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A table titled 'Events on the Sun past 24 hours' listing multiple solar flares on February 1, 2026. It details flare class (e.g., M5.2, X1, M6.7), start, maximum, and end times, with some events associated with region 4366.
A blue-toned coronagraph image showing coronal mass ejections (CMEs) from the Sun, dated 2026/01/31 23:43. Bright emissions extend outwards from the obscured solar disk, indicating significant solar activity.
A split-screen coronagraph image displaying coronal mass ejections (CMEs) from GOES-19 CCOR-1, LASCO C2, and LASCO C3, dated 2026/01/31 21:55. The blue-toned views show bright solar emissions.
A red-toned coronagraph image showing coronal mass ejections (CMEs) from the Sun, dated 2026/02/01 01:48. Bright, radial emissions are visible extending from the central obscured solar disk.
A red-toned coronagraph image displaying coronal mass ejections (CMEs), partially obscured by pixelation. Bright emissions are visible on the left side, indicating ongoing solar activity on 2026/02/01.
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Sun is booming!

2/1/26

2/1 Edited to

... Read moreThe Sun has entered an active phase as evidenced by a series of powerful solar flares and coronal mass ejections (CMEs) occurring on February 1, 2026. Notably, an X1-class solar flare—the strongest category for solar flares—was recorded at 12:24 UTC, accompanied by several M-class flares (M5.8, M6.7, M6.6, M5.2) occurring throughout the day. These events indicate strong magnetic activity on the solar surface, often linked to sunspot regions such as region 4366 identified in the reports. From personal experience monitoring space weather events, observing such intense solar activity suggests heightened chances for geomagnetic storms. These storms, caused by the impact of CMEs with Earth's magnetosphere, can lead to spectacular auroral displays closer to the poles and can affect satellite operations, radio communications, and power grids on Earth. Solar observers and space weather enthusiasts should keep track of updated forecasts and warnings from reliable sources like NOAA and NASA. For those interested in viewing auroras, the increased solar activity offers exciting opportunities to witness these natural light shows, especially in higher latitude regions. However, space weather is complex and unpredictable, so while such solar events increase aurora probability, other atmospheric and geomagnetic conditions also play a role. Monitoring instruments including the GOES-19 satellite X-ray flux data and LASCO coronagraph images reveal the timing and intensity of these solar flares and CMEs, providing valuable data for researchers and the public alike. Keeping informed about these events is essential for prepared communication and navigation systems, and provides a fascinating glimpse into our dynamic Sun’s behavior.