{"id":26582,"date":"2025-06-15T13:24:28","date_gmt":"2025-06-15T07:39:28","guid":{"rendered":"https:\/\/www.revoscience.com\/en\/?p=26582"},"modified":"2025-06-15T13:24:30","modified_gmt":"2025-06-15T07:39:30","slug":"solar-orbiter-gets-world-first-views-of-the-suns-poles","status":"publish","type":"post","link":"https:\/\/www.revoscience.com\/en\/solar-orbiter-gets-world-first-views-of-the-suns-poles\/","title":{"rendered":"Solar Orbiter gets world-first views of the Sun\u2019s poles"},"content":{"rendered":"\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio\"><div class=\"wp-block-embed__wrapper\">\n<div class=\"newspaper-x-video-container\"><iframe loading=\"lazy\" title=\"Solar Orbiter zooms into the Sun\u2019s south pole\" width=\"750\" height=\"422\" src=\"https:\/\/www.youtube.com\/embed\/TU4DcDgaMM0?feature=oembed&#038;enablejsapi=1&#038;origin=https:\/\/www.revoscience.com\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe><\/div>\n<\/div><\/figure>\n\n\n\n<p>Any image you have ever seen of the Sun was taken from around the Sun\u2019s equator. This is because Earth, the other planets, and all other modern spacecraft orbit the Sun within a flat disc around the Sun called the ecliptic plane. By tilting its orbit out of this plane, Solar Orbiter reveals the Sun from a whole new angle.<\/p>\n\n\n\n<p>The video above compares Solar Orbiter\u2019s view (in yellow) with the one from Earth (grey) on 23 March 2025. At the time, Solar Orbiter was viewing the Sun from an angle of 17\u00b0 below the solar equator, enough to directly see the Sun\u2019s south pole. Over the coming years, the spacecraft&nbsp;<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/9TfHMExlpzycMv2cbZuweItX9PLZQgYZiLrfOGbZueMx\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">will tilt its orbit even further<\/a>, so the best views are yet to come.<\/p>\n\n\n\n<p>\u201cToday we reveal humankind\u2019s first-ever views of the Sun\u2019s pole,\u201d says Prof. Carole Mundell, ESA&#8217;s Director of Science. \u201cThe Sun is our nearest star, giver of life and potential disruptor of modern space and ground power systems, so we must understand how it works and learn to predict its behavior. These new, unique views from our Solar Orbiter mission are the beginning of a new era of solar science.&#8221;<\/p>\n\n\n\n<p><strong>All eyes on the Sun\u2019s south pole<\/strong><\/p>\n\n\n\n<figure class=\"wp-block-image size-full\"><img data-dominant-color=\"584641\" data-has-transparency=\"false\" style=\"--dominant-color: #584641;\" loading=\"lazy\" decoding=\"async\" width=\"960\" height=\"540\" sizes=\"auto, (max-width: 960px) 100vw, 960px\" src=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA.webp\" alt=\"\" class=\"wp-image-26583 not-transparent\" title=\"\" srcset=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA.webp 960w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-675x380.webp 675w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-768x432.webp 768w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-150x84.webp 150w\" \/><\/figure>\n\n\n\n<p>The collage above shows the Sun\u2019s south pole as recorded on 16\u201317 March 2025, when Solar Orbiter was viewing the Sun from an angle of 15\u00b0 below the solar equator. This was the mission\u2019s first high-angle observation campaign, a few days before reaching its current maximum viewing angle of 17\u00b0.&nbsp;<\/p>\n\n\n\n<p>The images shown above were taken by three of&nbsp;<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/yRa1u0yHG3mJl46EIlMoAsJnAjYWoChBBMwRHrjBApsx\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">Solar Orbiter\u2019s scientific instruments<\/a>: the Polarimetric and Helioseismic Imager (PHI), the Extreme Ultraviolet Imager (EUI), and the Spectral Imaging of the Coronal Environment (SPICE) instrument. Click on the image to zoom in and see video versions of the data.&nbsp;<\/p>\n\n\n\n<p>\u201cWe didn\u2019t know what exactly to expect from these first observations\u2014the Sun\u2019s poles are literally terra incognita,\u201d says Prof. Sami Solanki, who leads the PHI instrument team from the Max Planck Institute for Solar System Research (MPS) in Germany.<\/p>\n\n\n\n<p>The instruments each observe the Sun in a different way. PHI images the Sun in visible light (top left) and maps the Sun\u2019s surface magnetic field (top center).<\/p>\n\n\n\n<p>EUI images the Sun in ultraviolet light (top right), revealing the million-degree charged gas in the Sun\u2019s outer atmosphere, the corona. The SPICE instrument (bottom row) captures light coming from different temperatures of charged gas above the Sun\u2019s surface, thereby revealing different layers of the Sun&#8217;s atmosphere.<\/p>\n\n\n\n<p>By comparing and analyzing the complementary observations made by these three imaging instruments, we can learn about how material moves in the Sun\u2019s outer layers. This may reveal unexpected patterns, such as polar vortices (swirling gas) similar to those seen around the poles of&nbsp;<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/PAtMTZ5jchFupRGRS2dF2pbMGkBatsu8Ncf277qb7X0x\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">Venus<\/a>&nbsp;and&nbsp;<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/p1IGpd7W7ytalcCFUH6K5ie7nkCw94cQaXTwzBG26lox\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">Saturn<\/a>.<\/p>\n\n\n\n<p>These groundbreaking new observations are also key to understanding the Sun\u2019s magnetic field and why it flips roughly every 11 years, coinciding with a peak in solar activity. Current models and predictions of the&nbsp;<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/RYdQyQcKej0eZadJH4sZwcB40SUrlGzPynpeJvUnR2Ix\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">11-year solar cycle<\/a>&nbsp;fall short of being able to predict exactly when and how powerfully the Sun will reach its most active state.<\/p>\n\n\n\n<p><strong>Messy magnetism at solar maximum<\/strong><\/p>\n\n\n<div class=\"wp-block-image\">\n<figure class=\"alignright size-large is-resized\"><img data-dominant-color=\"ebebc0\" data-has-transparency=\"false\" loading=\"lazy\" decoding=\"async\" width=\"621\" height=\"1100\" sizes=\"auto, (max-width: 621px) 100vw, 621px\" src=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole_article-621x1100.webp\" alt=\"\" class=\"wp-image-26584 not-transparent\" style=\"--dominant-color: #ebebc0; width:309px;height:auto\" title=\"\" srcset=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole_article-621x1100.webp 621w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole_article-381x675.webp 381w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole_article-768x1360.webp 768w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole_article-867x1536.webp 867w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole_article-150x266.webp 150w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole_article.webp 960w\" \/><\/figure>\n<\/div>\n\n\n<div class=\"wp-block-group is-nowrap is-layout-flex wp-container-core-group-is-layout-ad2f72ca wp-block-group-is-layout-flex\">\n<p>One of the first scientific findings from Solar Orbiter\u2019s polar observations is the discovery that at the south pole, the Sun\u2019s magnetic field is currently a mess. While a normal magnet has a clear north and south pole, the PHI instrument\u2019s magnetic field measurements show that both north and south polarity magnetic fields are present at the Sun\u2019s south pole.<\/p>\n<\/div>\n\n\n\n<p>This happens only for a short time during each solar cycle, at solar maximum, when the Sun\u2019s magnetic field flips and is at its most active. After the field flip, a single polarity should slowly build up and take over the Sun\u2019s poles. In 5\u20136 years from now, the Sun will reach its next solar minimum, during which its magnetic field is at its most orderly and the Sun displays its lowest levels of activity.<\/p>\n\n\n\n<p>\u201cHow exactly this build-up occurs is still not fully understood, so Solar Orbiter has reached high latitudes at just the right time to follow the whole process from its unique and advantageous perspective,\u201d notes Sami.<\/p>\n\n\n\n<p>PHI\u2019s view of the full Sun\u2019s magnetic field puts these measurements in context. The darker the colour (red\/blue), the stronger the magnetic field is along the line of sight from Solar Orbiter to the Sun.<\/p>\n\n\n\n<p>The strongest magnetic fields are found in two bands on either side of the Sun\u2019s equator. The dark red and dark blue regions highlight active regions, where the magnetic fields get concentrated in sunspots on the Sun\u2019s surface (<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/M0sxC9M7OJylTaJfU72Z1xFL0UmwqcAtxcdxjLZdhjcx\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">photosphere<\/a>).<\/p>\n\n\n\n<p>Meanwhile, both the Sun\u2019s south and north poles are speckled with red and blue patches. This demonstrates that at small scales, the Sun\u2019s magnetic field has a complex and ever-changing structure.<\/p>\n\n\n\n<p><strong>SPICE measures movement for the first time<\/strong><\/p>\n\n\n\n<figure class=\"wp-block-image size-large\"><img data-dominant-color=\"726653\" data-has-transparency=\"false\" style=\"--dominant-color: #726653;\" loading=\"lazy\" decoding=\"async\" width=\"1100\" height=\"550\" sizes=\"auto, (max-width: 1100px) 100vw, 1100px\" src=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/solar-orbiter-spice-instrument-1100x550.webp\" alt=\"\" class=\"wp-image-26588 not-transparent\" title=\"\" srcset=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/solar-orbiter-spice-instrument-1100x550.webp 1100w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/solar-orbiter-spice-instrument-675x337.webp 675w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/solar-orbiter-spice-instrument-768x384.webp 768w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/solar-orbiter-spice-instrument-150x75.webp 150w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/solar-orbiter-spice-instrument.webp 1403w\" \/><\/figure>\n\n\n\n<p>Another interesting \u2018first\u2019 for Solar Orbiter comes from the SPICE instrument. Being an imaging spectrograph, SPICE measures the light (spectral lines) sent out by specific chemical elements\u2014hydrogen, carbon, oxygen, neon, and magnesium\u2014at known temperatures. For the last five years, SPICE has used this to reveal what happens in different layers above the Sun\u2019s surface.<\/p>\n\n\n\n<p>Now, for the first time, the SPICE team has also managed to use precise tracking of spectral lines to measure how fast clumps of solar material are moving. This is known as a \u2018Doppler measurement\u2019, named after the same effect that makes passing ambulance sirens change pitch as they drive by.<\/p>\n\n\n\n<p>The resulting velocity map reveals how solar material moves within a specific layer of the Sun. Below, you can directly compare the location and movement of particles (carbon ions) in a thin layer called the&nbsp;<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/NrOs91GAhilnQNawvXe8mxrCqUAJvPuxCnfzGK9yFeox\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">&#8216;transition region\u2019<\/a>, where the Sun&#8217;s temperature rapidly increases from 10,000 \u00b0C to hundreds of thousands of degrees.<\/p>\n\n\n\n<p>The left image shows a radiance map, revealing the locations of clumps of carbon ions. The right image shows a velocity map, where blue and red indicate how fast the carbon ions are moving towards and away from the Solar Orbiter spacecraft, respectively. Darker blue and red patches are related to material flowing faster due to small plumes or jets.<\/p>\n\n\n\n<p>Crucially, Doppler measurements can reveal how particles are flung out from the Sun in the form of&nbsp;<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/xb4VzL2jesr7M91aOkkALNraIRIMA95TxGxdauJYqDEx\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">solar wind<\/a>. Uncovering how the Sun produces solar wind is one of Solar Orbiter\u2019s&nbsp;<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/rFWx5EzYogWZ2tJ9SyYsEHpsvdjWuBWHYlSxdbnfxv8x\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">key scientific goals<\/a>.<\/p>\n\n\n\n<p>\u201cDoppler measurements of solar wind setting off from the Sun by current and past space missions have been hampered by the grazing view of the solar poles. Measurements from high latitudes, now possible with Solar Orbiter, will be a revolution in solar physics,\u201d says SPICE team leader Fr\u00e9d\u00e9ric Auch\u00e8re from the University of Paris-Saclay (France).<\/p>\n\n\n\n<p><strong>The best is yet to come<\/strong><\/p>\n\n\n\n<figure class=\"wp-block-image size-full\"><img data-dominant-color=\"3c3f39\" data-has-transparency=\"false\" style=\"--dominant-color: #3c3f39;\" loading=\"lazy\" decoding=\"async\" width=\"960\" height=\"540\" sizes=\"auto, (max-width: 960px) 100vw, 960px\" src=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/Why_Solar_Orbiter_is_angling_towards_the_Sun_s_poles_article.webp\" alt=\"\" class=\"wp-image-26587 not-transparent\" title=\"\" srcset=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/Why_Solar_Orbiter_is_angling_towards_the_Sun_s_poles_article.webp 960w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/Why_Solar_Orbiter_is_angling_towards_the_Sun_s_poles_article-675x380.webp 675w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/Why_Solar_Orbiter_is_angling_towards_the_Sun_s_poles_article-768x432.webp 768w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/Why_Solar_Orbiter_is_angling_towards_the_Sun_s_poles_article-150x84.webp 150w\" \/><\/figure>\n\n\n\n<p>These are just the first observations made by Solar Orbiter from its newly inclined orbit, and much of this first set of data still awaits further analysis. The complete dataset of Solar Orbiter&#8217;s first full \u2018pole-to-pole&#8217; flight past the Sun is expected to arrive on Earth by October 2025. All ten of&nbsp;<a href=\"https:\/\/315157966b744091b431016c8a8048a6.svc.dynamics.com\/t\/t\/nM5cHdUCYrtRxIFZz6inmxej2eLW2etNM4MABxu4nHsx\/Zq9DKPNfrM4UdRQIqPBO5Kt8Tx5frjkhxfx5oKDFu1Yx\" target=\"_blank\" rel=\"noreferrer noopener\">Solar Orbiter\u2019s scientific instruments&nbsp;<\/a>will collect unprecedented data in the years to come.<\/p>\n\n\n\n<p>\u201cThis is just the first step of Solar Orbiter&#8217;s &#8216;stairway to heaven&#8217;: in the coming years, the spacecraft will climb further out of the ecliptic plane for even better views of the Sun&#8217;s polar regions. These data will transform our understanding of the Sun\u2019s magnetic field, the solar wind, and solar activity,\u201d notes Daniel M\u00fcller, ESA\u2019s Solar Orbiter project scientist.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Any image you have ever seen of the Sun was taken from around the Sun\u2019s equator. This is because Earth, the other planets, and all other modern spacecraft orbit the Sun within a flat disc around the Sun called the ecliptic plane. By tilting its orbit out of this plane, Solar Orbiter reveals the Sun [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":26583,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[3],"tags":[],"class_list":["post-26582","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news"],"featured_image_urls":{"full":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA.webp",960,540,false],"thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-200x200.webp",200,200,true],"medium":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-675x380.webp",675,380,true],"medium_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-768x432.webp",750,422,true],"large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA.webp",750,422,false],"1536x1536":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA.webp",960,540,false],"2048x2048":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA.webp",960,540,false],"ultp_layout_landscape_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA.webp",960,540,false],"ultp_layout_landscape":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-870x540.webp",870,540,true],"ultp_layout_portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-600x540.webp",600,540,true],"ultp_layout_square":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-600x540.webp",600,540,true],"newspaper-x-single-post":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-760x490.webp",760,490,true],"newspaper-x-recent-post-big":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-550x360.webp",550,360,true],"newspaper-x-recent-post-list-image":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-95x65.webp",95,65,true],"web-stories-poster-portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-640x540.webp",640,540,true],"web-stories-publisher-logo":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-96x96.webp",96,96,true],"web-stories-thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2025\/06\/the-sun-ESA-150x84.webp",150,84,true]},"author_info":{"info":["RevoScience"]},"category_info":"<a href=\"https:\/\/www.revoscience.com\/en\/category\/news\/\" rel=\"category tag\">News<\/a>","tag_info":"News","comment_count":"0","_links":{"self":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/26582","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/comments?post=26582"}],"version-history":[{"count":3,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/26582\/revisions"}],"predecessor-version":[{"id":26590,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/26582\/revisions\/26590"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media\/26583"}],"wp:attachment":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media?parent=26582"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/categories?post=26582"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/tags?post=26582"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}