The active Sun Spot group AR1429

The Sun Spot group AR1429 is a very active sun region that has produced recently two major solar flares with coronal mass ejections: the first one was an X1-class on March 5th 04:13UTC, and the second, even more powerful, an X5-class on March 7th at 00:28 UTC.

Several spacecraft have been affected by the heavy radiation and unleashed wave of solar plasma and energetic particles. By example, the Star Tracker units of the probe Venus Express were blinded for 2 days due to the harsh plasma environment in the aftermath of the CME cloud shock wave.

The next images, taken from ESAC on March 10th, 2012, show the Sun in visible and H-alpha, highlighting the AR1429.

AR1429 sunspot group in visible light. Stacked sequence with a Phillips ToUcam webcam, and a Celestron C8" NGT scope with Baader filter.

Visible light. Canon 550D image with a Celestron C8" NGT scope with Baader filter.

H-alpha image. Canon 550D image with a Coronado Solarmax 70. Limb and disk are processed separately and merged into the final image.

The telescope set-up: Coronado Solarmax 70, Celestron Advanced GT mount, Phillips ToUcam webcam.

Visible sunspots

The following mosaic was acquired on 14 October 2011 from ESAC with Michel's Celestron newtonian (1m focal, 20cm aperture) and a Baader film filter. Several sunspots groups (1314, 1316, 1317 and 1319) are visible in the image. Another smaller group is seen to the left of group 1319, but it quickly fainted in the following days. We named the group 1319 informally "the Canary Islands", due to the resemblance with the topography of these islands.

This other image was taken in H-alpha with the Solarmax Coronado and shows several dark filaments, along with the sunspots. This image can be compared with images on previous days (check this previous blog entry).

This last animation shows the position of the sunspots and other features in both visible and H-alpha wavelengths.

Sunspot Group no.1302, 22 Sep 2011

Hydrogen Alpha image sequence of the sunspot group 1302 and the prominence associated with the X1.4 class solar flare which peaked around 11:00 UTC on September 22nd, 2011.

The images have been captured from ESAC, with a Coronado Solarmax 70 Telescope.

Time coverage: 11:07 UTC - 14:40 UTC

Rate: 1 frame/minute

Michel, Leo and Miguel, dismounting the telescope after observation.