{"id":2158,"date":"2025-02-21T23:49:22","date_gmt":"2025-02-21T23:49:22","guid":{"rendered":"https:\/\/aurorasaurudev.wpengine.com\/?p=2158"},"modified":"2025-02-21T23:53:44","modified_gmt":"2025-02-21T23:53:44","slug":"what-is-an-auroral-substorm","status":"publish","type":"post","link":"https:\/\/blog.aurorasaurus.org\/?p=2158","title":{"rendered":"What is an auroral substorm?"},"content":{"rendered":"<p><span style=\"font-weight: 400;\">Guest post by Vincent Ledvina, Laura Edson<\/span><\/p>\n<p><i><span style=\"font-weight: 400;\">With thanks to Valerie Svaldi for additional input<\/span><\/i><\/p>\n<p><span style=\"font-weight: 400;\">One of the <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=1555\"><span style=\"font-weight: 400;\">terms<\/span><\/a><span style=\"font-weight: 400;\"> you\u2019ll often aurora chasers and scientists use is \u201csubstorm.\u201d You might hear it referring to the best parts of an aurora chase, or as something to patiently wait for. But what does it mean, and where does it come from? While the aurora is commonly depicted in film and photos as erupting into color and motion, it doesn\u2019t dance that way continuously all night. Instead, the aurora has a natural progression called a \u201csubstorm\u201d, a sort of\u00a0 \u201clife cycle\u201d every few hours that happens multiple times a day. Substorms vary drastically due to the ever-changing energy from the Sun that drives them, but scientists look for telltale signatures in visible aurora and other data; there is a standard rhythm to their dance. In this blog post, we\u2019ll walk through the basic steps. Note that this post is about daily auroras at northern high latitudes like Fairbanks, Yellowknife, Churchill, Troms\u00f8, Abisko, and Kiruna, and does <\/span><b>not <\/b><span style=\"font-weight: 400;\">include the larger geomagnetic storms that cause more widespread, irregular displays. We will also primarily be covering the perspective of being underneath the lights at these high latitudes, rather than viewing them more from the side hundreds of miles further from the poles.\u00a0<\/span><\/p>\n<p><center><iframe loading=\"lazy\" title=\"YouTube video player\" src=\"https:\/\/www.youtube.com\/embed\/OSWLRLaTXpk?si=yxcYdiZqXbmgMW_S\" width=\"560\" height=\"315\" frameborder=\"0\" allowfullscreen=\"allowfullscreen\"><\/iframe><\/center><span style=\"font-weight: 400;\">In the above video, you can see how matter and magnetism from the Sun, the \u201csolar wind,\u201d energize the Earth\u2019s magnetic field. This energy is stored on the night side of the planet (the side away from the sun) in the \u201cmagnetotail,\u201d where the flow of the solar wind stretches out the magnetic field. Substorms happen when energy stored in the magnetotail is suddenly <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.youtube.com\/watch?v=-PvE-ACxn1w\"><span style=\"font-weight: 400;\">released toward the Earth\u2019s poles<\/span><\/a><span style=\"font-weight: 400;\"> via magnetic reconnection. Substorms are normal, everyday phenomena that repeat multiple times per day as this huge storage and release system naturally does its job. They vary greatly but experienced aurora chasers know their signature rhythms.\u00a0<\/span><\/p>\n<h2><span style=\"font-weight: 400;\">Growth Phase | Hours | Growing, discrete arcs<\/span><\/h2>\n<figure id=\"attachment_2162\" aria-describedby=\"caption-attachment-2162\" style=\"width: 814px\" class=\"wp-caption aligncenter\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-183256.png\"><img loading=\"lazy\" decoding=\"async\" class=\" wp-image-2162\" src=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-183256.png\" alt=\"An only slightly wavy lone stripe of green aurora stretches across the sky like a celestial snake\" width=\"814\" height=\"543\" srcset=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-183256.png 1070w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-183256-300x200.png 300w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-183256-1024x683.png 1024w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-183256-768x512.png 768w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-183256-930x620.png 930w\" sizes=\"auto, (max-width: 814px) 100vw, 814px\" \/><\/a><figcaption id=\"caption-attachment-2162\" class=\"wp-caption-text\">Photo of the growth phase of a substorm by Vincent Ledvina. The photo was taken taken on March 3, 2023, 22:47 AKST from Poker Flat Research Range.<\/figcaption><\/figure>\n<p><span style=\"font-weight: 400;\">In the evening hours local time, an observer on the ground before midnight would notice quiet, ribbonlike <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=1877\"><span style=\"font-weight: 400;\">discrete<\/span><\/a><span style=\"font-weight: 400;\"> auroral arcs without much motion within the structures: the growth phase of a substorm. The arcs gradually move toward the equator: this follows the movement of the overall <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=1555#oval\"><span style=\"font-weight: 400;\">auroral oval<\/span><\/a><span style=\"font-weight: 400;\">. At the same time, out in space the magnetotail is stretching out more and more. Similar to a rubber band, as the magnetic field lines in the magnetotail stretch, they become more tense. This can last a few hours, so it\u2019s good to be patient and wait for these discrete arcs to start growing before you get out into the cold. Locals will recognize the quiet growth phase arc as a regular early evening appearance to the north or northeast.\u00a0<\/span><\/p>\n<h2><span style=\"font-weight: 400;\">Onset or Breakup Phase | 10-15 minutes | Auroral beads may appear<\/span><\/h2>\n<figure id=\"attachment_2160\" aria-describedby=\"caption-attachment-2160\" style=\"width: 894px\" class=\"wp-caption aligncenter\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182235.png\"><img loading=\"lazy\" decoding=\"async\" class=\" wp-image-2160\" src=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182235.png\" alt=\"A series of six aurora photos shows auroral beads forming in the second and third photo, one minute apart\" width=\"894\" height=\"446\" srcset=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182235.png 1237w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182235-300x150.png 300w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182235-1024x511.png 1024w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182235-768x383.png 768w\" sizes=\"auto, (max-width: 894px) 100vw, 894px\" \/><\/a><figcaption id=\"caption-attachment-2160\" class=\"wp-caption-text\">Formation of auroral beads over time. Photos by Vincent Ledvina, taken on January 13, 2023, five miles from Seljalandsfoss, Iceland at around 10:52 pm local time. Note that the beads form in a more southerly arc (to the left in this photo).<\/figcaption><\/figure>\n<figure id=\"attachment_2161\" aria-describedby=\"caption-attachment-2161\" style=\"width: 165px\" class=\"wp-caption alignright\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182815.png\"><img loading=\"lazy\" decoding=\"async\" class=\" wp-image-2161\" src=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182815.png\" alt=\"A bar magnet, oriented vertically, is surrounded with iron filings that take the shape of &quot;butterfly wings&quot; from pole to pole.\" width=\"165\" height=\"224\" srcset=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182815.png 364w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-182815-221x300.png 221w\" sizes=\"auto, (max-width: 165px) 100vw, 165px\" \/><\/a><figcaption id=\"caption-attachment-2161\" class=\"wp-caption-text\">Dipole magnet with iron filings showing the magnetic field. Image from NASA Space Math.<\/figcaption><\/figure>\n<p><span style=\"font-weight: 400;\">As quiet arcs get more active and start to cover more of the sky, the next big things to look for are <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=398\"><span style=\"font-weight: 400;\">auroral beads<\/span><\/a><span style=\"font-weight: 400;\">: a row of brighter spots or stripes in line along an auroral arc. They usually only last seconds to minutes, so auroral beads are a signal to pay close attention to what happens next! Beads are rare, and if the substorm breakup is happening significantly east or west of your location, you might not see them.\u00a0<\/span><\/p>\n<p><span style=\"font-weight: 400;\">Auroral beads are a signature of the \u201conset\u201d of a substorm, also called the \u201cbreakup\u201d because the arcs will break up all over the sky. Previously quiet auroral arcs can suddenly twist into many dynamic forms. At this time, the aurora dramatically shifts from the equatorward part of the sky and snaps back towards the nearest magnetic pole (the North or South Pole). In the northern hemisphere it is common to see auroras move from the southern to northern horizon in a matter of ten minutes or so. It\u2019s a stunning sight! Scientists have debated for at least half a century about how exactly the energy release that triggers the breakup gets started. However, we do know that in space, the magnetotail moves toward the Earth, becoming less and less stretched out and more closely resembling the shape of a dipole bar magnet\u2019s magnetic field: hence, this effect is called \u201cdipolarization.\u201d\u00a0<\/span><\/p>\n<h2><span style=\"font-weight: 400;\">Expansion Phase | 15-30 minutes | Bursting into motion and bright color<\/span><\/h2>\n<figure id=\"attachment_2165\" aria-describedby=\"caption-attachment-2165\" style=\"width: 868px\" class=\"wp-caption aligncenter\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/March-5-2022-2-am-AKST-Fort-Yukon-Alaska-facing-east-scaled.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\" wp-image-2165\" src=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/March-5-2022-2-am-AKST-Fort-Yukon-Alaska-facing-east-scaled.jpg\" alt=\"Glowing green over a snowy landscape, aurora takes up half the sky in curling patterns like wood grain\" width=\"868\" height=\"579\" srcset=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/March-5-2022-2-am-AKST-Fort-Yukon-Alaska-facing-east-scaled.jpg 2560w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/March-5-2022-2-am-AKST-Fort-Yukon-Alaska-facing-east-300x200.jpg 300w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/March-5-2022-2-am-AKST-Fort-Yukon-Alaska-facing-east-1024x683.jpg 1024w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/March-5-2022-2-am-AKST-Fort-Yukon-Alaska-facing-east-768x512.jpg 768w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/March-5-2022-2-am-AKST-Fort-Yukon-Alaska-facing-east-1536x1024.jpg 1536w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/March-5-2022-2-am-AKST-Fort-Yukon-Alaska-facing-east-2048x1365.jpg 2048w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/March-5-2022-2-am-AKST-Fort-Yukon-Alaska-facing-east-930x620.jpg 930w\" sizes=\"auto, (max-width: 868px) 100vw, 868px\" \/><\/a><figcaption id=\"caption-attachment-2165\" class=\"wp-caption-text\">Photo of the expansion phase of a substorm by Vincent Ledvina, taken March 5, 2022, 2 am AKST, Fort Yukon, Alaska, facing east.<\/figcaption><\/figure>\n<p><span style=\"font-weight: 400;\">The expansion phase is the most famous part of the aurora\u2019s dance. There is usually at least one per night at high latitudes, usually occurring around magnetic midnight. It usually lasts about 15-30 minutes and can include spectacular ribbonlike shapes, bright colors, and active movements.\u00a0<\/span><\/p>\n<p><span style=\"font-weight: 400;\">Behind the scenes: the aurora occurs in ovals around Earth\u2019s geomagnetic poles. If you are underneath the <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=1555#oval\"><span style=\"font-weight: 400;\">auroral oval<\/span><\/a><span style=\"font-weight: 400;\"> at its strongest point, you\u2019ll look up and see the aurora dancing above you. Imagine a substorm like dropping a large rock into a pond: the auroral oval becomes energized in a certain spot, and then that energy spreads around the world to the east and west. If you are right under this energized spot, you will see beads form right above you and the aurora \u201cexplode\u201d overhead, but if you are under the auroral oval hundreds of miles away from the energized spot, you may see aurora racing toward you from the eastern or western horizon: a \u201cwestward-traveling surge\u201d. This is like feeling the waves from the splash from far away.\u00a0<\/span><\/p>\n<p><span style=\"font-weight: 400;\">Sometimes during the auroral substorm expansion phase, a large spiral of aurora forms, and moves westward, it can even be visible from space. Along with spirals, you may see vortex structures like smaller-scale \u201cfolds,\u201d and \u201c<\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=1877\"><span style=\"font-weight: 400;\">curls<\/span><\/a><span style=\"font-weight: 400;\">,\u201d which wind the opposite direction from spirals.<\/span><\/p>\n<figure id=\"attachment_2163\" aria-describedby=\"caption-attachment-2163\" style=\"width: 882px\" class=\"wp-caption aligncenter\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Sep-29-2022-11_38-pm-CDT-Churchill-MB-facing-west.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\" wp-image-2163\" src=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Sep-29-2022-11_38-pm-CDT-Churchill-MB-facing-west.jpg\" alt=\"Over a lake with a red boat docked, above tiny scattered clouds, a cinnamon roll-like aurora swirls, twirling into a second one in the distance\" width=\"882\" height=\"627\" srcset=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Sep-29-2022-11_38-pm-CDT-Churchill-MB-facing-west.jpg 7867w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Sep-29-2022-11_38-pm-CDT-Churchill-MB-facing-west-300x213.jpg 300w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Sep-29-2022-11_38-pm-CDT-Churchill-MB-facing-west-1024x729.jpg 1024w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Sep-29-2022-11_38-pm-CDT-Churchill-MB-facing-west-768x546.jpg 768w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Sep-29-2022-11_38-pm-CDT-Churchill-MB-facing-west-1536x1093.jpg 1536w\" sizes=\"auto, (max-width: 882px) 100vw, 882px\" \/><\/a><figcaption id=\"caption-attachment-2163\" class=\"wp-caption-text\">Photo of spirals during the expansion phase of a substorm by Vincent Ledvina, taken Sep 29, 2022, 11:38 pm CDT, Churchill, MB, facing west.<\/figcaption><\/figure>\n<h2><span style=\"font-weight: 400;\">Recovery Phase | 1+ hours | Quiet, with pulsating patches<\/span><\/h2>\n<figure id=\"attachment_2164\" aria-describedby=\"caption-attachment-2164\" style=\"width: 891px\" class=\"wp-caption aligncenter\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Jan-18-2023-2_42-am-AKST-Fairbanks-Alaska-facing-east-scaled.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\" wp-image-2164\" src=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Jan-18-2023-2_42-am-AKST-Fairbanks-Alaska-facing-east-scaled.jpg\" alt=\"Over a snowy landscape with fir trees in the distance, patchy, shredded aurora fills the middle of the sky\" width=\"891\" height=\"594\" srcset=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Jan-18-2023-2_42-am-AKST-Fairbanks-Alaska-facing-east-scaled.jpg 2560w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Jan-18-2023-2_42-am-AKST-Fairbanks-Alaska-facing-east-300x200.jpg 300w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Jan-18-2023-2_42-am-AKST-Fairbanks-Alaska-facing-east-1024x683.jpg 1024w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Jan-18-2023-2_42-am-AKST-Fairbanks-Alaska-facing-east-768x512.jpg 768w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Jan-18-2023-2_42-am-AKST-Fairbanks-Alaska-facing-east-1536x1024.jpg 1536w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Jan-18-2023-2_42-am-AKST-Fairbanks-Alaska-facing-east-2048x1365.jpg 2048w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Jan-18-2023-2_42-am-AKST-Fairbanks-Alaska-facing-east-930x620.jpg 930w\" sizes=\"auto, (max-width: 891px) 100vw, 891px\" \/><\/a><figcaption id=\"caption-attachment-2164\" class=\"wp-caption-text\">Photo of the recovery phase of a substorm by Vincent Ledvina, taken Jan 18, 2023, 2:42 am AKST, Fairbanks, Alaska, facing east.<\/figcaption><\/figure>\n<p><span style=\"font-weight: 400;\">This part of the dance can last one or more hours. The aurora becomes diffuse and cloudlike, <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.aurorasaurus.org\/learn#common-shapes\"><span style=\"font-weight: 400;\">usually<\/span><\/a><span style=\"font-weight: 400;\"> dim with much slower motion. (But if you can see stars through the glow, then it is likely an aurora, not a cloud.) That said, it is <\/span><span style=\"font-weight: 400;\">often the time of <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=1792\"><span style=\"font-weight: 400;\">pulsating patches<\/span><\/a><span style=\"font-weight: 400;\">, parts of the aurora that seem to <\/span><span style=\"font-weight: 400;\">turn on and off every few seconds and occupy <\/span><span style=\"font-weight: 400;\">the \u201cequatorward\u201d side of the main auroral oval<\/span><span style=\"font-weight: 400;\">. These tend to occur closer to morning, as the Earth rotates underneath the aurora. <\/span><span style=\"font-weight: 400;\">Sometimes the recovery phase marks the finale of a night of an aurora, but sometimes another substorm happens right afterward, especially on active nights. It\u2019s easy to underestimate how long this recovery process takes: be patient when waiting for another substorm.\u00a0<\/span><\/p>\n<h2><span style=\"font-weight: 400;\">A\u00a0 mid-latitude perspective shows height and motion<\/span><\/h2>\n<p><span style=\"font-weight: 400;\">If you are further toward the equator when a substorm onset occurs, the biggest difference is that you will be <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2022\/05\/Chenille-Stem-Aurora-Perspective-Viewer.pdf\"><span style=\"font-weight: 400;\">looking at the aurora sideways<\/span><\/a><span style=\"font-weight: 400;\"> rather than from underneath, and the translucent arcs seem to layer over one another. From far away you can\u2019t see the north-south motions of the arcs very easily, but you can tell when the activity picks up.\u00a0<\/span><\/p>\n<figure id=\"attachment_2166\" aria-describedby=\"caption-attachment-2166\" style=\"width: 1852px\" class=\"wp-caption alignnone\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-185043.png\"><img loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-2166\" src=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-185043.png\" alt=\"Three photos show the stages of a curtainlike substorm from the side: the first fainter and fuzzy, the second bright and stripey, and the third messy and patchy\" width=\"1852\" height=\"412\" srcset=\"https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-185043.png 1852w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-185043-300x67.png 300w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-185043-1024x228.png 1024w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-185043-768x171.png 768w, https:\/\/blog.aurorasaurus.org\/wp-content\/uploads\/2025\/02\/Screenshot-2025-02-21-185043-1536x342.png 1536w\" sizes=\"auto, (max-width: 1852px) 100vw, 1852px\" \/><\/a><figcaption id=\"caption-attachment-2166\" class=\"wp-caption-text\">Photos by Christian Harris, Sept 29, 2024. Each represents a substorm phase\u2014Growth, Expansion, and Recovery, respectively\u2014from a mid-latitude location at Tofte Lake, MN.<\/figcaption><\/figure>\n<p><span style=\"font-weight: 400;\">For example, at the start of the breakup phase, auroral beads may appear as bright shifting and dancing pillars on the horizon. Poleward expansion may move away from you, but since from a distance all the auroral arcs are layered, the display can become quite bright! It may look more like curtains waving on the horizon. The substorm follows the same steps, though, even if you are looking at it from a different angle.\u00a0<\/span><\/p>\n<h2><span style=\"font-weight: 400;\">What do substorms mean for Earth?<\/span><\/h2>\n<p><span style=\"font-weight: 400;\">Substorms are important to study because they are not only a fundamental process by which energy moves through our planet\u2019s magnetic fields and into the atmosphere, but they can affect technology in space like <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/agupubs.onlinelibrary.wiley.com\/doi\/full\/10.1029\/2010SW000588\"><span style=\"font-weight: 400;\">satellites<\/span><\/a><span style=\"font-weight: 400;\">, and on the ground: for example, <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.youtube.com\/watch?v=3oQ2bXgkVtk\"><span style=\"font-weight: 400;\">large power grids<\/span><\/a><span style=\"font-weight: 400;\">. This normal, daily dance between the Earth and Sun is important to understand for advancing and engineering technology.\u00a0<\/span><\/p>\n<p><span style=\"font-weight: 400;\">That said, substorms are tricky to fully understand because the processes in the Earth\u2019s magnetic field that cause them are so large; while they are basic <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/science.nasa.gov\/heliophysics\/\"><span style=\"font-weight: 400;\">heliophysics<\/span><\/a><span style=\"font-weight: 400;\"> processes, the way they \u201cbreakup\u201d is still <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.frontiersin.org\/journals\/astronomy-and-space-sciences\/articles\/10.3389\/fspas.2023.1296626\/full\"><span style=\"font-weight: 400;\">hotly<\/span><\/a> <a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.nature.com\/articles\/s41561-023-01206-2\"><span style=\"font-weight: 400;\">debated<\/span><\/a><span style=\"font-weight: 400;\"> because of this. Observers on the ground can provide key clues that might help unlock what a satellite is measuring far out in space. This blog post is just an introduction to substorms, and you can learn more from the resource list below. You can also help scientists study them! When you make a report to Aurorasaurus, you can include the exact start time of the different substorm phases if you notice it, even from mid-latitudes. In particular, we\u2019d like to know the time of \u201cbreakup\u201d and if you see any distinct, short-lived auroral beads. Special catalogs of substorms are used in this kind of research, so doing so will help scientists match your observation with other data.\u00a0<\/span><\/p>\n<h2><span style=\"font-weight: 400;\">Getting to know substorms<\/span><\/h2>\n<p><span style=\"font-weight: 400;\">Substorms were originally <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.ss.ncu.edu.tw\/~lyu\/lecture_files_en\/Lyu_Aurora\/Ref_Papers_AuroraSubstorm\/Akasofu_1964.pdf\"><span style=\"font-weight: 400;\">defined by Dr. Syun-Ichi Akasofu<\/span><\/a><span style=\"font-weight: 400;\"> as \u201cthe sequence of auroral events over the entire polar region during the passage from auroral quiet through the various active phases to subsequent calm.\u201d In other words, a sort of \u201c<\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.youtube.com\/watch?v=iENJ8-fZ6lI&amp;list=PL6bJMVfHeH05r5s5UBFs8d99ofpGcnSGc&amp;index=3\"><span style=\"font-weight: 400;\">life cycle<\/span><\/a><span style=\"font-weight: 400;\">\u201d of aurora. In this cycle, the onset and expansion phase usually contain the best and most active auroras, but between those peaks the aurora will die down for a while. Learning to recognize the stages of a substorm will help you get a sense for when the aurora might become active again\u2014and when you can see less-noticed but still cool features like pulsating patches!<\/span><\/p>\n<p><center><iframe loading=\"lazy\" title=\"YouTube video player\" src=\"https:\/\/www.youtube.com\/embed\/Jrm59KbTCEo?si=EVPgoVCrEOHcrDza\" width=\"560\" height=\"315\" frameborder=\"0\" allowfullscreen=\"allowfullscreen\"><\/iframe><\/center><span style=\"font-weight: 400;\">This video shows some fairly canonical substorms: be sure to click in and read the detailed description on YouTube. In this image from a University of Alaska Fairbanks allsky camera, North is at the bottom, East is to the right, South is at the top, and West is to the left.\u00a0<\/span><\/p>\n<h2><span style=\"font-weight: 400;\">Resources<\/span><\/h2>\n<ul>\n<li style=\"font-weight: 400;\" aria-level=\"1\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.ss.ncu.edu.tw\/~lyu\/lecture_files_en\/Lyu_Aurora\/Ref_Papers_AuroraSubstorm\/Akasofu_1964.pdf\"><span style=\"font-weight: 400;\">The Development of the Auroral Substorm<\/span><\/a><span style=\"font-weight: 400;\">, by Dr. Syun-Ichi Akasofu<\/span>\n<ul>\n<li style=\"font-weight: 400;\" aria-level=\"2\"><span style=\"font-weight: 400;\">The OG substorm paper, this goes over the details of substorm formation and progression. Aurorasaurus held a <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.youtube.com\/watch?v=iENJ8-fZ6lI&amp;list=PL6bJMVfHeH05r5s5UBFs8d99ofpGcnSGc&amp;index=3\"><span style=\"font-weight: 400;\">Journal Club<\/span><\/a><span style=\"font-weight: 400;\"> read-together of the article.\u00a0<\/span><\/li>\n<\/ul>\n<\/li>\n<li style=\"font-weight: 400;\" aria-level=\"1\"><span style=\"font-weight: 400;\">\u201c<\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/theauroraguy.com\/blogs\/blog\/what-is-an-auroral-substorm\"><span style=\"font-weight: 400;\">What is an auroral substorm<\/span><\/a><span style=\"font-weight: 400;\">?\u201d a new blog post by Vincent Ledvina<\/span><\/li>\n<li style=\"font-weight: 400;\" aria-level=\"1\"><span style=\"font-weight: 400;\">Space Weather Unplugged <\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.youtube.com\/watch?v=QaDnJDOkvVs\"><span style=\"font-weight: 400;\">episode<\/span><\/a><span style=\"font-weight: 400;\">: \u201cChasing a Substorm\u201d<\/span><\/li>\n<li style=\"font-weight: 400;\" aria-level=\"1\"><span style=\"font-weight: 400;\">\u201c<\/span><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/www.glendaleskye.com\/aurora-phases.php\/1000\"><span style=\"font-weight: 400;\">The Lifecycle of an Aurora<\/span><\/a><span style=\"font-weight: 400;\">\u201d by Andy Stables<\/span><\/li>\n<li style=\"font-weight: 400;\" aria-level=\"1\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=1877\"><span style=\"font-weight: 400;\">What Is Discrete Aurora? (It\u2019s Not Discreet!)<\/span><\/a><span style=\"font-weight: 400;\"> blog post by Aurorasaurus<\/span><\/li>\n<li style=\"font-weight: 400;\" aria-level=\"1\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=398\"><span style=\"font-weight: 400;\">Which processes in space cause these mysterious auroral beads?<\/span><\/a><span style=\"font-weight: 400;\"> Aurorasaurus guest blog post by Nadine Kalmoni<\/span><\/li>\n<li style=\"font-weight: 400;\" aria-level=\"1\"><a target=\"_blank\" rel=\"noopener noreferrer\" href=\"https:\/\/blog.aurorasaurus.org\/?p=1792\"><span style=\"font-weight: 400;\">Like an Outdoor Nightclub: Q&amp;A on Pulsating Auroras<\/span><\/a><span style=\"font-weight: 400;\"> blog post by Aurorasaurus<\/span><\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>Guest post by Vincent Ledvina, Laura Edson With thanks to Valerie Svaldi for additional input One of the terms you\u2019ll often aurora chasers and scientists use is \u201csubstorm.\u201d You might hear it referring to the best parts of an aurora chase, or as something to patiently wait for. But what does it mean, and where&hellip;&nbsp;<a href=\"https:\/\/blog.aurorasaurus.org\/?p=2158\" rel=\"bookmark\">Read More &raquo;<span class=\"screen-reader-text\">What is an auroral substorm?<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":2165,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"rop_custom_images_group":[],"rop_custom_messages_group":[],"rop_publish_now":"initial","rop_publish_now_accounts":[],"rop_publish_now_history":[],"rop_publish_now_status":"pending","neve_meta_sidebar":"","neve_meta_container":"","neve_meta_enable_content_width":"off","neve_meta_content_width":70,"neve_meta_title_alignment":"","neve_meta_author_avatar":"","neve_post_elements_order":"","neve_meta_disable_header":"","neve_meta_disable_footer":"","neve_meta_disable_title":"","footnotes":""},"categories":[7,17,12],"tags":[22,20,23,28],"class_list":["post-2158","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-education","category-other-resources-for-aurora-hunters","category-understanding-the-aurora","tag-arctic","tag-auroras","tag-northern-lights","tag-science"],"_links":{"self":[{"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=\/wp\/v2\/posts\/2158","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=2158"}],"version-history":[{"count":0,"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=\/wp\/v2\/posts\/2158\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=\/wp\/v2\/media\/2165"}],"wp:attachment":[{"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=2158"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=2158"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/blog.aurorasaurus.org\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=2158"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}