dr. Gabriele Pierantoni (TCD). Contents. What is Heliophysics ? How could workflows help ? Some examples What we are doing. Solar and Helio physics. - PowerPoint PPT PresentationTRANSCRIPT
![Page 1: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/1.jpg)
SolarFlowsDr. Gabriele Pierantoni (TCD)
![Page 2: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/2.jpg)
Contents
• What is Heliophysics ? • How could workflows help ?• Some examples• What we are doing...
![Page 3: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/3.jpg)
Solar and Helio physics• Solar physics: the study of the Sun. It is
a branch of astrophysics that specializes in exploiting and explaining the detailed measurements that are possible only for our closest star.
• Heliophysics: the study of the system composed of the Sun’s heliosphere and the objects that interact with it.
![Page 4: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/4.jpg)
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
![Page 5: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/5.jpg)
Heliophysics• Automated searches are difficult when major events can be
“missed” and searches for long duration events would yield spurious results
![Page 6: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/6.jpg)
Requirements (1 of 4)
Location is important
Effects depend on type of emission
Propagation is influenced by the interplanetary magnetic field for particles
Propagation models are fundamental !
![Page 7: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/7.jpg)
Requirements (2 of 4)
Data and Metadata interactions
From Data to Metadata : extraction of features and events from raw data. This is a potentially computationally intensive process.
From Metadata to Data : find raw data using metadata (catalogues and lists).
![Page 8: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/8.jpg)
Requirements (3 of 4)
Research Community
Research is currently developed by many different communities who need reliable data models and metadata to be able to work together.
![Page 9: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/9.jpg)
Requirements (4 or 4)
• Use of standard web service protocols• Support of looping• Execution of workflows in both a client and a
server environment• Available support and documentation• Platform independence• Support of multiple instances of a service and
automatic fail-over
![Page 10: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/10.jpg)
Heliophysics, the old way.
![Page 11: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/11.jpg)
Heliophysics, the NEW way.
HELIO Service
HELIO Service
HELIO Service
AccessLayer
HELIOAPI
![Page 12: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/12.jpg)
Heliophysics, the NEW way.
![Page 13: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/13.jpg)
HELIO
http://www.helio-vo.eu/services/service_interfaces.php
![Page 14: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/14.jpg)
HELIO
http://helio.i4ds.technik.fhnw.ch/Helio-dev/prototype/explorer
![Page 15: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/15.jpg)
USER Workflows
![Page 16: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/16.jpg)
ADMIN Workflows
Enabling Services
Resources
Resources
![Page 17: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/17.jpg)
Different Workflows in Heliophysics(So far....)
• Integration tests at development time in order to assert consistency between different services.
• Virtual services which provide basic building blocks to be reused in other services.
• The actual science by combining services, user-defined operations and virtual workows into larger workflows.
![Page 18: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/18.jpg)
Test data and services
Tests the integrity of instruments IDs between two HELIO services (ICS and DPAS). It does not require any inputs since it is checking the complete content of the ICS against the the instrument registered in the DPAS.
![Page 19: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/19.jpg)
Virtual Service
This workflow is an example ofa virtual service that combines several service calls. The calls are used to properly handle asynchronous service calls.
![Page 20: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/20.jpg)
Real Science1. Find which SEP events have been
observed at Earth during the time of interest.
2. Propagate the events found backwards to retrieve the time and position in which the particles were accelerated towards Earth.
3. Flare catalogues at the HEC are queried using the times previously calculated
4. Coronal mass ejections and radio shocks are events observed above the solar atmosphere; thus two new queries to the HEC are made using the new time ranges obtained in the previous step.
5. Finally, a summary table is created which links each SEP event to the associated are, CME and radio shock.
![Page 21: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/21.jpg)
Propagation Model 1st prototype
![Page 22: SolarFlows Dr. Gabriele Pierantoni (TCD)](https://reader036.vdocuments.mx/reader036/viewer/2022081802/5681658e550346895dd85b90/html5/thumbnails/22.jpg)
What we’re doing, What we will do
• Customisable Propagation Model
• Validation of Propagation Model through HELIO (and other) services.
• Show and discuss it to the Heliophysics community at the CDAW event in September 2012
• Workflow Interoperability.