{"id":1657,"date":"2016-09-27T16:13:57","date_gmt":"2016-09-27T16:13:57","guid":{"rendered":"http:\/\/www.radio-science.eu\/?page_id=1657"},"modified":"2023-11-10T14:56:57","modified_gmt":"2023-11-10T14:56:57","slug":"venus-ionosphaere","status":"publish","type":"page","link":"https:\/\/fip-koeln.de\/en_us\/missionen-und-ziele\/venus-express\/venus-ionosphaere\/","title":{"rendered":"Venus ionosphere"},"content":{"rendered":"<p>The day side ionosphere of Venus is primarily the product of solar photoionization of the planetary neutral atmosphere and subsequent photochemical processes. Its major characteristics are the main layer V2 and the underlying smaller V1 layer. While V2 is in general produced by solar radiation (extreme ultraviolet), the V1 layer is primarily produced from solar X-ray photoionization and secondary impact ionization of photo-electrons. O2+ yields the highest ion density in the main peak altitude range while at higher altitudes O+ dominates. VeRa observations from 2004 to 2014 show the day side maximum of V2 at altitudes from 135 km to 145 km. The V2 electron density in the VeRa observations varies from 15e10 to 55e10 electrons\/m3 as a function of the solar radiation incidence angle and solar activity. Information on additional properties of the Venus ionosphere in comparison with Mars can be found here.<!--:--><!--:en--><\/p>","protected":false},"excerpt":{"rendered":"<p>Die Tagionosph\u00e4re der Venus entsteht zum Gro\u00dfteil durch Photoionisation der planetaren Neutralatmosph\u00e4re und darauffolgende photochemische Prozesse. Ihre hervorstechendsten Eigenschaften sind das Hauptmaximum V2 und die darunterliegende kleinere V1-Schicht. W\u00e4hrend V2 haupts\u00e4chlich durch solare Strahlung im extremen Ultraviolett erzeugt wird, entsteht die V1 Schicht zum Gro\u00dfteil durch Photoionisation mittels solarer R\u00f6ntgenstrahlung und sekund\u00e4re Einschlagsionisation von Photo-Elektronen. [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":98,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_uag_custom_page_level_css":"","site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"default","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","ast-disable-related-posts":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"footnotes":""},"class_list":["post-1657","page","type-page","status-publish","hentry"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Venus Ionosph\u00e4re - Radio Science<\/title>\n<meta name=\"description\" content=\"Die Venus Ionosph\u00e4re ist ebenfalls Bestandteil der Forschung um diesen Planeten. Sie ist die obere, durch die Sonne ionisierte Schicht.\" \/>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/fip-koeln.de\/en_us\/missionen-und-ziele\/venus-express\/venus-ionosphaere\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Venus Ionosph\u00e4re - Radio Science\" \/>\n<meta property=\"og:description\" content=\"Die Venus Ionosph\u00e4re ist ebenfalls Bestandteil der Forschung um diesen Planeten. 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