{"id":16433,"date":"2025-04-30T10:50:07","date_gmt":"2025-04-30T08:50:07","guid":{"rendered":"https:\/\/micromega-dynamics.com\/project\/astronomy\/"},"modified":"2025-05-12T10:22:32","modified_gmt":"2025-05-12T08:22:32","slug":"astronomy","status":"publish","type":"project","link":"https:\/\/micromega-dynamics.com\/de\/project\/astronomy\/","title":{"rendered":"Astronomie"},"content":{"rendered":"<p>[et_pb_section fb_built=&#8220;1&#8243; admin_label=&#8220;Header&#8220; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; background_image=&#8220;https:\/\/micromega-dynamics.com\/files\/uploads\/2024\/11\/Cover-Usecase-1-1.jpg&#8220; parallax=&#8220;on&#8220; custom_padding=&#8220;8vw||0vw||false|false&#8220; border_radii=&#8220;off|||0vw|0vw&#8220; collapsed=&#8220;on&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_row custom_padding_last_edited=&#8220;on|phone&#8220; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; max_width=&#8220;1800px&#8220; custom_padding=&#8220;|237px||||&#8220; custom_padding_tablet=&#8220;|237px||||&#8220; custom_padding_phone=&#8220;|0px|||false|false&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_column type=&#8220;4_4&#8243; _builder_version=&#8220;4.22.0&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_text _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;2a1fa9e3-278a-4815-a8b6-86e3861ec73b&#8220; text_text_color=&#8220;#3C9100&#8243; header_text_color=&#8220;#ffffff&#8220; header_font_size=&#8220;56px&#8220; header_4_font=&#8220;|600|||||||&#8220; header_4_text_color=&#8220;#ffffff&#8220; header_4_font_size=&#8220;23px&#8220; background_color=&#8220;rgba(10,10,10,0.5)&#8220; max_width=&#8220;1440px&#8220; custom_margin=&#8220;||||true|true&#8220; custom_padding=&#8220;10px|10px|10px|10px|true|true&#8220; border_radii=&#8220;on|5px|5px|5px|5px&#8220; global_colors_info=&#8220;{}&#8220;]<\/p>\n<h1>Astronomie<\/h1>\n<h4><span class=\"OYPEnA font-feature-liga-off font-feature-clig-off font-feature-calt-off text-decoration-none text-strikethrough-none\">Technische Dienstleistungen : Aktuatoren<\/span><\/h4>\n<p>[\/et_pb_text][et_pb_button button_url=&#8220;@ET-DC@eyJkeW5hbWljIjp0cnVlLCJjb250ZW50IjoicG9zdF9saW5rX3VybF9wYWdlIiwic2V0dGluZ3MiOnsicG9zdF9pZCI6IjEzMjczIiwiZW5hYmxlX2h0bWwiOiJvZmYifX0=@&#8220; button_text=&#8220;Kontaktieren Sie uns&#8220; _builder_version=&#8220;4.27.4&#8243; _dynamic_attributes=&#8220;button_url&#8220; _module_preset=&#8220;8904402d-84ed-403f-be1c-6de59b1d4dcb&#8220; button_bg_color=&#8220;#0071BB&#8220; button_border_radius=&#8220;5px&#8220; button_on_hover=&#8220;off&#8220; custom_padding=&#8220;11px|32px|11px|32px|true|true&#8220; hover_enabled=&#8220;0&#8243; global_colors_info=&#8220;{}&#8220; sticky_enabled=&#8220;0&#8243;][\/et_pb_button][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=&#8220;1&#8243; admin_label=&#8220;About&#8220; _builder_version=&#8220;4.24.0&#8243; _module_preset=&#8220;default&#8220; custom_padding=&#8220;||3px|||&#8220; collapsed=&#8220;on&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_row column_structure=&#8220;2_3,1_3&#8243; _builder_version=&#8220;4.24.0&#8243; _module_preset=&#8220;default&#8220; max_width=&#8220;1800px&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_column type=&#8220;2_3&#8243; _builder_version=&#8220;4.22.0&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_text _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;d4beb851-2ed0-4803-97e0-f2d50020575e&#8220; global_colors_info=&#8220;{}&#8220;]<\/p>\n<h2><span class=\"OYPEnA font-feature-liga-off font-feature-clig-off font-feature-calt-off text-decoration-none text-strikethrough-none\">Astronomie<\/span><\/h2>\n<p>[\/et_pb_text][et_pb_text _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;52afce6b-0212-4de0-94d1-88b79e261070&#8243; global_colors_info=&#8220;{}&#8220;]Um die sehr hohe Aufl\u00f6sung zu erreichen, die f\u00fcr die Beobachtung weit entfernter astronomischer Objekte erforderlich ist, m\u00fcssen die Spiegel gro\u00dfer Astronomieteleskope ihre Form unter allen Umst\u00e4nden beibehalten, trotz st\u00e4ndig wechselnder Ausrichtungen und Temperaturen. Um dieses Ziel zu erreichen, sind die Spiegel normalerweise sehr dick, was sie teuer und schwer macht und zu sehr starken\/steifen mechanischen Strukturen f\u00fchrt, um sie zu st\u00fctzen. Heutzutage bevorzugen die Hersteller von Teleskopen d\u00fcnnere und leichtere Spiegel, die mit einem Netzwerk von Aktuatoren zur Spiegelformung ausgestattet sind, um ihre unzureichende Steifigkeit auszugleichen und die reflektierende Oberfl\u00e4che des Spiegels st\u00e4ndig in einem m\u00f6glichst perfekten Zustand zu halten.[\/et_pb_text][\/et_pb_column][et_pb_column type=&#8220;1_3&#8243; _builder_version=&#8220;4.22.0&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_image src=&#8220;https:\/\/micromega-dynamics.com\/files\/uploads\/2024\/11\/ry-10.jpg&#8220; alt=&#8220;Astronomie Schwingungskontrolle&#8220; title_text=&#8220;Astronomie Schwingungskontrolle&#8220; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; custom_margin=&#8220;34px|||||&#8220; border_radii=&#8220;on|8px|8px|8px|8px&#8220; global_colors_info=&#8220;{}&#8220;][\/et_pb_image][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=&#8220;1&#8243; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; background_color=&#8220;#f9f9f9&#8243; custom_padding=&#8220;14px||20px|||&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_row column_structure=&#8220;1_2,1_2&#8243; _builder_version=&#8220;4.24.3&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_column type=&#8220;1_2&#8243; _builder_version=&#8220;4.24.3&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_text _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;d4beb851-2ed0-4803-97e0-f2d50020575e&#8220; global_colors_info=&#8220;{}&#8220;]<\/p>\n<h3><strong><span class=\"OYPEnA font-feature-liga-off font-feature-clig-off font-feature-calt-off text-decoration-none text-strikethrough-none\">Was wir tun<\/span><\/strong><\/h3>\n<div class=\"flex max-w-full flex-col flex-grow\">\n<div data-message-author-role=\"assistant\" data-message-id=\"c7f50d3f-bbc0-43e0-9f03-e40e25aa0859\" dir=\"auto\" class=\"min-h-8 text-message flex w-full flex-col items-end gap-2 whitespace-normal break-words [.text-message+&amp;]:mt-5\">\n<div class=\"flex w-full flex-col gap-1 empty:hidden first:pt-[3px]\">\n<div class=\"markdown prose w-full break-words dark:prose-invert light\">\n<ul>\n<li>Design und Herstellung von spiegelnden<span> <\/span><a href=\"https:\/\/micromega-dynamics.com\/engineering-services\/actuators\/\" title=\"Entwicklung und Herstellung von Aktuatoren zur Spiegelformung auf der Grundlage sehr strenger Kundenspezifikationen (Kraftbereich und -genauigkeit, Verlustleistung, parasit\u00e4re Steifigkeit...). \">Aktuatoren<\/a><span> <\/span>basierend auf sehr strengen Kundenspezifikationen (Kraftbereich und -genauigkeit, Verlustleistung, parasit\u00e4re Steifigkeit usw.)<\/li>\n<li><a href=\"https:\/\/micromega-dynamics.com\/de\/engineering-services\/calibration\/\" title=\"Kalibrierung von Aktuatoren zur Spiegelformung\">Kalibrierung<\/a><span> <\/span>von Spiegelformungsaktuatoren<\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<p>[\/et_pb_text][\/et_pb_column][et_pb_column type=&#8220;1_2&#8243; _builder_version=&#8220;4.24.3&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_text _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;d4beb851-2ed0-4803-97e0-f2d50020575e&#8220; global_colors_info=&#8220;{}&#8220;]<\/p>\n<h3><strong><span class=\"OYPEnA font-feature-liga-off font-feature-clig-off font-feature-calt-off text-decoration-none text-strikethrough-none\">Vorteile<\/span><\/strong><\/h3>\n<div class=\"flex max-w-full flex-col flex-grow\">\n<div data-message-author-role=\"assistant\" data-message-id=\"c7f50d3f-bbc0-43e0-9f03-e40e25aa0859\" dir=\"auto\" class=\"min-h-8 text-message flex w-full flex-col items-end gap-2 whitespace-normal break-words [.text-message+&amp;]:mt-5\">\n<div class=\"flex w-full flex-col gap-1 empty:hidden first:pt-[3px]\">\n<div class=\"markdown prose w-full break-words dark:prose-invert light\">\n<ul>\n<li>Integriertes Know-how (Mechanik, eingebettete Elektronik, Echtzeitsoftware)<\/li>\n<li>Entwicklung spezieller Sensoren und Aktoren mit Konditionierungs- und Steuerelektronik<\/li>\n<li>Qualifizierung des Mechanismus (d.h. Leistungs-, Temperatur- und Schwingungstests)<\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=&#8220;1&#8243; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_row _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_column type=&#8220;4_4&#8243; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_text _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; header_2_font_size=&#8220;54px&#8220; global_colors_info=&#8220;{}&#8220;]<\/p>\n<h2 style=\"text-align: center;\">Anwendungsf\u00e4lle<\/h2>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][et_pb_row column_structure=&#8220;1_2,1_2&#8243; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_column type=&#8220;1_2&#8243; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_text _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;52afce6b-0212-4de0-94d1-88b79e261070&#8243; global_colors_info=&#8220;{}&#8220;]<\/p>\n<h2>DKIST-Sonnenteleskop<\/h2>\n<p>Das Daniel K. Inouye Solar Telescope (DKIST) ist das<a href=\"https:\/\/www.nso.edu\/telescopes\/dki-solar-telescope\/\" title=\"Das gr\u00f6\u00dfte Sonnenteleskop der Welt\">gr\u00f6\u00dfte Sonnenteleskop der Welt<\/a><span> <\/span>.<\/p>\n<p>Das Design und die Herstellung des Prim\u00e4rspiegels mit einem Durchmesser von 4,2 m und der ihn umgebenden Zelle wurde an das Unternehmen<span> <\/span><a href=\"https:\/\/www.amos.be\/project\/mirror-cell-for-dkist\" title=\"AMOS\">AMOS<\/a> vergeben.<\/p>\n<p>Als Unterauftragnehmer von AMOS hat Micromega die 142 hydraulischen und pneumatischen Aktuatoren entwickelt und hergestellt, die die Form des d\u00fcnnen Prim\u00e4rspiegels kontinuierlich mit einer Genauigkeit von mehr als 45 nm RMS korrigieren.<\/p>\n<p>Die Zelle wurde im Jahr 2017 in das Teleskop integriert und getestet. Im Januar 2020 enth\u00fcllte das Daniel K. Inouye Solar Telescope die detailliertesten Bilder, die jemals von der Oberfl\u00e4che unserer Sonne aufgenommen wurden. <\/p>\n<p>[\/et_pb_text][\/et_pb_column][et_pb_column type=&#8220;1_2&#8243; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_image src=&#8220;https:\/\/micromega-dynamics.com\/files\/uploads\/2024\/11\/ry-11.jpg&#8220; alt=&#8220;Astronomie Schwingungskontrolle und \u00dcberwachung&#8220; title_text=&#8220;Astronomie Schwingungskontrolle und \u00dcberwachung&#8220; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][\/et_pb_image][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=&#8220;1&#8243; _builder_version=&#8220;4.24.3&#8243; _module_preset=&#8220;default&#8220; custom_padding=&#8220;0px|||||&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_row _builder_version=&#8220;4.24.3&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_column type=&#8220;4_4&#8243; _builder_version=&#8220;4.24.3&#8243; _module_preset=&#8220;default&#8220; global_colors_info=&#8220;{}&#8220;][et_pb_text _builder_version=&#8220;4.24.3&#8243; _module_preset=&#8220;default&#8220; header_3_font=&#8220;|600|||||||&#8220; header_3_font_size=&#8220;31px&#8220; global_colors_info=&#8220;{}&#8220;]<\/p>\n<h3>Andere Projekte entdecken<\/h3>\n<p>[\/et_pb_text][et_pb_portfolio fullwidth=&#8220;off&#8220; posts_number=&#8220;4&#8243; include_categories=&#8220;current&#8220; show_categories=&#8220;off&#8220; show_pagination=&#8220;off&#8220; _builder_version=&#8220;4.27.2&#8243; _module_preset=&#8220;default&#8220; title_font=&#8220;|700|||||||&#8220; title_line_height=&#8220;1.8em&#8220; global_colors_info=&#8220;{}&#8220;][\/et_pb_portfolio][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Astronomie Technische Dienstleistungen : AktuatorenAstronomieUm die sehr hohe Aufl\u00f6sung zu erreichen, die f\u00fcr die Beobachtung weit entfernter astronomischer Objekte erforderlich ist, m\u00fcssen die Spiegel gro\u00dfer Astronomieteleskope ihre Form unter allen Umst\u00e4nden beibehalten, trotz st\u00e4ndig wechselnder Ausrichtungen und Temperaturen. Um dieses Ziel zu erreichen, sind die Spiegel normalerweise sehr dick, was sie teuer und schwer macht [&hellip;]<\/p>\n","protected":false},"author":13,"featured_media":16436,"comment_status":"open","ping_status":"closed","template":"","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":"","footnotes":""},"project_category":[121],"project_tag":[],"class_list":["post-16433","project","type-project","status-publish","has-post-thumbnail","hentry","project_category-uberwachung-von-vibrationen"],"yoast_head":"<!-- This site is optimized with the Yoast SEO Premium plugin v27.5 (Yoast SEO v27.5) - https:\/\/yoast.com\/product\/yoast-seo-premium-wordpress\/ -->\n<title>Astronomie: Adaptive Optik Aktuatoren - Micromega Dynamics<\/title>\n<meta name=\"description\" content=\"Leichte Teleskopspiegel verwenden Aktuatoren, um eine perfekte Reflexion aufrechtzuerhalten, die sich an Ausrichtungs- und Temperaturschwankungen anpasst.\" \/>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/micromega-dynamics.com\/de\/project\/astronomy\/\" \/>\n<meta property=\"og:locale\" content=\"de_DE\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Astronomie\" \/>\n<meta property=\"og:description\" content=\"Leichte Teleskopspiegel verwenden Aktuatoren, um eine perfekte Reflexion aufrechtzuerhalten, die sich an Ausrichtungs- und Temperaturschwankungen anpasst.\" \/>\n<meta property=\"og:url\" content=\"https:\/\/micromega-dynamics.com\/de\/project\/astronomy\/\" \/>\n<meta property=\"og:site_name\" content=\"Micromega Dynamics\" \/>\n<meta property=\"article:modified_time\" content=\"2025-05-12T08:22:32+00:00\" \/>\n<meta property=\"og:image\" content=\"https:\/\/micromega-dynamics.com\/files\/uploads\/2024\/11\/ry-1-2.jpg\" \/>\n\t<meta property=\"og:image:width\" content=\"900\" \/>\n\t<meta property=\"og:image:height\" content=\"900\" \/>\n\t<meta property=\"og:image:type\" content=\"image\/jpeg\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Gesch\u00e4tzte Lesezeit\" \/>\n\t<meta name=\"twitter:data1\" content=\"5\u00a0Minuten\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\"@context\":\"https:\\\/\\\/schema.org\",\"@graph\":[{\"@type\":\"WebPage\",\"@id\":\"https:\\\/\\\/micromega-dynamics.com\\\/de\\\/project\\\/astronomy\\\/\",\"url\":\"https:\\\/\\\/micromega-dynamics.com\\\/de\\\/project\\\/astronomy\\\/\",\"name\":\"Astronomie: Adaptive Optik Aktuatoren - 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