This figure shows the definitions used for the set-up of the Web Services that return unique identifiers of cell lines in CABRI catalogues after a search either by name or by property (free text search)

<p><b>Copyright information:</b></p><p>Taken from "Web services and workflow management for biological resources"</p><p></p><p>BMC Bioinformatics 2005;6(Suppl 4):S24-S24.</p><p>Published online 1 Dec 2005</p><p>PMCID:PMC1866383.</p><p></p> These definitions are written in the ACD language and must be converted into XML before they can be used. Differences between the two definitions consist in the comment line where the actual parameters for the remote call to the CABRI site are define

This diagram lists one of the workflows that have been created and are available on-line for demonstration purposes

<p><b>Copyright information:</b></p><p>Taken from "Web services and workflow management for biological resources"</p><p></p><p>BMC Bioinformatics 2005;6(Suppl 4):S24-S24.</p><p>Published online 1 Dec 2005</p><p>PMCID:PMC1866383.</p><p></p> Two web services are used (getBacteriaIdsByname and getBacteriaById), together with some local string elaborations. This output has been generated by the Taverna Workbench

The general architecture of the system includes three blocks: workflows creation and annotation (WCA), user interface (UI) and workflows execution (WE)

<p><b>Copyright information:</b></p><p>Taken from "Web services and workflow management for biological resources"</p><p></p><p>BMC Bioinformatics 2005;6(Suppl 4):S24-S24.</p><p>Published online 1 Dec 2005</p><p>PMCID:PMC1866383.</p><p></p> The "Taverna" and "FreeFluo" boxes refer to open source software developed externally from the project. The boxes named "Repository Manager", "Workflow Executor" and "Interface" refer to purpose applications developed within the project. All other boxes refer to databases, either local or remote

Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe-Metis/Solar Orbiter Observations

The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in combination with the remote-sensing observation of the coronal source region provided by the METIS coronagraph aboard Solar Orbiter. The coronal outflows observed near the ecliptic by Metis on 2021 January 17 at 16:30 UT, between 3.5 and 6.3 R ⊙ above the eastern solar limb, can be associated with the streams sampled by PSP at 0.11 and 0.26 au from the Sun, in two time intervals almost 5 days apart. The two plasma flows come from two distinct source regions, characterized by different magnetic field polarity and intensity at the coronal base. It follows that both the global and local properties of the two streams are different. Specifically, the solar wind emanating from the stronger magnetic field region has a lower bulk flux density, as expected, and is in a state of well-developed Alfvénic turbulence, with low intermittency. This is interpreted in terms of slab turbulence in the context of nearly incompressible magnetohydrodynamics. Conversely, the highly intermittent and poorly developed turbulent behavior of the solar wind from the weaker magnetic field region is presumably due to large magnetic deflections most likely attributed to the presence of switchbacks of interchange reconnection origin.</p