Large solar flares and CME eruption

On 3 June 2026, Active region 14455 produced several major (M- and X-class) flares and eruptions. Attached video shows solar activity during this period as observed by GONG/El Teide (Canary Islands). A major flare of M7.7 class peaked at about 7:00 UT and another flare of X1.0 class peaked at about 11:28 UT. Flares of this class are typically associated with the coronal mass ejections (CMEs) and in fact, there is an idication of the erupting material during the first flare (see dark filamentary structures appearing shortly after the flare brightenning). LASCO C3 coronagraph shows CME signatures for both events.

NSO/Kitt Peak Fourier Transform Spectrometer

 

https://noirlab.edu/public/images/noao-sun/

The Fourier Transform Spectrometer  (FTS) was operating at NSO's McMath-Pierce Solar Telescope from early 1970 (1971-1976) till 2001. In 2012, it was relocated to Old Dominion University in Norfolk, VA. The FTS data were used for solar and atmospheric physics research, and to develop several high-spectral resolution atlases of solar spectra: Flux from 296 to 1300 nm; Photosphere from 357 to 740.5 nm; Photosphere from 735 to 1123 nm; Infrared from 1100 to 5400 nm; Sunspot from 8100 to 21,000 nm plus photosphere from 16,000 to 22,000 nm; Sunspot umbra from 664.2 to 1123 nm; Sunspot umbra from 1160 to 5100 nm.

Recently, Mr. John Williams developed an interface for displaying solar spectra and extracting data from different FTS atlases. The interface can be accessed via fts.terrazoom.com.

Solar Activity Report: May 25 - 31, 2026

 

During the past week, solar activity was predominantly low, characterized by low‑intensity C‑class flares. The most significant event was an M1.1 flare on 29 May originating from Active Region 14455 in the northeast quadrant. All remaining activity consisted of low C‑class flares, and no Earth‑directed CMEs were identified.

GONG data processing update

 Processing of the network-merged daily velocity and magnetogram images,  p-mode-coefficient time series, and ring-diagram analysis products for GONG month 313,  and  the  p-mode frequency data products for central GONG month 312 is completed and the data products are now available.

Solar Activity Report: May 18 - 24, 2026

 Solar activity at the beginning of the week was at low levels, with the X‑ray flux holding in the B range except for a few low‑intensity C‑class flares. Activity dipped even further on 20 May, when the flux remained entirely below the B–C threshold. By mid‑day on 21 May, conditions shifted. Activity rose following three short‑duration, high‑intensity impulsive C‑class flares from Active Region 14436 as it approached the northwest limb: C5.6, C8.3, and C9.5. A more substantial increase occurred on 22 May, when an M2.3 flare erupted from just beyond the northwest limb, near the same active region, pushing activity into the moderate range. On 23 May, a series of low and medium intensity C‑class flares were recorded and the week concluded with low flaring activity. Most of the flaring during the last two days originated from newly emerged Active Region 14446 near the southeast limb. Multiple CMEs were observed in coronagraph imagery, but none were Earth‑directed.

Helioseismic map of the far hemisphere (see the attached pictures) reveals two strong active regions, marked by while circles, forecast to return to Earth view on 27 and 31 May.  A third region, marked by a red circle, shows a detectable helioseismic signature, but its probability of appearance remains below our confidence threshold. If it continues to strengthen, it should reach the east limb on 29 May. The far‑side active region mentioned in last week’s report has now rotated onto the front side and has been assigned NOAA 14446.

Small flare near solar central meridian

 Not all solar flares are large. This example shows a relatively weak flare (X-ray C1.3 class), which erupted from active region 14439 on 22 May 2026. The flare started at about 4:38 UT and peaked at 4:50 UT.  C-class flares are typically not associated with the Coronal Mass Ejections (CMEs). GONG at Learmonth, Australia captured the flare with its H-alpha instrument, as shown in this short video (4:20 UT - 7:12 UT)

 

GONG Network Window Function

Last week, NISP Data Center has been working on re-instating the GONG network window function monthly plots that were generated and discontinued a few years ago. Once completed, the window function plots would be available at https://gong.nso.edu/data/merged/gong+_merged_plots.html. Example of old-format window function for the month of April, 2026 is shown below. For each day of the month, red-colored bars represent periods with network observations. Gaps shown in the white color are periods without observations. The impact of missing observations from GONG at Mauna Loa observatory is clearly visible as larger data gaps in late (20-24 UT)  and early (0-4 UT) periods of the day. Numbers of the right side of the plot show average daily duty cycle (% of 24 hour period with observations). Even with one station down, the network still meets the required duty cycle.