{"id":52,"date":"2025-03-26T10:26:21","date_gmt":"2025-03-26T13:26:21","guid":{"rendered":"https:\/\/lara.iar.unlp.edu.ar\/?post_type=acora_portfolio&#038;p=52"},"modified":"2025-10-22T10:03:39","modified_gmt":"2025-10-22T13:03:39","slug":"science","status":"publish","type":"acora_portfolio","link":"https:\/\/lara.iar.unlp.edu.ar\/index.php\/portfolio\/science\/","title":{"rendered":"Science"},"content":{"rendered":"\n<h3 class=\"wp-block-heading\"><strong>The Moon offers extraordinary opportunities for radio astronomy due to:<\/strong><\/h3>\n\n\n\n<ul>\n<li>Inert environment: Minimal interference from the Moon itself.<\/li>\n\n\n\n<li>Absence of a magnetic field and atmosphere: Reduces background noise and interference.<\/li>\n\n\n\n<li>Shielding from terrestrial electromagnetic interference: Especially beneficial for observations on the far side of the Moon.<\/li>\n<\/ul>\n\n\n\n<ul>\n<li><strong>Low frequency bands:<\/strong> First steps aiming to the 5<strong>0 to 150 MHz range<\/strong>, that are difficult to access from Earth due to man made interference.<\/li>\n<\/ul>\n\n\n<div id='fwdsiscDiv0' class='fwdsisc fwd-hide'><\/div><ul id='fwdsiscPlaylist_Science_Data' class='fwdsisc no-display'><li data-source='https:\/\/lara.iar.unlp.edu.ar\/wp-content\/uploads\/2025\/03\/25.jpg' data-width='859' data-height='654' data-text-vertical-alignment='bottom'><p class='text'>LARA Solar burst simulation response below 150MHz<\/p><\/li><li data-source='https:\/\/lara.iar.unlp.edu.ar\/wp-content\/uploads\/2025\/03\/26.jpg' data-width='1044' data-height='654' data-text-vertical-alignment='bottom'><p class='text'>Green Bank Solar Radio Burst Spectrometer, RFI below 200 MHz hides different features. Image credit: Stephen White.<\/p><\/li><li data-source='https:\/\/lara.iar.unlp.edu.ar\/wp-content\/uploads\/2025\/03\/27.jpg' data-width='700' data-height='654' data-text-vertical-alignment='bottom'><p class='text'>Radio emission from Jupiter. Synchrotron radiation dominates above ~50 MHz and DAM emissions below ~ 50 MHz. de Pater 2006.<\/p><\/li><\/ul>\n\n\n\n<h4 class=\"wp-block-heading\"><strong>This capability enables observations related to:<\/strong><\/h4>\n\n\n\n<ul>\n<li><strong>Solar activity and environmental disturbances:<\/strong> Particularly in lunar orbit Low Sensitivity Measurements (LS-M).<\/li>\n\n\n\n<li><strong>Jupiter\u2019s radiation:<\/strong> Essential for diagnosing space weather in the Solar System and studying Jupiter\u2019s magnetic field High Sensitivity Measurements (HS-M).<\/li>\n<\/ul>\n\n\n\n<h4 class=\"wp-block-heading\"><strong>Technical observations:<\/strong><\/h4>\n\n\n\n<ul>\n<li>Man made radiofrequency monitoring of signal emissions at low frequency bands through cislunar orbit for future instruments and analysis (RFI-M).<\/li>\n<\/ul>\n","protected":false},"author":2,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","acora_category":[],"acora_tags":[],"_links":{"self":[{"href":"https:\/\/lara.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/acora_portfolio\/52"}],"collection":[{"href":"https:\/\/lara.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/acora_portfolio"}],"about":[{"href":"https:\/\/lara.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/types\/acora_portfolio"}],"author":[{"embeddable":true,"href":"https:\/\/lara.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/lara.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/comments?post=52"}],"wp:attachment":[{"href":"https:\/\/lara.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/media?parent=52"}],"wp:term":[{"taxonomy":"acora_category","embeddable":true,"href":"https:\/\/lara.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/acora_category?post=52"},{"taxonomy":"acora_tags","embeddable":true,"href":"https:\/\/lara.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/acora_tags?post=52"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}