Sun news, September 23, 2025. NOAA has announced the launch of SWFO-L1 tomorrow, a solar-wind-monitoring satellite that will head into space alongside 2 other sun-focused spacecraft. Image via NOAA.
Sun News September 23: Triplet of space weather missions launch tomorrow
(11 UTC to 11 UTC)
Today’s top story: NASA and NOAA have announced that SpaceX will launch a triplet of missions tomorrow to study the sun and its solar wind. The Falcon 9 rocket will carry NASA’s Interstellar Mapping and Acceleration Probe (IMAP), the Carruthers Geocorona Observatory, and NOAA’s Space Weather Follow-On L1 (SWFO-L1). Together, these spacecraft will expand our ability to monitor the sun, measure the solar wind, and forecast space weather. Liftoff is set for 7:30 a.m. EDT from Kennedy Space Center, with a 90% chance of favorable weather.
Flare activity: The sun stayed at low levels, producing 7 C-class flares over the past day.
Strongest: C4.2 from an unnumbered southeast region at 16:09 UTC on September 22.
Other notable flares: C3.8 (AR4227 at 17:26 UTC), C2.6 (AR4227 at 16:47 UTC), and C2.2 (unnumbered northeast region at 0:12 UTC). AR4227 was the most productive region with three C flares.
Sunspot regions: The Earth-facing side of the sun shows 10 numbered active regions.
AR4217 (southwest, beta-gamma) gained a gamma configuration.
The rest of the regions remained small, stable, or slowly decayed.
Blasts from the Sun? No Earth-directed CMEs appeared in coronagraph imagery. A striking prominence, which you can see below, erupted on the sun’s far side and is not Earth-directed.
Solar wind: The solar wind surged. Speeds climbed from 300 km/s at the start of the period to 669 km/s, peaking at 812 km/s at 21 UTC on September 22. The IMF rose to moderate levels, and the Bz flipped between north and south before ending northward.
Earth’s magnetic field: Conditions ranged from quiet to unsettled (Kp = 2–3). The Kp index was just below 3 at the close of the period.
What’s ahead? Sun–Earth forecast
Flare activity forecast: Mostly C-class activity is expected, with a 35% chance of an M-class (R1–R2) flare, most likely from AR4220 or AR4217.
Geomagnetic activity forecast:
September 23: Unsettled-to-active conditions expected, with isolated G1 (minor) storms likely and a slight chance of G2 (moderate) storms from the corotating interaction region (CIR) impact.
September 24–25: Conditions should ease from quiet to unsettled as coronal hole effects diminish.
September 23, 2025. The GOES-19 satellite observed this fiery prominence emerging from the far side of the sun over the past day. SUVI 304 angstrom. Image via NOAA.This image shows sun activity – with the most active regions labeled – as of 2 UTC on September 23, 2025, as seen from Learmonth Solar Observatory in Australia. Original image, without labels, via NSO/GONG. Today’s sun is posted by Armando Caussade. Why are east and west on the sun reversed?
Sun news September 22: Solar wind set to rise; auroras possible
Flare activity: Solar activity stayed at low levels with 12 flares in the past 24 hours, all in the C (common) range.
Strongest: C6.6 from AR4223 at 21:16 UTC on September 21.
Other notable events: C3.3 (AR4224 at 17:43 UTC), C2.3 (AR4220 at 17:01 UTC), and C2.7 (AR4217 at 21:31 UTC). AR4217 kept busy with multiple smaller C flares, including three during the early hours of September 22.
Sunspot regions: Ten numbered regions are currently on the solar disk.
AR4220 (southwest, beta-gamma) stayed the most active and complex, though its trailing spots showed some decay.
AR4223 (south-central, alpha) decayed to a simpler form but still managed the strongest flare of the day.
AR4217 (southwest, beta) added intermediate spots and stayed moderately active.
AR4224 (south-central, beta-gamma) continued to grow and produced one of the larger C flares.
Other regions remained small, stable, or in slow decay.
Blasts from the Sun? No Earth-directed coronal mass eejections CMEs appeared in coronagraph imagery. Several prominence eruptions were spotted on September 21, but none are Earth-directed.
Solar wind: The solar wind stayed slow, below 300 km/s. The interplanetary magnetic field (IMF) was weak and the Bz flipped gently between north and south. A rise in speed and density is expected later today as the fast solar wind arrives.
Earth’s magnetic field: Earth’s magnetic field stayed quiet yesterday (Kp = 0–2). Forecasts call for unsettled-to-active conditions, with isolated G1 (minor) storms possible today as the fast solar wind arrives. A slight chance exists for G2 (moderate) conditions when the corotating interaction region hits. Conditions should ease back to quiet-to-unsettled by September 23–24.
This image shows sun activity – with the most active regions labeled – as of 2 UTC on September 22, 2025, as seen from Learmonth Solar Observatory in Australia. Image via NSO/ GONG.This image shows sun activity – with the most active regions labeled – as of 2 UTC on September 21, 2025, as seen from Learmonth Solar Observatory in Australia. Image via NSO/ GONG.This image shows sun activity – with the most active regions labeled – as of 4 UTC on September 20, 2025, as seen from Learmonth Solar Observatory in Australia. Image via NSO/ GONG.
Sun images from our community
We sometimes feature sun images obtained using hydrogen-alpha filters. Read why.
View at EarthSky Community Photos. | Patricio León in Santiago, Chile, captured this filtered image of the sun on September 22, 2025. Patricio wrote: “Many sunspots of all sizes and shapes fill the solar face from limb to limb. This is quite a grand show! Uneasy sun, Kp index and solar wind speed are medium high.” Thank you, Patricio!View at EarthSky Community Photos. | Mandy Daniels in Derbyshire, United Kingdom, captured this filtered image on September 22, 2025. Mandy wrote: “The sun, showing a good few sunspots today.” Thank you, Mandy!View at EarthSky Community Photos. | David Hawkes in South Yorkshire, United Kingdom, captured this filtered image of the sun on September 21, 2025. David wrote: “After a pretty appalling bout of rainy UK weather, the sun finally came out of hiding for eclipse day with a nice arrangement of sunspots.” Thank you, David!View at EarthSky Community Photos. | Mario Rana in Hampton, Virginia, captured these filtered images on September 20, 2025. Mario wrote: “The sun in various wavelengths: hydrogen-alpha, hydrogen-beta, hydrogen-gamma, hydrogen-delta, helium D3, and calcium-H.” Thank you, Mario!View at EarthSky Community Photos. | Jim Militello in Tucson, Arizona, captured this filtered image of the sun on September 18, 2025. Jim wrote: “Hydrogen-alpha image of the sun showing numerous sunspot active regions and prominences.” Thank you, Jim!
C. Alex Young is a solar astrophysicist studying the Sun and space weather. Alex is passionate about sharing science with diverse audiences. This led him to start The Sun Today with his designer wife, Linda. First through Facebook and Twitter then adding an extensive website thesuntoday.org, the two work together to engage the public about the Sun and its role in our solar system. Alex led national engagement efforts for the 2017 total solar eclipse. He is the Associate Director for Science in the Heliophysics Science Division at NASA Goddard Space Flight Center.
Raúl Cortés studied engineering at the Autonomous University of Nuevo León in Monterrey, Mexico, obtained a scholarship to continue his studies in Japan and after returning to Monterrey he got credits on MBA from the Graduate School of Mechanical and Electrical Engineering Faculty. He became a teacher at the University UANL teaching Math and Physics and dedicated the rest of his professional career to serve in engineering areas for USA, Japan and Germany based corporations. His passion for the skies go back to when he was a child, always intrigued about the stars and constellations and reading and researching about the matter. From 2010 on, he dedicated his attention to photographing the stars, constellations, the moon and the sun. Raúl's work on his photography has been published and posted on the ESC as well as in other platforms and has gained attention to be published by local Monterrey newspapers.
Armando is known primarily as an astronomy educator, after 30+ years of extensive public outreach and 10 years teaching in colleges. As one of only a handful of science communicators in Puerto Rico during Comet Halley's last visit, he assumed a pioneering role starting in 1985 when science was just beginning to enter the collective mindset. Over the years, his work as a teacher, speaker and writer, inspired people to pursue interests in science and brought enduring change to Puerto Rican culture. After being accepted into the 2014–2015 Antarctic season of PolarTREC, Armando was assigned to the Amundsen-Scott South Pole Station, where in 2015 he successfully conducted 10 days of work at the IceCube Neutrino Observatory. His affiliations include Ana G. Méndez University, Cupey campus (2014 to 2021), the University of Puerto Rico, Aguadilla campus (2015 to 2017), NASA JPL's Solar System Ambassadors (2004 to 2006), and NASA Space Grant (2017 to 2019) where he served as an affiliate representative.
Like what you read? Subscribe and receive daily news delivered to your inbox.
Thank you! Your submission has been received!
Oops! Something went wrong while submitting the form.