Differences

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--- results:gallery:mercury [2024/11/29 15:43] – etienne
+++ results:gallery:mercury [2024/11/29 15:49] (current) – etienne
@@ Line 1: / Line 1: @@
-===== THEMIS solar prominences and protuberances observations =====
+===== THEMIS Mercury observations =====
 Terms of use: unless otherwise specified, all graphical (webcam records, movies, pictures) or non-graphical material (text) from this site is property of CNRS-THEMIS under a [[https://creativecommons.org/licenses/by/4.0/ |Creative Commons CC-BY 4.0 license]].
@@ Line 5: / Line 5: @@
 === Images ===
-[[.png|{{.png?0x150}}]]
+[[https://www.themis.iac.es/lib/exe/fetch.php?cache=&media=mercemission_2d_20211028_1_2_d1_na_co_v1.jpg|{{https://www.themis.iac.es/lib/exe/fetch.php?cache=&media=mercemission_2d_20211028_1_2_d1_na_co_v1.jpg?0x150}}]]
-mercemission_2d_20211028_1_2_d1_na_co_v1.jpg?
 === Animations ===
+<columns 100% 50%>
 <html>
 <video onloadedmetadata="this.muted = true" height="150" controls autoplay loop><source src="/wdata/A_Merc/Mercury_AO.mp4" type="video/mp4"></video>
-</html> //
+</html> </columns>
 Solar AO running at 150Hz on Mercury in daytime //
-//
+<columns 100% 50%>
 <html>
 <video onloadedmetadata="this.muted = true" height="150" controls autoplay loop><source src="/wdata/A_Merc/Merc_scanning_over_F2slit.mp4" type="video/mp4">
-</video></html>//
+</video></html></columns>
+//
 Mercury is scanned across the spectrograph slit using our OBJ2 scanning mirror. Scanning is performed along  Mercury polar axis and acrosse its equator. Planet orientation is adjusted (if necessary), by setting an offset to the field rotator.
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