Commands
10
Queries
19.35 ms
Query time
0
Failed Queries
| # | Time | Connection | Command |
|---|---|---|---|
| 1 | 0.72 ms | cache | CONNECT redis.internal 6379 5 <null> 5 5 |
| 2 | 0.36 ms | cache | SELECT 0 |
| 3 | 0.28 ms | cache | MGET wJo3GJ9dRH:data > anonymous-media > id=2738,locale=fr,domain=junior |
| 4 | 15.21 ms | cache | INFO Memory |
| 5 | 0.03 ms | cache | MULTI 2 |
| 6 | 0.12 ms | cache | SETEX wJo3GJ9dRH:data > anonymous-media > id=2738,locale=fr,domain=junior 2678399 �t�A 3_ Oa:2:{i:0;s:13:"cache-service";i:1;s:36:"cache-service-data > anonymous-media";}a:15:{s:2:"id";i:398;s:5:"title";s:12:"Jour et nuit";s:4:"slug";s:12:"jour-et-nuit";s:9:"mediaType";s:10:"simulation";s:14:"thumbnailSizes";a:3:{s:9:"node_pack";s:160:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_node_pack/uploads/media/thumbnails/398-6545f34b104cd302421004.webp";s:10:"suggestion";s:161:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_suggestion/uploads/media/thumbnails/398-6545f34b104cd302421004.webp";s:5:"title";s:156:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_title/uploads/media/thumbnails/398-6545f34b104cd302421004.webp";}s:19:"thumbnailBackground";s:7:"#f6adcc";s:11:"publishedAt";O:17:"DateTimeImmutable":3:{s:4:"date";s:26:"2015-05-11 00:00:00.000000";s:13:"timezone_type";i:3;s:8:"timezone";s:3:"UTC";}s:8:"isExpert";b:0;s:5:"goals";s:61:"<ul> <li>Comprendre l'alternance jour/nuit.</li> </ul>";s:5:"width";i:550;s:6:"height";i:440;s:11:"description";s:534:"<p>L'alternance jour/nuit provient de la rotation terrestre face au Soleil. Une montre est à votre disposition pour afficher l'heure solaire. Midi est l'heure de la journée à laquelle l'ombre de tout objet est minimale.</p> <p>La configuration représentée est celle du solstice d'été. L'inclinaison de la Terre provoque à cette date une forte inégalité de la durée du jour entre les villes d'un même méridien.</p>";s:11:"suggestions";a:6:{i:0;a:9:{s:2:"id";i:426;s:5:"title";s:29:"Les 3 types d'ondes sismiques";s:4:"slug";s:29:"les-3-types-d-ondes-sismiques";s:9:"mediaType";s:10:"simulation";s:14:"thumbnailSizes";a:3:{s:9:"node_pack";s:160:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_node_pack/uploads/media/thumbnails/426-6545f35b22453002997606.webp";s:10:"suggestion";s:161:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_suggestion/uploads/media/thumbnails/426-6545f35b22453002997606.webp";s:5:"title";s:156:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_title/uploads/media/thumbnails/426-6545f35b22453002997606.webp";}s:19:"thumbnailBackground";s:7:"#00b7ad";s:11:"publishedAt";O:17:"DateTimeImmutable":3:{s:4:"date";s:26:"2015-05-11 00:00:00.000000";s:13:"timezone_type";i:3;s:8:"timezone";s:3:"UTC";}s:8:"isExpert";b:0;s:5:"goals";s:73:"<ul> <li>Étudier la propagation des ondes sismiques.</li> </ul>";}i:1;a:9:{s:2:"id";i:169;s:5:"title";s:16:"La montre (Quiz)";s:4:"slug";s:14:"la-montre-quiz";s:9:"mediaType";s:10:"simulation";s:14:"thumbnailSizes";a:3:{s:9:"node_pack";s:160:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_node_pack/uploads/media/thumbnails/169-6545f2c86095d258039926.webp";s:10:"suggestion";s:161:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_suggestion/uploads/media/thumbnails/169-6545f2c86095d258039926.webp";s:5:"title";s:156:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_title/uploads/media/thumbnails/169-6545f2c86095d258039926.webp";}s:19:"thumbnailBackground";s:7:"#f6951d";s:11:"publishedAt";O:17:"DateTimeImmutable":3:{s:4:"date";s:26:"2015-05-11 00:00:00.000000";s:13:"timezone_type";i:3;s:8:"timezone";s:3:"UTC";}s:8:"isExpert";b:0;s:5:"goals";s:163:"<ul> <li>Enseigner/comprendre comment lire l'heure.</li> <li>Faire la comparaison des différentes représentations de l'heure.</li> </ul>";}i:2;a:9:{s:2:"id";i:1002;s:5:"title";s:24:"Un an = 365 jours et 1/4";s:4:"slug";s:22:"un-an-365-jours-et-1-4";s:9:"mediaType";s:10:"simulation";s:14:"thumbnailSizes";a:3:{s:9:"node_pack";s:177:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_node_pack/uploads/media/thumbnails/1000-calendrier-3d-1-666b2add93a44392659196.webp";s:10:"suggestion";s:178:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_suggestion/uploads/media/thumbnails/1000-calendrier-3d-1-666b2add93a44392659196.webp";s:5:"title";s:173:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_title/uploads/media/thumbnails/1000-calendrier-3d-1-666b2add93a44392659196.webp";}s:19:"thumbnailBackground";N;s:11:"publishedAt";O:17:"DateTimeImmutable":3:{s:4:"date";s:26:"2024-06-13 17:27:49.000000";s:13:"timezone_type";i:3;s:8:"timezone";s:3:"UTC";}s:8:"isExpert";b:0;s:5:"goals";s:416:"<ul> <li>Faire le lien entre le calendrier et la révolution de la Terre autour du Soleil ;</li> <li>Distinguer l'année astronomique (365,25 jours) et l'année calendaire (365 jours). </li> <li>Définir et localiser les équinoxes et les solstices ;</li> <li>Définir la ligne de changement de date (méridien 180°).</li> </ul>";}i:3;a:9:{s:2:"id";i:494;s:5:"title";s:19:"Sources de lumière";s:4:"slug";s:18:"sources-de-lumiere";s:9:"mediaType";s:10:"simulation";s:14:"thumbnailSizes";a:3:{s:9:"node_pack";s:160:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_node_pack/uploads/media/thumbnails/494-6545f38439322017403228.webp";s:10:"suggestion";s:161:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_suggestion/uploads/media/thumbnails/494-6545f38439322017403228.webp";s:5:"title";s:156:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_title/uploads/media/thumbnails/494-6545f38439322017403228.webp";}s:19:"thumbnailBackground";s:7:"#ec008d";s:11:"publishedAt";O:17:"DateTimeImmutable":3:{s:4:"date";s:26:"2015-05-11 00:00:00.000000";s:13:"timezone_type";i:3;s:8:"timezone";s:3:"UTC";}s:8:"isExpert";b:0;s:5:"goals";s:506:"<ul> <li>Distinguer sources primaires et sources secondaires, et leurs effets respectifs sur une scène ;</li> <li>Expliquer comment les ombres apparaissent après avoir identifié les trois éléments que sont la source de lumière, l'objet et le plan de projection ;</li> <li>Prédire quelle source crée une ombre ;</li> <li>Utiliser la propagation rectiligne de la lumière pour expliquer la forme d'une ombre.</li> </ul>";}i:4;a:9:{s:2:"id";i:638;s:5:"title";s:28:"Différents types de failles";s:4:"slug";s:27:"differents-types-de-failles";s:9:"mediaType";s:10:"simulation";s:14:"thumbnailSizes";a:3:{s:9:"node_pack";s:160:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_node_pack/uploads/media/thumbnails/638-6545f3e705948949390576.webp";s:10:"suggestion";s:161:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_suggestion/uploads/media/thumbnails/638-6545f3e705948949390576.webp";s:5:"title";s:156:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_title/uploads/media/thumbnails/638-6545f3e705948949390576.webp";}s:19:"thumbnailBackground";s:7:"#f487b9";s:11:"publishedAt";O:17:"DateTimeImmutable":3:{s:4:"date";s:26:"2015-05-11 00:00:00.000000";s:13:"timezone_type";i:3;s:8:"timezone";s:3:"UTC";}s:8:"isExpert";b:0;s:5:"goals";s:75:"<ul> <li>Étude des différents types de failles.</li> </ul>";}i:5;a:9:{s:2:"id";i:237;s:5:"title";s:12:"Eratosthène";s:4:"slug";s:11:"eratosthene";s:9:"mediaType";s:10:"simulation";s:14:"thumbnailSizes";a:3:{s:9:"node_pack";s:160:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_node_pack/uploads/media/thumbnails/237-6545f2eea05e6705480539.webp";s:10:"suggestion";s:161:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_suggestion/uploads/media/thumbnails/237-6545f2eea05e6705480539.webp";s:5:"title";s:156:"https://junior.preprod-yousg3q-etbsswybjvlic.fr-3.platformsh.site/media-cache/media_thumbnail_title/uploads/media/thumbnails/237-6545f2eea05e6705480539.webp";}s:19:"thumbnailBackground";s:7:"#462f92";s:11:"publishedAt";O:17:"DateTimeImmutable":3:{s:4:"date";s:26:"2015-05-11 00:00:00.000000";s:13:"timezone_type";i:3;s:8:"timezone";s:3:"UTC";}s:8:"isExpert";b:0;s:5:"goals";s:108:"<ul> <li>Illustrer la méthode d'Eratosthène pour mesurer le rayon terrestre.</li> </ul>";}}s:4:"tags";a:9:{i:0;s:5:"heure";i:1;s:4:"jour";i:2;s:4:"midi";i:3;s:6:"minuit";i:4;s:4:"nuit";i:5;s:8:"période";i:6;s:6:"soleil";i:7;s:5:"temps";i:8;s:6:"zenith";}s:12:"baseNodeName";s:19:"Le ciel et la Terre";} |
| 7 | 0.04 ms | cache | SADD wJo3GJ9dRH:tagscache-service wJo3GJ9dRH:data > anonymous-media > id=2738,locale=fr,domain=junior |
| 8 | 0.08 ms | cache | SADD wJo3GJ9dRH:tagscache-service-data > anonymous-media wJo3GJ9dRH:data > anonymous-media > id=2738,locale=fr,domain=junior |
| 9 | 0.55 ms | cache | EXEC |
| 10 | 1.95 ms | cache | MGET wJo3GJ9dRH:data > locale-page-groups > locale=fr |