{"id":60408,"date":"2024-07-24T19:40:58","date_gmt":"2024-07-24T19:40:58","guid":{"rendered":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/?p=60408"},"modified":"2024-07-25T13:52:07","modified_gmt":"2024-07-25T13:52:07","slug":"how-small-of-a-rocket-signature-can-goes-see","status":"publish","type":"post","link":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/60408","title":{"rendered":"How Small of a Rocket Signature can GOES &#8220;see&#8221;?"},"content":{"rendered":"\n<p>There are many examples of <a href=\"https:\/\/www.nesdis.noaa.gov\/\">NOAA<\/a>&#8216;s <a href=\"http:\/\/cimss.ssec.wisc.edu\/goes\/goesdata.html\">GOES<\/a> <a href=\"http:\/\/cimss.ssec.wisc.edu\/goes\/GOESR_QuickGuides.html\">ABI<\/a> detecting the <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/category\/rocket-signatures\">spectral signatures of large rockets<\/a>. These include <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/27179\">GOES-S<\/a>, <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/44902\">GOES-T<\/a>, <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/60087\">GOES-U<\/a>, GOES-U <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/60173\">boosters<\/a>, <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/59689\">Starliner<\/a>, <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/58400\">Falcon 9<\/a>, <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/49206\">Ariane<\/a>, <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/22519\">Himawari-9<\/a>, <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/34945\">Antares<\/a>, etc. If the rocket is large enough, there is often a signal in each of the 16 ABI bands. Of course the timing of the ABI scan needs to correspond to the times of the rocket&#8217;s brightest \/ hottest phases, which is more likely if there&#8217;s a meso-scale sector covering the area of interest, either at 1-min or 30-second cadence.<\/p>\n\n\n\n<p>Smaller rockets, such as the Firefly, may be be an order of magnitude darker\/cooler compared to a Falcon, given their very different maximum thrust. The Firefly maximum rocket thrust is approximately <a href=\"https:\/\/en.wikipedia.org\/wiki\/Firefly_Alpha\">165,000 lbf<\/a> (pound-force) [736.1 kN] and the Falcon 9 is about <a href=\"https:\/\/en.wikipedia.org\/wiki\/Falcon_9\">1,700,000 lbf<\/a> [7,000 kN].<\/p>\n\n\n\n<h2 class=\"wp-block-heading\">Firefly on July 4th<\/h2>\n\n\n\n<p>Late on July 3rd (local time, early July 4th UTC) there was a <a href=\"https:\/\/www.nasaspaceflight.com\/2024\/07\/firefly-noise-of-summer\/#more-100560\">Firefly rocket launch<\/a> from <a href=\"https:\/\/www.google.com\/maps\/place\/Vandenberg+Air+Force+Base\/@34.7327376,-120.6521778,11.21z\/data=!4m6!3m5!1s0x80ec3ce573ed3d19:0xd7ea9c09f025e90f!8m2!3d34.7420267!4d-120.5724404!16zL20vMHI2NTM?entry=ttu\">Vandenberg<\/a> Air Force base.<\/p>\n\n\n\n<figure class=\"wp-block-embed is-type-rich is-provider-twitter wp-block-embed-twitter\"><div class=\"wp-block-embed__wrapper\">\n<blockquote class=\"twitter-tweet\" data-width=\"500\" data-dnt=\"true\"><p lang=\"en\" dir=\"ltr\">?<a href=\"https:\/\/twitter.com\/hashtag\/ICYMI?src=hash&amp;ref_src=twsrc%5Etfw\">#ICYMI<\/a>:  Firefly&#39;s <a href=\"https:\/\/twitter.com\/hashtag\/NoiseofSummer?src=hash&amp;ref_src=twsrc%5Etfw\">#NoiseofSummer<\/a> Alpha rocket lifted off from SLC-2 at Vandenberg Space Force Base in California at 9:04pm PDT July 3\/12:04am EDT July 4.<br><br>On board were 8?? small payloads for NASA\u2019s CubeSat Launch Initiative! <a href=\"https:\/\/t.co\/qRCLVFceGI\">pic.twitter.com\/qRCLVFceGI<\/a><\/p>&mdash; NASA&#39;s Launch Services Program (@NASA_LSP) <a href=\"https:\/\/twitter.com\/NASA_LSP\/status\/1809278891116359834?ref_src=twsrc%5Etfw\">July 5, 2024<\/a><\/blockquote><script async src=\"https:\/\/platform.twitter.com\/widgets.js\" charset=\"utf-8\"><\/script>\n<\/div><figcaption class=\"wp-element-caption\">Launched at 12:04 am EDT on July 5th. <\/figcaption><\/figure>\n\n\n\n<p>Given the smaller rocket size, a fair question is if it can be seen by the GOES ABI. Often the <a href=\"https:\/\/geosphere.ssec.wisc.edu\/#coordinate:1366870,3817853;zoom:4.7;satellite:goeswest;coverage:radm1;\">&#8220;Meso 1&#8221; sector from GOES-West<\/a> covers most of California (the <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/images\/2022\/02\/ABI_PixelArea_1km_GOES_West_CONUS_DefaultMESOs_Mar2019_Annotations.png\" data-type=\"link\" data-id=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/images\/2022\/02\/ABI_PixelArea_1km_GOES_West_CONUS_DefaultMESOs_Mar2019_Annotations.png\">default location<\/a> for this sector). This was the case on July 3, into July 4, 2024. A first look at the 16 spectral bands on the ABI, using default enhancements, shows no discernible rocket plume signature. (The signal of the <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/42331\">explosion on the maiden Firefly rocket flight<\/a> was seen by each band of the ABI.)<\/p>\n\n\n\n<figure class=\"wp-block-video\"><video controls src=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/images\/2024\/07\/G18ABI_M_PLUME_loop_GOES-18_2024186_040227_2024186_040827.mp4\"><\/video><figcaption class=\"wp-element-caption\">The 16 bands of the GOES-18 ABI with 1-min imagery on July 4, 2024. (Click to Play)<\/figcaption><\/figure>\n\n\n\n<p>Yet, a highly-enhanced (stretched) ABI band 5 (1.61 micrometers) showed a glimpse of the rocket launch. (Some instrument noise is also seen.)<\/p>\n\n\n\n<figure class=\"wp-block-video\"><video controls src=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/images\/2024\/07\/FIREFLY_loop_GOES-18_B05_enhanced_2024186_040227_2024186_040827.mp4\"><\/video><figcaption class=\"wp-element-caption\">Animation of NOAA&#8217;s GOES-18 ABI highly enhanced Band 5 (1.6 micrometer) on July 4, 2024. (Click to Play)<\/figcaption><\/figure>\n\n\n\n<p>The rocket signature is more evident in the <a href=\"https:\/\/www.star.nesdis.noaa.gov\/goes\/documents\/QuickGuide_GOESR_NtMicroRGB_final.pdf\">nighttime micro-physics RGB combination<\/a>. Watch near the coast for the first signature.<\/p>\n\n\n\n<figure class=\"wp-block-video\"><video autoplay controls loop src=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/images\/2024\/07\/GOES-18_RadM2_night_microphysics_2024186_040227_2024186_040827.mp4\"><\/video><figcaption class=\"wp-element-caption\">GOES-18 nighttime micro-physics RGB on July 4, 2024.<\/figcaption><\/figure>\n\n\n\n<p>While it&#8217;s hard to tell, there may be some indication of the <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/images\/2024\/07\/GOES_SPLIT_WINDOW_B13_MINUS_B15_FIREFLY_loop_GOES-18_2024186_040227_2024186_040827.mp4\">plume in the 11-12 micrometer split window difference<\/a> from the CONUS sectors. <\/p>\n\n\n\n<h2 class=\"wp-block-heading\">H\/T<\/h2>\n\n\n\n<p>The GOES ABI data was accessed via the UW\/SSEC Data Services. <a href=\"https:\/\/www.ssec.wisc.edu\/mcidas\/software\/x\/\">McIDAS-X<\/a>, <a href=\"https:\/\/cimss.ssec.wisc.edu\/csppgeo\/geo2grid.html\">geo2grid<\/a> and AWIPS software were used to generate the images. More <a href=\"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/archives\/category\/rocket-signatures\">UW\/CIMSS Satellite Blogs associated with rocket signatures<\/a>. <a href=\"https:\/\/www.ssec.wisc.edu\/~tims\/\">T. Schmit<\/a> works for NOAA\/NESDIS\/STAR and is stationed in Madison, WI.<\/p>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>There are many examples of NOAA&#8216;s GOES ABI detecting the spectral signatures of large rockets. These include GOES-S, GOES-T, GOES-U, GOES-U boosters, Starliner, Falcon 9, Ariane, Himawari-9, Antares, etc. If the rocket is large enough, there is often a signal in each of the 16 ABI bands. Of course the timing of the ABI scan [&hellip;]<\/p>\n","protected":false},"author":21,"featured_media":60439,"comment_status":"closed","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"footnotes":""},"categories":[10,114,106],"tags":[],"class_list":["post-60408","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-general-interpretation","category-goes-18","category-rocket-signatures"],"acf":[],"_links":{"self":[{"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/posts\/60408","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/users\/21"}],"replies":[{"embeddable":true,"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/comments?post=60408"}],"version-history":[{"count":16,"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/posts\/60408\/revisions"}],"predecessor-version":[{"id":60461,"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/posts\/60408\/revisions\/60461"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/media\/60439"}],"wp:attachment":[{"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/media?parent=60408"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/categories?post=60408"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/cimss.ssec.wisc.edu\/satellite-blog\/wp-json\/wp\/v2\/tags?post=60408"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}