{"id":17483,"date":"2026-02-02T09:06:07","date_gmt":"2026-02-02T09:06:07","guid":{"rendered":"https:\/\/readtrends.com\/en\/space-weather-week-feb-1-7-2026\/"},"modified":"2026-02-02T09:06:07","modified_gmt":"2026-02-02T09:06:07","slug":"space-weather-week-feb-1-7-2026","status":"publish","type":"post","link":"https:\/\/readtrends.com\/en\/space-weather-week-feb-1-7-2026\/","title":{"rendered":"Space Weather Activity Story for the Week of 1-7 February, 2026 &#8211; NOAA (National Oceanic and Atmospheric Administration) (.gov)"},"content":{"rendered":"<article>\n<p><strong>Lead:<\/strong> NOAA reported on 1 February 2026 that active region RGN 4366 has developed into a complex sunspot group and produced solar flares in the M1\u2013X1 range during the week of Feb 1\u20137, 2026. Those flares correspond to radio blackout categories roughly R1\u2013R3 (Minor to Strong), but, as of the agency&#8217;s 18:43 UTC bulletin on Feb 1, there was no clear evidence of associated coronal mass ejections (CMEs) directed at Earth. Operational impacts so far are limited: NOAA notes weak or minor HF radio degradation on the sunlit side and brief low-frequency navigation degradation. Forecasters say the region remains the principal watch item for the coming days.<\/p>\n<h2>Key Takeaways<\/h2>\n<ul>\n<li>NOAA published the update on Sunday, February 01, 2026 at 18:43 UTC concerning RGN 4366 and the Feb 1\u20137 space weather outlook.<\/li>\n<li>RGN 4366 produced flares in the M1\u2013X1 range; these flare magnitudes map to radio blackout categories near R1\u2013R3 (Minor to Strong).<\/li>\n<li>As of the bulletin time, NOAA reported no clear evidence of CMEs associated with those flares \u2014 Earth-directed CME status remained unconfirmed.<\/li>\n<li>Observed operational effects included weak\/minor HF radio degradation on the sunlit side and brief degradation of low-frequency navigation signals.<\/li>\n<li>NOAA advised continued monitoring: RGN 4366 was identified as the region most likely to produce additional activity during the week of Feb 1\u20137, 2026.<\/li>\n<\/ul>\n<h2>Background<\/h2>\n<p>Active regions on the Sun are concentrations of magnetic flux that can generate solar flares and, occasionally, CMEs. Larger, magnetically complex sunspot groups are more likely to produce high-energy flares; RGN 4366\u2019s growth into a complex configuration increases the statistical probability of further energetic eruptions. The NOAA Space Weather Scales (R, S, G) are commonly used to translate solar output into operational categories for radio blackouts, radiation storms, and geomagnetic storms, respectively. Those scales help infrastructure operators\u2014satellite controllers, aviation planners, and power-grid managers\u2014assess and prepare for potential impacts.<\/p>\n<p>Solar flare classification (C, M, X) measures X-ray brightness; M-class flares are moderate while X-class are the most powerful. A flare\u2019s classification alone does not guarantee a damaging geomagnetic event at Earth\u2014an accompanying CME and its direction, magnetic orientation, and speed determine geomagnetic consequences. NOAA\u2019s routine bulletins combine remote-sensing observations (X-ray, EUV, and coronagraph imagery) with modelling to assess whether flares lead to Earth-directed CMEs and to produce watch or warning levels.<\/p>\n<h2>Main Event<\/h2>\n<p>RGN 4366 grew into a magnetically complex sunspot group in late January and early February 2026, according to NOAA\u2019s Feb 1 bulletin. During the initial reporting period it produced multiple flares assessed between M1 and X1 in peak X-ray flux. Those flare magnitudes correspond to potential radio blackout categories in the R1\u2013R3 range, which NOAA flagged as the likely radio-impact band for the period.<\/p>\n<p>Despite the flare activity, NOAA reported no clear coronagraph signature or other corroborating evidence of CMEs that would be unambiguously Earth-directed as of 18:43 UTC on Feb 1. The absence of a confirmed CME reduced the immediate risk of a geomagnetic storm (G-scale) at Earth, though forecasters emphasized that CMEs can be delayed or emerge after initial flares. Operational effects observed in the bulletin included weak or minor HF radio degradation on the sunlit side and short interruptions in low-frequency navigation signals.<\/p>\n<p>NOAA characterized RGN 4366 as the principal region to watch through Feb 7, 2026, noting that further flare activity is possible and that any future CME signatures would trigger rapid reassessment. Forecasters recommended users of HF communications, aviation polar routes, and precise navigation services maintain situational awareness and monitor NOAA updates. The agency pointed readers to its spaceweather.gov resources for near-real-time alerts and forecasts.<\/p>\n<h2>Analysis &#038; Implications<\/h2>\n<p>The immediate operational implication of M1\u2013X1 flares without confirmed CMEs is primarily in HF radio and short-duration navigation impacts rather than wide-scale geomagnetic storms. R1\u2013R3 radio blackouts can degrade high-frequency communications on the sunlit hemisphere, affecting aviation, maritime, and some military communications\u2014especially at higher latitudes. Because NOAA reported only weak or minor HF impacts so far, most ground-based systems and infrastructure are unlikely to experience severe disruptions in the short term.<\/p>\n<p>However, the situation remains dynamic. If future flares from RGN 4366 are followed by a fast, Earth-directed CME with a southward magnetic field component, that combination could elevate geomagnetic activity (G-scale) and pose stronger risks to power systems, satellite operations, and pipeline corrosion. Spacecraft operators and satellite fleets should therefore review mitigation plans for increased radiation or drag, and power-grid managers should be alert to geomagnetically induced current (GIC) risks if geomagnetic activity rises.<\/p>\n<p>For aviation, the main concern is increased radiation exposure on polar and high-altitude routes if an S-scale radiation storm develops; current NOAA guidance indicates no confirmed S-scale escalation. Navigation services using low-frequency transponders and some GNSS-dependent systems can experience brief degradations during R1\u2013R3 events, but those impacts are typically short-lived and localized to the sunlit hemisphere. The key operational recommendation is sustained monitoring\u2014forecasts can change rapidly if a delayed CME signature appears.<\/p>\n<h2>Comparison &#038; Data<\/h2>\n<figure>\n<table>\n<thead>\n<tr>\n<th>Metric<\/th>\n<th>Typical Range<\/th>\n<th>Operational Effect<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr>\n<td>Flare class<\/td>\n<td>M1\u2013X1<\/td>\n<td>Potential R1\u2013R3 radio blackouts; HF degradation<\/td>\n<\/tr>\n<tr>\n<td>Radio blackout (R-scale)<\/td>\n<td>R1\u2013R3<\/td>\n<td>Minor to Strong HF impacts on sunlit side<\/td>\n<\/tr>\n<tr>\n<td>Geomagnetic storm (G-scale)<\/td>\n<td>Not elevated (no confirmed CME)<\/td>\n<td>Low immediate geomagnetic risk<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<\/figure>\n<p>This table summarizes the bulletin\u2019s core data: the reported flare magnitudes and the corresponding operational categories NOAA associated with them, alongside the observed geomagnetic status at the time of the report. It clarifies why HF and navigation services were noted as the principal affected systems while larger geomagnetic impacts remained unlikely absent a confirmed CME.<\/p>\n<h2>Reactions &#038; Quotes<\/h2>\n<p>NOAA\u2019s public bulletin framed the situation as active but not yet escalated into a geomagnetic emergency. The agency urged continued monitoring and pointed users to operational products.<\/p>\n<blockquote>\n<p>&#8220;RGN 4366 has grown into a complex sunspot group&#8221;<\/p>\n<p><cite>NOAA Space Weather Prediction Center (official bulletin, Feb 1, 2026)<\/cite><\/p><\/blockquote>\n<blockquote>\n<p>&#8220;Stay space weather aware at spaceweather.gov&#8221;<\/p>\n<p><cite>NOAA Space Weather Prediction Center (official advisory)<\/cite><\/p><\/blockquote>\n<h2>\n<aside>\n<details>\n<summary>Explainer \/ Glossary<\/summary>\n<p>The NOAA Space Weather Scales: R (radio blackouts) measures X-ray flare impacts on HF communications; S (solar radiation storms) measures energetic particle fluxes that can affect satellites and aviation; G (geomagnetic storms) measures disturbances in Earth\u2019s magnetic field caused by CMEs. Flare classes\u2014C, M, X\u2014are based on peak 1\u20138 \u00c5 X-ray flux recorded by space-based sensors. A flare\u2019s classification does not alone predict geomagnetic storm strength; the presence, speed, direction, and magnetic orientation of a CME determine downstream geomagnetic effects. Operational users monitor both flare activity and coronagraph imagery to assess CME likelihood and potential Earth impacts.<\/p>\n<\/details>\n<\/aside>\n<\/h2>\n<h2>Unconfirmed<\/h2>\n<ul>\n<li>No CME was clearly identified in NOAA\u2019s Feb 1 bulletin; a delayed or faint CME associated with the reported flares cannot be ruled out without further coronagraph analysis.<\/li>\n<li>Whether any newly formed CME (if later detected) would be Earth-directed and possess a southward magnetic component\u2014key to strong geomagnetic storms\u2014remains unconfirmed.<\/li>\n<li>Forecasted escalation to higher R, S, or G categories during Feb 1\u20137 is possible but not yet supported by confirmed observational evidence at the time of the bulletin.<\/li>\n<\/ul>\n<h2>Bottom Line<\/h2>\n<p>RGN 4366 produced M1\u2013X1 class flares early in the week of Feb 1\u20137, 2026, creating a credible but not yet realized risk to HF communications and navigation. NOAA\u2019s bulletin (Feb 1, 2026, 18:43 UTC) emphasized the absence of confirmed CMEs at that time, which kept immediate geomagnetic risk low. Operational users\u2014especially HF communicators, aviation polar planners, satellite operators, and navigation-reliant services\u2014should remain vigilant: conditions can change quickly if a CME is later identified.<\/p>\n<p>For now, the practical expectation is localized, short-duration HF and navigation effects on the sunlit hemisphere rather than widespread geomagnetic disruption. Follow-up NOAA updates, coronagraph observations, and model runs will determine whether RGN 4366\u2019s activity translates into broader space weather impacts during the remainder of Feb 1\u20137, 2026.<\/p>\n<h2>Sources<\/h2>\n<ul>\n<li><a href=\"https:\/\/www.swpc.noaa.gov\/news\/space-weather-activity-story-week-1-7-february-2026\" target=\"_blank\" rel=\"noopener\">NOAA Space Weather Prediction Center: Space Weather Activity Story for the Week of 1-7 February, 2026<\/a> (official NOAA bulletin)<\/li>\n<li><a href=\"https:\/\/www.swpc.noaa.gov\/\" target=\"_blank\" rel=\"noopener\">NOAA Space Weather Prediction Center main site<\/a> (official agency resource and operational products)<\/li>\n<\/ul>\n<\/article>\n","protected":false},"excerpt":{"rendered":"<p>Lead: NOAA reported on 1 February 2026 that active region RGN 4366 has developed into a complex sunspot group and produced solar flares in the M1\u2013X1 range during the week of Feb 1\u20137, 2026. Those flares correspond to radio blackout categories roughly R1\u2013R3 (Minor to Strong), but, as of the agency&#8217;s 18:43 UTC bulletin on &#8230; <a title=\"Space Weather Activity Story for the Week of 1-7 February, 2026 &#8211; NOAA (National Oceanic and Atmospheric Administration) (.gov)\" class=\"read-more\" href=\"https:\/\/readtrends.com\/en\/space-weather-week-feb-1-7-2026\/\" aria-label=\"Read more about Space Weather Activity Story for the Week of 1-7 February, 2026 &#8211; NOAA (National Oceanic and Atmospheric Administration) (.gov)\">Read more<\/a><\/p>\n","protected":false},"author":1,"featured_media":17481,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"rank_math_title":"Space Weather Week Feb 1\u20137, 2026 \u2014 NOAA summary | DeepSpace Brief","rank_math_description":"NOAA reports sunspot region RGN 4366 produced M1\u2013X1 flares the week of Feb 1\u20137, 2026 with no confirmed CMEs. Read implications for HF radio, navigation, and near-term forecasts.","rank_math_focus_keyword":"space weather,RGN 4366,solar flares,NOAA,HF radio","footnotes":""},"categories":[2],"tags":[],"class_list":["post-17483","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-top-stories"],"_links":{"self":[{"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/posts\/17483","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/comments?post=17483"}],"version-history":[{"count":0,"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/posts\/17483\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/media\/17481"}],"wp:attachment":[{"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/media?parent=17483"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/categories?post=17483"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/readtrends.com\/en\/wp-json\/wp\/v2\/tags?post=17483"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}