QLop: Issueshttps://hephaistos.lpp.polytechnique.fr/redmine/https://hephaistos.lpp.polytechnique.fr/redmine/redmine/favicon.ico?15080976012017-11-03T13:04:43ZRedmine
Redmine SciQLOP - Feature #2252 (New): Affichage d'une variable en cours d'initialisationhttps://hephaistos.lpp.polytechnique.fr/redmine/issues/22522017-11-03T13:04:43ZAnonymousSciQLOP - Feature #919 (New): allow possible connection between events in catalogshttps://hephaistos.lpp.polytechnique.fr/redmine/issues/9192017-01-27T18:29:24ZNicolas Aunainicolas.aunai@lpp.polytechnique.fr
<p>It should be possible to link events with other events. <br>
Either they are part of the same observation/conjunection of spacecraft, or hey are somehow casually linked like for example a iCME seen by ACE, could be externally linked to a SOHO distant observation of the sun where the CME is seen as an image.<br>
This is useful for space weather where some events may be seen at different distance from the sun and/or by different s/c</p>
SciQLOP - Feature #918 (New): View catalog timelineshttps://hephaistos.lpp.polytechnique.fr/redmine/issues/9182017-01-27T18:27:02ZNicolas Aunainicolas.aunai@lpp.polytechnique.fr
<p>It should be possible to see a histogram showing the number of events in different catalogs in a given time period.<br>
On the attached pic. I have selected 3 catalogs, and as a function of time I see the number of events in these catalogs.<br>
The histogram is dynamically adjusted (bin size) as I zoom in and out. <br>
I should be able, by putting my mouse over the histogram bars, to see some metadata, like number of events, spacecraft etc.</p>
<p>This should be very useful to see if other events have been catalogued as I'm browsing data on, say, Cluster... I look at the time period I'm currently plotting, and I see events have been labeled with Geotail spacecraft, and I might be interested in looking at this data.</p>
SciQLOP - Feature #895 (New): Data tree filter real time filtering https://hephaistos.lpp.polytechnique.fr/redmine/issues/8952017-01-13T12:29:33ZAlexis Jeandet
<p>For now we have to hit enter to get result, it would be better to have real time filtering </p>
SciQLOP - Feature #892 (New): Add category choice for filter on data tree https://hephaistos.lpp.polytechnique.fr/redmine/issues/8922017-01-13T12:17:18ZAlexis Jeandet
<p>The data tree filter searches on all attributes, we should be able to select on which attribute we want to filter.</p>
SciQLOP - Feature #891 (New): Add expand/collapse all on data treehttps://hephaistos.lpp.polytechnique.fr/redmine/issues/8912017-01-13T12:14:01ZAlexis Jeandet
<p>The data tree filter expands all nodes, this not cool. </p>
SciQLOP - Feature #673 (New): code must be documentedhttps://hephaistos.lpp.polytechnique.fr/redmine/issues/6732016-03-11T21:10:57ZNicolas Aunainicolas.aunai@lpp.polytechnique.fr
<p>The code is not currently documented.<br>
Functions/modules/classes etc. should be fully documented with the doxygen system.</p>
SciQLOP - Feature #664 (Closed): Add progress bar in time selection windowhttps://hephaistos.lpp.polytechnique.fr/redmine/issues/6642016-03-11T20:21:50ZNicolas Aunainicolas.aunai@lpp.polytechnique.fr
<p>User should be able to see the progress of the download.</p>
SciQLOP - Feature #654 (Resolved): Horizontal Zoomhttps://hephaistos.lpp.polytechnique.fr/redmine/issues/6542016-03-09T10:31:40ZAnonymous
<p>Zooming horizontally (along X axis only) must be implemented.<br>
As far as I know, this feature is not available directly from the QChart library, so we need to add it.</p>
SciQLOP - Feature #640 (New): Feature "Same As" for data time selectionhttps://hephaistos.lpp.polytechnique.fr/redmine/issues/6402016-03-01T16:46:07ZAnonymous
<p>This feature needs improvement in the database and in the way data are stored in order to be deployed.</p>
<p>Missing points :</p>
<ul>
<li>start and stop dates of data in the database are not stored in metadata, so we need to develop something to provide access to it.</li>
<li>in the case of data extracted from direct files, it is necessary to check deep inside metadata to access start and stop time (especially for cdf files).</li>
</ul>
Feature #474 (New): Data Downloadhttps://hephaistos.lpp.polytechnique.fr/redmine/issues/4742015-07-21T11:38:18ZLina hadidlina.hadid@lpp.polytechnique.fr
<p>Download zipped data</p>
<p>e.g.: <a href="http://ppi.pds.nasa.gov/ditdos/download?f=zip&id=pds://PPI/CO-E_SW_J_S-MAG-3-RDR-FULL-RES-V1.0/DATA/2007/182_212_JUL/07182_FGM_KRTP">http://ppi.pds.nasa.gov/ditdos/download?f=zip&id=pds://PPI/CO-E_SW_J_S-MAG-3-RDR-FULL-RES-V1.0/DATA/2007/182_212_JUL/07182_FGM_KRTP</a></p>
SciQLOP - Feature #466 (Closed): Add some extra formats to export datahttps://hephaistos.lpp.polytechnique.fr/redmine/issues/4662015-07-13T13:18:30ZAlexis Jeandet
<p>It may be a good feature to be able to export electric or magnetic fields to wav,mp3 or ogg formats. It as already been asked by users.</p>
SciQLOP - Feature #435 (Closed): Full integration of IPython.https://hephaistos.lpp.polytechnique.fr/redmine/issues/4352015-06-11T16:25:42ZAlexis Jeandet
<p>Seems possible:</p>
<p>from IPython import embed; embed()<br>
</p>
<p>But gives this output:</p>
<p>Traceback (most recent call last):<br>
File "", line 2, in <br>
File "/usr/lib/python2.7/site-packages/IPython/terminal/embed.py", line 290, in embed<br>
shell = InteractiveShellEmbed.instance(**kwargs)<br>
File "/usr/lib/python2.7/site-packages/IPython/config/configurable.py", line 354, in instance<br>
inst = cls(*args, **kwargs)<br>
File "/usr/lib/python2.7/site-packages/IPython/terminal/embed.py", line 92, in <strong>init</strong><br>
display_banner=display_banner<br>
File "/usr/lib/python2.7/site-packages/IPython/terminal/interactiveshell.py", line 328, in <strong>init</strong><br>
**kwargs<br>
File "/usr/lib/python2.7/site-packages/IPython/core/interactiveshell.py", line 483, in <strong>init</strong><br>
self.init_readline()<br>
File "/usr/lib/python2.7/site-packages/IPython/core/interactiveshell.py", line 1884, in init_readline<br>
self.refill_readline_hist()<br>
File "/usr/lib/python2.7/site-packages/IPython/core/interactiveshell.py", line 1893, in refill_readline_hist<br>
stdin_encoding = sys.stdin.encoding or "utf-8"<br>
AttributeError: 'PythonQtStdInRedirect' object has no attribute 'encoding'</p>
<p>"here":<a href="http://sourceforge.net/p/pythonqt/discussion/631393/thread/82f8056d/">http://sourceforge.net/p/pythonqt/discussion/631393/thread/82f8056d/</a> we can find some hints about how to extend PythonQtStdIn.</p>
Feature #366 (New): visualisation de spectrogrammeshttps://hephaistos.lpp.polytechnique.fr/redmine/issues/3662015-03-17T10:22:28ZNicolas Aunainicolas.aunai@lpp.polytechnique.fr
<p>Il serait bien de pouvoir regarder des spectrogrammes (de particules ou d'ondes) : <a href="http://www.igpp.ucla.edu/public/THEMIS/SCI/Pubs/Nuggets/Magnetopause%20Crossing/figure_2.jpg">http://www.igpp.ucla.edu/public/THEMIS/SCI/Pubs/Nuggets/Magnetopause%20Crossing/figure_2.jpg</a></p>
SciQLOP - Feature #352 (Closed): visualisation des distribution moyennées ou au spin sur des inte...https://hephaistos.lpp.polytechnique.fr/redmine/issues/3522015-03-05T20:08:08ZNicolas Aunainicolas.aunai@lpp.polytechnique.fr
<p>L'idée est de pouvoir visualiser les distributions de particules de façon interactive en sélectionnant des intervalles sur des séries temporelles (par ex. de B). Les distributions seraient soit données au spin sur le nombre de spin/intervalles, ou moyennées sur les intervalles sélectionnés pour augmenter la stat. On devrait pouvoir les visualiser en mode projection (Vx,Vy) (Vx,Vz), (Vy,Vz), en GSE, en GSM, dans un repère donnée par l'utilisateur, ou alors dans un plan de coupe obtenu avec un curseur sur chaque dimension. On devrait aussi pouvoir les visualiser en 3D sous forme d'isocontour avec le niveau du contour changeable avec un curseur.<br>
Sur ces distributions, on peut afficher diverses informations utiles comme : </p>
<p>la position de la vitesse moyenne<br>
la position de la vitesse de dérive ExB dans le plan représenté<br>
la direction locale du champ magnétique (ou moyennées sur l'intervalle de sélection)<br>
une ellipse de demi grand et petit axes données par la température Perp et Para.</p>
<p>Afin de pouvoir voir l'effet de moyenne, on pourrait imaginer un curseur qui ferait dynamiquement la moyenne sur les N spins présents dans l'intervalle sélectionné.</p>
<p>On peut aussi afficher des informations, comme la valeur des températures perp/para, le coefficient de nongyrotropie de la distribution etc. a voir par la suite.</p>
<p>A voir plus tard : la visualisation de distributions sub-spin.</p>