{"id":23799,"date":"2025-06-16T00:16:15","date_gmt":"2025-06-15T16:16:15","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/solar-orbiter-makes-first-ever-observations-of-suns-south-pole-reveals-messy-magnetic-field\/"},"modified":"2025-06-16T00:16:15","modified_gmt":"2025-06-15T16:16:15","slug":"solar-orbiter-makes-first-ever-observations-of-suns-south-pole-reveals-messy-magnetic-field","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/solar-orbiter-makes-first-ever-observations-of-suns-south-pole-reveals-messy-magnetic-field\/","title":{"rendered":"Solar Orbiter makes first ever observations of Sun\u2019s south pole, reveals messy magnetic field"},"content":{"rendered":"<p>Following a flyby of Venus in February that successfully increased its orbital inclination around the Sun, the European Space Agency\u2019s Solar Orbiter recently imaged the Sun\u2019s poles for the first time. The images are the first to show how the Sun\u2019s immense magnetic field interacts at its poles, and will improve scientists\u2019 understanding of the solar cycle and solar weather.<\/p>\n<p>While the images are the first of the solar poles ever taken, they are not the last. Over the next five years, Solar Orbiter\u2019s orbit will continue to increase in inclination, giving scientists unparalleled views of the Sun\u2019s northern and southern poles.<\/p>\n<\/p>\n<p>Given the location of Earth and the other planets within the Sun\u2019s ecliptic plane, every photograph ever taken of the Sun is taken facing directly at the solar equator. Solar Orbiter is the first spacecraft to ever significantly shift the inclination of its heliocentric orbit beyond the ecliptic plane. This shift in inclination \u2014 17 degrees to be exact \u2014 allowed its cameras to view the Sun\u2019s south pole for the first time.<\/p>\n<\/p>\n<p><iframe title=\"Solar Orbiter zooms into the Sun\u2019s south pole\" src=\"https:\/\/www.youtube.com\/embed\/TU4DcDgaMM0?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen=\"\" name=\"fitvid0\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\"><\/iframe><\/p>\n<p>\u201cThe Sun is our nearest star, giver of life and potential disruptor of modern space and ground power systems, so it is imperative that we understand how it works and learn to predict its behaviour. These new, unique views from our Solar Orbiter mission are the beginning of a new era of solar science,\u201d said Prof. Carole Mundell, who serves as the Director of Science for the European Space Agency (ESA).<\/p>\n<h4 class=\"widget-title penci-border-arrow\">See Also<\/h4>\n<ul>\n<li>Solar Orbiter Updates<\/li>\n<li>Space Science Coverage<\/li>\n<li>NSF Shop<\/li>\n<li>Click Here to Join L2<\/li>\n<\/ul>\n<p>Solar Orbiter first got a glimpse of the south pole on March 16 when it was 15 degrees below the solar equator. Throughout the following day, the spacecraft imaged the south pole through a variety of filters as part of the mission\u2019s first high-angle observation campaign, which continued until Solar Orbiter reached its maximum orbital inclination of 17 degrees.<\/p>\n<p>The spacecraft used three of its instruments to capture the images and measurements. The Polarimetric and Helioseismic Imager (PHI) provides high-resolution and full-disk measurements of the Sun\u2019s photosphere\u2019s vector magnetic field. The Extreme Violet Imager (EUI) provides imagery of the atmospheric layers of the photosphere, or the layer of a star\u2019s outer atmosphere from which light is radiated. Lastly, the Spectral Imaging of the Coronal Environment (SPICE) instrument collects extreme ultraviolet imagery and spectroscopic measurements of the plasma properties of the Sun\u2019s corona.<\/p>\n<p>Space Shuttle models<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>Rocket building kits<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>NASA mission patches<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>\n<p>     (adsbygoogle = window.adsbygoogle || []).push({});<\/p>\n<p>\u201cWe didn\u2019t know what exactly to expect from these first observations \u2014 the Sun\u2019s poles are literally terra incognita,\u201d says PHI instrument team lead Prof. Sami Solanki of the Max Planck Institute for Solar System Research in Germany.<\/p>\n<p><img fetchpriority=\"high\" decoding=\"async\" aria-describedby=\"caption-attachment-107219\" class=\"size-full wp-image-107219\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/Solar_Orbiter_s_instruments-scaled.jpg\" alt=\"\" width=\"2560\" height=\"1440\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/Solar_Orbiter_s_instruments-scaled.jpg 2560w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/Solar_Orbiter_s_instruments-350x197.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/Solar_Orbiter_s_instruments-622x350.jpg 622w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/Solar_Orbiter_s_instruments-768x432.jpg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/Solar_Orbiter_s_instruments-1920x1080.jpg 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/Solar_Orbiter_s_instruments-1170x658.jpg 1170w\" sizes=\"(max-width: 2560px) 100vw, 2560px\"><\/p>\n<p id=\"caption-attachment-107219\" class=\"wp-caption-text\">Diagram showing Solar Orbiter\u2019s suite of instruments. (Credit: ESA)<\/p>\n<p>For the first high-angle observation program, PHI imaged the Sun in visible light and mapped its surface magnetic field, EUI imaged the Sun in ultraviolet light and its corona, and SPICE imaged light radiating from charged gas of varying temperatures above the Sun\u2019s surface.<\/p>\n<p>The observations made by the three instruments highlighted how material moves within the Sun\u2019s outer layers and could reveal polar vortices similar to those seen at Saturn\u2019s poles. Furthermore, observing the Sun\u2019s polar regions will reveal more about the Sun\u2019s intense magnetic field and why it flips every 11 years. Solar activity usually peaks when this magnetic field flips, but current models struggle to predict exactly when the Sun will reach its most active state and how powerful its peak will be.<\/p>\n<p>One such discovery made regarding the Sun\u2019s magnetic field is that, at the solar south pole, the Sun\u2019s magnetic field is quite a mess. Measurements from PHI showed that both north and south polarity magnetic fields are present at the south pole. Normally, planetary poles will feature one of the two polarities, not both.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-107220\" class=\"size-full wp-image-107220\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole.png\" alt=\"\" width=\"2657\" height=\"1500\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole.png 2657w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole-350x198.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole-620x350.png 620w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole-768x434.png 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole-1920x1084.png 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/PHI_sees_mixed-up_magnetism_at_the_Sun_s_south_pole-1170x661.png 1170w\" sizes=\"(max-width: 2657px) 100vw, 2657px\"><\/p>\n<p id=\"caption-attachment-107220\" class=\"wp-caption-text\">PHI data showing the \u201cmessy\u201d magnetic field at the solar south pole. Each red and blue patch indicated a different magnetic polarity. (Credit: ESA\/NASA\/Solar Orbiter\/PHI Team\/J. Hirzberger (MPS))<\/p>\n<p>Interestingly, however, this \u201cmess\u201d only briefly occurs during a solar maximum, when the Sun\u2019s magnetic field flips and is at its most active state. Given that the Sun reached its most recent solar maximum in October 2024 and will continue to stay highly active until September or October, the observations were not unexpected. After the magnetic field flips and the Sun\u2019s activity begins to die down, a single polarity will build up and take over at each of the Sun\u2019s poles. The magnetic field will reach its most orderly state in five to six years, when the Sun reaches its solar minimum.<\/p>\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 Solanki said.<\/p>\n<p>PHI\u2019s observations and mapping of the Sun\u2019s magnetic field further highlighted the complexity of the magnetic field at solar maximum. The strongest magnetic fields were identified in two large bands on either side of the Sun\u2019s equator. Furthermore, multiple \u201csunspots\u201d were noted in the PHI data, or regions where the magnetic field is heavily concentrated on the Sun\u2019s surface.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-107221\" class=\"size-full wp-image-107221\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/PHI_s_pole-to-pole_view_of_the_Sun_s_magnetic_field.gif\" alt=\"\" width=\"800\" height=\"800\"><\/p>\n<p id=\"caption-attachment-107221\" class=\"wp-caption-text\">PHI\u2019s complete map of the Sun\u2019s magnetic field. The darker the shade of red or blue, the stronger the magnetic field. (Credit: ESA\/NASA\/Solar Orbiter\/PHI Team\/J. Hirzberger (MPS))<\/p>\n<p>While PHI mapped the Sun\u2019s magnetic field, SPICE was busy measuring the spectral lines emitted by chemical elements \u2014 such as hydrogen, carbon, and oxygen \u2014 within the solar surface, revealing what happens in different atmospheric layers above the Sun\u2019s surface. What\u2019s more, the SPICE team successfully performed a \u201cDoppler measurement\u201d with the instrument for the first time, during which SPICE precisely tracked spectral lines to measure the velocities of clumps of solar material.<\/p>\n<p>The team performed multiple Doppler measurements during the first high-angle observations, creating a velocity map that revealed how solar material moves at different layers of the Sun\u2019s atmosphere.<\/p>\n<p>These measurements can reveal how solar material is ejected from the Sun during coronal mass ejections and other solar events. The ejected solar material, then known as \u201csolar wind,\u201d is responsible for the incredible aurora light shows we see on Earth, Jupiter, Mars, and many other planets. Investigating the origins of solar wind is one of Solar Orbiter\u2019s key scientific objectives, and the latest polar observations are just the first of many that will reveal more about solar wind and how it is created.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-107222\" class=\"size-full wp-image-107222\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/SPICE_sees_movement_at_the_Sun_s_south_pole.png\" alt=\"\" width=\"2310\" height=\"1299\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/SPICE_sees_movement_at_the_Sun_s_south_pole.png 2310w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/SPICE_sees_movement_at_the_Sun_s_south_pole-350x197.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/SPICE_sees_movement_at_the_Sun_s_south_pole-622x350.png 622w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/SPICE_sees_movement_at_the_Sun_s_south_pole-768x432.png 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/SPICE_sees_movement_at_the_Sun_s_south_pole-1920x1080.png 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2025\/06\/SPICE_sees_movement_at_the_Sun_s_south_pole-1170x658.png 1170w\" sizes=\"(max-width: 2310px) 100vw, 2310px\"><\/p>\n<p id=\"caption-attachment-107222\" class=\"wp-caption-text\">SPICE\u2019s velocity map of the Sun\u2019s south pole. The red and blue colors represent the different motions of material, with red highlighting material moving away from Solar Orbiter. (Credit: ESA\/NASA\/Solar Orbiter\/SPICE Team\/M. Janvier (ESA)\/J. Plowman (SwRI))<\/p>\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 of the University of Paris-Saclay in France.<\/p>\n<p>All of these findings stem from Solar Orbiter\u2019s first pass in its newly inclined orbit. As its orbital inclination continues to increase, so will the spacecraft\u2019s visibility of the poles and its ability to research them. In fact, much of the data collected from the first passes has yet to be analyzed. Though Solar Orbiter has already completed its first full \u201cpole-to-pole\u201d flight, the complete data set of that is expected to arrive in October.<\/p>\n<p>\u201cThis is just the first step of Solar Orbiter\u2019s \u2018stairway to heaven\u2019: in the coming years, the spacecraft will climb further out of the ecliptic plane for ever better views of the Sun\u2019s polar regions. These data will transform our understanding of the Sun\u2019s magnetic field, the solar wind, and solar activity,\u201d said Solar Orbiter project scientist Daniel M\u00fcller.<\/p>\n<p><em>(Lead image: Solar Orbiter image of the Sun\u2019s south pole. Credit: ESA\/NASA\/Solar Orbiter\/EUI Team\/D. Berghmans (ROB))<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Following a flyby of Venus in February that successfully increased its orbital inclination around the Sun, the European Space Agency\u2019s Solar Orbiter recently imaged the Sun\u2019s poles for the first time. The images are the first to show how the Sun\u2019s immense magnetic field interacts at its poles, and will improve scientists\u2019 understanding of the [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[2],"tags":[3664,1238,246,190,8098,8099,4813,2169,2311,8100,2170],"class_list":["post-23799","post","type-post","status-publish","format-standard","hentry","category-news","tag-aurora","tag-corona","tag-esa","tag-nasa","tag-polar","tag-pole","tag-solar","tag-solar-orbiter","tag-solar-wind","tag-south-pole","tag-sun"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/23799"}],"collection":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/comments?post=23799"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/23799\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=23799"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=23799"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=23799"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}