{"id":245041,"date":"2025-07-02T05:32:42","date_gmt":"2025-07-01T19:32:42","guid":{"rendered":"https:\/\/science.nasa.gov\/science-research\/heliophysics\/nasa-missions-help-explain-predict-severity-of-solar-storms\/"},"modified":"2025-07-02T05:32:42","modified_gmt":"2025-07-01T19:32:42","slug":"nasa-missions-help-explain-predict-severity-of-solar-storms","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=245041","title":{"rendered":"NASA Missions Help Explain, Predict Severity of Solar Storms"},"content":{"rendered":"<p>An unexpectedly strong solar storm rocked our planet on April 23, 2023, sparking auroras as far south as southern Texas in the U.S. and taking the world by surprise.\u00a0<\/p>\n<p>Two days earlier, the Sun blasted a coronal mass ejection (CME) \u2014 a cloud of energetic particles, magnetic fields, and solar material \u2014 toward Earth.\u00a0Space scientists took notice, expecting it could cause disruptions to Earth\u2019s magnetic field, known as a geomagnetic storm.\u00a0But the CME wasn\u2019t especially fast or massive, and it was preceded by a relatively weak solar flare, suggesting the storm would be minor.\u00a0But it became severe.<\/p>\n<p>Using\u00a0<a href=\"https:\/\/science.nasa.gov\/heliophysics\/\" rel=\"noopener\">NASA heliophysics<\/a>\u00a0missions, new studies of this storm and others are helping scientists learn why some CMEs have more intense effects \u2014 and better predict the impacts of future solar eruptions on our lives.<\/p>\n<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-inline\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \"><a href=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/hpd\/space-weather\/Aurora%20from%20Larimore%20North%20Dakota%204-24-23_courtesy%20Elan%20Azriel.jpg?w=2048&#038;h=1153&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img fetchpriority=\"high\" decoding=\"async\" width=\"2048\" height=\"1153\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/hpd\/space-weather\/Aurora%20from%20Larimore%20North%20Dakota%204-24-23_courtesy%20Elan%20Azriel.jpg?w=2048&#038;h=1153&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"Curtains of green aurora shimmer against a dark blue night sky above a flat, snowy landscape. A small, dark road stretches away from the photographer toward the horizon. Leafless trees stand along the left side of the road and in the distance on the right. A band of white clouds separates the horizon from the green aurora above.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"eager\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">During the night of April 23 to 24, 2023, a geomagnetic storm produced auroras that were witnessed as far south as Arizona, Arkansas, and Texas in the U.S. This photo shows green aurora shimmering over Larimore, North Dakota, in the early morning of April 24.<\/div>\n<div class=\"hds-credits\">Copyright Elan Azriel, used with permission<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<h3 class=\"wp-block-heading\"><strong>Why Was This Storm So Intense?<\/strong><\/h3>\n<p>A\u00a0<a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/adb8d3\" rel=\"noopener\">paper<\/a>\u00a0published in the Astrophysical Journal on March 31 suggests the CME\u2019s orientation relative to Earth likely caused the April 2023 storm to become surprisingly strong.<\/p>\n<p>The researchers gathered observations from five heliophysics spacecraft across the inner solar system to study the CME in detail as it emerged from the Sun and traveled to Earth.<\/p>\n<p>They noticed\u00a0a\u00a0large coronal hole near the\u00a0CME\u2019s birthplace. Coronal holes are areas where the\u00a0<a href=\"https:\/\/science.nasa.gov\/sun\/what-is-the-solar-wind\/\" rel=\"noopener\">solar wind<\/a>\u00a0\u2014 a stream of particles flowing from the Sun \u2014 floods outward at higher than normal speeds.<\/p>\n<p>\u201cThe fast solar wind coming from this coronal hole acted like an air current, nudging the CME away from its original straight-line path and pushing it closer to Earth\u2019s orbital plane,\u201d said\u00a0the paper\u2019s lead author, Evangelos Paouris of the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland. \u201cIn addition to this deflection, the CME also rotated slightly.\u201d<\/p>\n<p>Paouris says this turned the CME\u2019s magnetic fields opposite to Earth\u2019s magnetic field and held them there \u2014 allowing more of the Sun\u2019s energy to pour into Earth\u2019s environment and intensifying the storm.<\/p>\n<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-inline\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \"><a href=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=2048&#038;h=2048&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img decoding=\"async\" width=\"2048\" height=\"2048\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=2048&#038;h=2048&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"The Sun appears in shades of gold with some brighter and darker regions, set against a black background. In the lower right part of the Sun is a bright flash of white, a solar flare.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=2048&#038;h=2048&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=150&#038;h=150&#038;fit=crop&#038;crop=faces%2Cfocalpoint 150w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=300&#038;h=300&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=768&#038;h=768&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=1024&#038;h=1024&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=1536&#038;h=1536&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=50&#038;h=50&#038;fit=crop&#038;crop=faces%2Cfocalpoint 50w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=100&#038;h=100&#038;fit=crop&#038;crop=faces%2Cfocalpoint 100w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=200&#038;h=200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=400&#038;h=400&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=600&#038;h=600&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=900&#038;h=900&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=1200&#038;h=1200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/sdo\/SDO_AIA_20230421_183705_2048_0193.jpg?w=2000&#038;h=2000&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 2048px) 100vw, 2048px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">The strength of the April 2023 geomagnetic storm was a surprise in part because the coronal mass ejection (CME) that produced it followed a relatively weak solar flare, seen as the bright area to the lower right of center in this extreme ultraviolet image of the Sun from NASA\u2019s Solar Dynamics Observatory. The CMEs that produce severe geomagnetic storms are typically preceded by stronger flares. However, a team of scientists think fast solar wind from a coronal hole (the dark area below the flare in this image) helped rotate the CME and made it more potent when it struck Earth.<\/div>\n<div class=\"hds-credits\">NASA\/SDO<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<h3 class=\"wp-block-heading\"><strong>Cool Thermosphere<\/strong><\/h3>\n<p>Meanwhile, NASA\u2019s\u00a0<a href=\"https:\/\/science.nasa.gov\/mission\/gold\/\" rel=\"noopener\">GOLD<\/a>\u00a0(Global-scale Observations of Limb and Disk) mission revealed another unexpected consequence of the April 2023 storm\u00a0at Earth.<\/p>\n<p>Before, during, and after the storm, GOLD studied the temperature in the middle thermosphere, a part of Earth\u2019s upper atmosphere about 85 to 120 miles overhead. During the storm, temperatures increased throughout GOLD\u2019s wide field of view over the Americas. But surprisingly, after the storm, temperatures dropped about 90 to 198 degrees Fahrenheit lower than they were before the storm (from about 980 to 1,070 degrees Fahrenheit before the storm to 870 to 980 degrees Fahrenheit afterward).<\/p>\n<p>\u201cOur measurement is the first to show widespread cooling in the middle thermosphere after a strong storm,\u201d said Xuguang Cai of the University of Colorado, Boulder, lead author of a\u00a0<a href=\"https:\/\/agupubs.onlinelibrary.wiley.com\/doi\/abs\/10.1029\/2025JA033912\" rel=\"noopener\">paper<\/a>\u00a0about GOLD\u2019s observations published in the journal JGR Space Physics on April 15, 2025.<\/p>\n<p>The thermosphere\u2019s temperature is important, because it affects how much drag Earth-orbiting satellites and space debris experience.<\/p>\n<p>\u201cWhen the thermosphere cools, it contracts and becomes less dense at satellite altitudes, reducing drag,\u201d Cai said. \u201cThis can cause satellites and space debris to stay in orbit longer than expected, increasing the risk of collisions. Understanding how geomagnetic storms and solar activity affect Earth\u2019s upper atmosphere helps protect technologies we all rely on \u2014 like GPS, satellites, and radio communications.\u201d<\/p>\n<h3 class=\"wp-block-heading\"><strong>Predicting When Storms Strike<\/strong><\/h3>\n<p>To predict when a CME will trigger a geomagnetic storm, or be \u201cgeoeffective,\u201d some scientists are combining observations with machine learning. A\u00a0<a href=\"https:\/\/link.springer.com\/article\/10.1007\/s11207-024-02385-w\" rel=\"noopener\">paper<\/a>\u00a0published last November in the journal Solar Physics describes one such approach called GeoCME.<\/p>\n<p>Machine learning is a type of artificial intelligence in which a computer algorithm learns from data to identify patterns, then uses those patterns to make decisions or predictions.<\/p>\n<p>Scientists trained GeoCME by giving it images from the NASA\/ESA (European Space Agency)\u00a0<a href=\"https:\/\/science.nasa.gov\/mission\/soho\/\" rel=\"noopener\">SOHO<\/a>\u00a0(Solar and Heliospheric Observatory) spacecraft of different CMEs that reached Earth along with SOHO images of the Sun before, during, and after each CME. They then told the model whether each CME produced a geomagnetic storm.<\/p>\n<p>Then, when it was given images from three different science instruments on SOHO, the model\u2019s predictions were highly accurate. Out of 21 geoeffective CMEs, the model correctly predicted all 21 of them; of 7 non-geoeffective ones, it correctly predicted 5 of them.<\/p>\n<p>\u201cThe algorithm shows promise,\u201d said heliophysicist Jack Ireland of NASA\u2019s Goddard Space Flight Center in Greenbelt, Maryland, who was not involved in the study. \u201cUnderstanding if a CME will be geoeffective or not can help us protect infrastructure in space and technological systems on Earth. This paper shows machine learning approaches to predicting geoeffective CMEs are feasible.\u201d<\/p>\n<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-inline\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \"><a href=\"https:\/\/assets.science.nasa.gov\/content\/dam\/science\/missions\/soho\/SOHO_C3_2023-04-21_cme.gif?w=512&#038;h=512&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img decoding=\"async\" width=\"512\" height=\"512\" src=\"https:\/\/assets.science.nasa.gov\/content\/dam\/science\/missions\/soho\/SOHO_C3_2023-04-21_cme.gif?w=512&#038;h=512&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"A circular, blue-colored view shows stars around the Sun, which is covered by a dark blue disk at the center. A small white circle in the center of the disk shows the size of the Sun. Streams of material extend away from the disk, and then a white halo of material erupts and moves away from the disk in all directions. A bright dot appears on the right.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">The white cloud expanding outward in this image sequence is a coronal mass ejection (CME) that erupted from the Sun on April 21, 2023. Two days later, the CME struck Earth and produced a surprisingly strong geomagnetic storm. The images in this sequence are from a coronagraph on the NASA\/ESA (European Space Agency) SOHO (Solar and Heliospheric Observatory) spacecraft. The coronagraph uses a disk to cover the Sun and reveal fainter details around it. The Sun\u2019s location and size are indicated by a small white circle. The planet Jupiter appears as a bright dot on the far right.<\/div>\n<div class=\"hds-credits\">NASA\/ESA\/SOHO<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<h3 class=\"wp-block-heading\"><strong>Earlier Warnings<\/strong><\/h3>\n<p>During a severe geomagnetic storm in May 2024 \u2014\u00a0<a href=\"https:\/\/science.nasa.gov\/science-research\/heliophysics\/how-nasa-tracked-the-most-intense-solar-storm-in-decades\/\"  rel=\"noreferrer noopener\">the strongest to rattle Earth in over 20 years<\/a> \u2014\u00a0NASA\u2019s\u00a0<a href=\"https:\/\/science.nasa.gov\/mission\/stereo\/\"  rel=\"noreferrer noopener\">STEREO<\/a>\u00a0(Solar Terrestrial Relations Observatory) measured the magnetic field structure of CMEs as they passed by.<\/p>\n<p>When a CME headed for Earth hits a spacecraft first, that spacecraft can often measure the CME and its magnetic field directly, helping scientists determine how strong the geomagnetic storm will be at Earth. Typically, the first spacecraft to get hit are one million miles from Earth toward the Sun at a place called Lagrange Point 1 (L1), giving us only 10 to 60 minutes advanced warning.<\/p>\n<p>By chance, during the May 2024 storm, when several CMEs erupted from the Sun and merged on their way to Earth, NASA\u2019s STEREO-A spacecraft happened to be between us and the Sun, about 4 million miles closer to the Sun than L1.<\/p>\n<p>A\u00a0<a href=\"https:\/\/agupubs.onlinelibrary.wiley.com\/doi\/10.1029\/2024SW004260\"  rel=\"noreferrer noopener\">paper<\/a>\u00a0published March 17, 2025, in the journal Space Weather reports that if STEREO-A had served as a CME sentinel, it could have provided an accurate prediction of the resulting storm\u2019s strength 2 hours and 34 minutes earlier than a spacecraft could at L1.<\/p>\n<p>According to the paper\u2019s lead author, Eva Weiler of the Austrian Space Weather Office in Graz, \u201cNo other Earth-directed superstorm has ever been observed by a spacecraft positioned closer to the Sun than L1.\u201d<\/p>\n<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-inline\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \"><a href=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/hpd\/05-lagrange-points-715x574.png?w=715&#038;h=574&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img decoding=\"async\" width=\"715\" height=\"574\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/hpd\/05-lagrange-points-715x574.png?w=715&#038;h=574&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"A graphic shows the Sun at the center with Earth's orbit drawn as a blue circle around it. Earth appears along the orbit to the right of the Sun, at the 3 o'clock position on the circle. L1 is marked as a white dot to the left of Earth along a horizontal dashed line that extends from the left side of the circle through the Sun and beyond Earth and the right side of the circle. L2 is marked as a white dot to the right of Earth at the right end of the dashed line. L3 is marked with a white dot on the left side of the circle, to the left of the Sun, at the left end of the dashed line. L4 is marked with a white dot near the top of the circle, at about the 1 o'clock position. L5 is marked with a white dot along the lower right part of the circle, near the 5 o'clock position.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/hpd\/05-lagrange-points-715x574.png?w=715&#038;h=574&#038;fit=crop&#038;crop=faces%2Cfocalpoint 715w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/hpd\/05-lagrange-points-715x574.png?w=300&#038;h=241&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/hpd\/05-lagrange-points-715x574.png?w=400&#038;h=321&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/hpd\/05-lagrange-points-715x574.png?w=600&#038;h=482&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w\" sizes=\"auto, (max-width: 715px) 100vw, 715px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Earth\u2019s Lagrange points are places in space where the gravitational pull between the Sun and Earth balance, making them relatively stable locations to put spacecraft.<\/div>\n<div class=\"hds-credits\">NASA<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p><strong><em>By <a href=\"mailto:vanessa.j.thomas@nasa.gov\">Vanessa Thomas<\/a><\/em><br \/><em>NASA\u2019s <a href=\"https:\/\/www.nasa.gov\/goddard\/\" data-type=\"link\" data-id=\"https:\/\/www.nasa.gov\/goddard\/\" rel=\"noopener\">Goddard Space Flight Center<\/a>, Greenbelt, Md.<\/em><\/strong><\/p>\n","protected":false},"excerpt":{"rendered":"<p>An unexpectedly strong solar storm rocked our planet on April 23, 2023, sparking auroras as far south as southern Texas in the U.S. and taking the world by surprise.\u00a0 Two days earlier, the Sun blasted a coronal mass ejection (CME) \u2014 a cloud of energetic particles, magnetic fields, and solar material \u2014 toward Earth.\u00a0Space scientists [\u2026]<\/p>\n","protected":false},"author":24,"featured_media":1,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"om_disable_all_campaigns":false,"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"_uf_show_specific_survey":0,"_uf_disable_surveys":false,"footnotes":""},"categories":[15614,16658,15766,15877,17290,16344,17291],"tags":[12280],"class_list":["post-245041","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-goddard-space-flight-center","category-gold-global-scale-observations-of-the-limb-and-disk","category-heliophysics","category-heliophysics-division","category-soho-solar-and-heliospheric-observatory","category-space-weather","category-stereo-solar-terrestrial-relations-observatory","tag-the-sun"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/245041","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/users\/24"}],"replies":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=245041"}],"version-history":[{"count":2,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/245041\/revisions"}],"predecessor-version":[{"id":245083,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/245041\/revisions\/245083"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/"}],"wp:attachment":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=245041"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=245041"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=245041"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}