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File:Wie kommt es zur Haloerscheinung?.webm

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Deutsch: Wenn Eiskristalle in großer Höhe in sogenannten Zirruswolken das Sonnenlicht brechen, kommt es zur Haloerscheinung. Aber nur bei einem Austrittswinkel von 22 Grad ist ein klassischer Halo zu sehen.
English: When ice crystals break the sunlight at high altitude in so-called cirrus clouds, the halo phenomenon occurs. But a classic halo can only be seen at an exit angle of 22 degrees.
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https://www.zdf.de/dokumentation/terra-x/wie-kommt-es-zur-haloerscheinung-creative-commons-clip-100.html

Die ganze Doku zum Clip: https://www.zdf.de/wissen/terra-xpress/das-licht-des-nordens-100.html

https://www.dwd.de/DE/service/lexikon/Functions/glossar.html?lv3=101154&lv2=101094
Author ZDF/Terra Xpress/Autorenkombinat/Birthe Heer/Sebastian Kerz/Tobias Schönke/Maximilian Heß

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Date/TimeThumbnailDimensionsUserComment
current09:53, 2 May 202334 s, 1,920 × 1,080 (44.61 MB)ZDF Terra X Redaktion (talk | contribs)Uploaded a work by ZDF/Terra Xpress/Autorenkombinat/Birthe Heer/Sebastian Kerz/Tobias Schönke/Maximilian Heß from https://www.zdf.de/dokumentation/terra-x/wie-kommt-es-zur-haloerscheinung-creative-commons-clip-100.html Die ganze Doku zum Clip: https://www.zdf.de/wissen/terra-xpress/das-licht-des-nordens-100.html https://www.dwd.de/DE/service/lexikon/Functions/glossar.html?lv3=101154&lv2=101094 with UploadWizard

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Format Bitrate Download Status Encode time
VP9 1080P 4.09 Mbps Completed 09:56, 2 May 2023 2 min 39 s
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VP9 720P 1.61 Mbps Completed 09:54, 2 May 2023 1 min 8 s
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VP9 480P 842 kbps Completed 09:54, 2 May 2023 58 s
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VP9 360P 488 kbps Completed 09:54, 2 May 2023 28 s
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VP9 240P 306 kbps Completed 09:54, 2 May 2023 26 s
Streaming 240p (VP9) 195 kbps Completed 12:30, 5 December 2023 1.0 s
WebM 360P 568 kbps Completed 09:54, 2 May 2023 17 s
Streaming 144p (MJPEG) 1.03 Mbps Completed 23:55, 18 November 2023 5.0 s
Stereo (Opus) 110 kbps Completed 06:11, 24 November 2023 1.0 s
Stereo (MP3) 128 kbps Completed 23:55, 18 November 2023 2.0 s

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