A long-duration M3.4 solar flare erupted from Active Region 3032 at 04:07 UTC. The event started at 02:58 and ended at 05:12, releasing a large Coronal Mass Ejection (CME).
This event was associated with a Type II Radio Emission with an estimated velocity of 325 km/s (detected at 03:24 UTC). Type II emissions occur in association with eruptions on the Sun and typically indicate a coronal mass ejection is associated with a flare event.
A Type IV radio emission was registered at 03:36 UTC, indicating a strong CME and solar radiation storms were produced.
Additionally, a 10 cm Radio Burst lasting 53 minutes and with a peak flux of 670 sfu was associated with this flare event.
The CME appears to be heading mostly to the east and away from the Earth.
Region 3032 has a ‘beta’ magnetic configuration and is capable of producing more moderate to strong eruptions on the Sun. While its position currently doesn’t favor Earth-directed CMEs, this will change in the days ahead as it moves toward the center of the solar disk.
Featured image: CME produced by the long-duration M3.4 solar flare on June 13, 2022. Credit: NASA/ESA SOHO LASCO C2
If you value what we do here, create your ad-free account and support our journalism.
Your support makes a difference
Dear valued reader,
We hope that our website has been a valuable resource for you.
The reality is that it takes a lot of time, effort, and resources to maintain and grow this website. We rely on the support of readers like you to keep providing high-quality content.
If you have found our website to be helpful, please consider making a contribution to help us continue to bring you the information you need. Your support means the world to us and helps us to keep doing what we love.
Support us by choosing your support level – Silver, Gold or Platinum.
Other support options include Patreon pledges, one-off payments using PayPal and purchasing products from our webshop.
Thank you for your consideration. Your support is greatly appreciated.