The geomagnetic field was at quiet to active levels on June 29, decreasingly under the influence of CME effects. The high latitude magnetometer at Andenes recorded quiet to major storm levels. The above 10 MeV proton flux was at background levels at the end of the day.
Solar flux density measured at 20h UT on 2.8 GHz was 186.4 - increasing 6.6 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 163.20. In comparison SC24 peaked on June 28, 2014 at 145.50. Current SC25 peak: 163.20 on December 30, 2023). The Potsdam WDC planetary A index was 13 (STAR Ap - based on the mean of three hour interval ap indices: 12.6). Three hour interval K indices: 43222333 (planetary), 32363333 (Boulder), 42223346 (Andenes).
The background x-ray flux is at the class C1 level (GOES 16).
At the time of counting spots (see image time), spots were observed in 23 active regions using 2K resolution (SN: 459) and in 19 active regions using 1K resolution (SN: 287) SDO/HMI images.
Region 13719 [S17W69] decayed slowly and
was mostly quiet. C1 flares: C1.6 @ 03:21 UT
Region 13720 [S05W53] decayed slowly and quietly.
Region 13721 [N27W27] was quiet and stable.
Region 13722 [S13W29] decayed slowly and quietly.
Region 13723 [S21W05] decayed slowly and quietly.
Region 13725 [N22W42] decayed slowly and quietly.
Region 13726 [S06W14] was quiet and stable.
Region 13727 [S18E08] was mostly quiet and stable. C1 flares: C1.4 @
11:33 UT
Region 13728 [S28E04] has weak polarity intermixing and produced a
few C flares. C1 flares: C1.5 @ 07:15 UT
Region 13729 [S04E27] has weak polarity intermixing and was mostly
quiet. Some decay was observed in the trialing spot section.
Region 13730 [S17W21] decayed slowly and quietly.
Region 13731 [S16E36] decayed slowly and quietly.
New region 13733 [N04E28] emerged on June 28 and was numbered by SWPC
the next day.
New region 13734 [N08E69] rotated into view on June 28 with SWPC
numbering the region the following day. The region produced several C
flares. C1 flares: C1.8 @ 00:49, C1.8 @ 01:10, C1.7 @ 05:56, C1.3 @ 11:34,
C1.8 @ 14:55, C1.8 @ 15:15 UT
New region 13735 [N17E76] rotated into view with a mature spot.
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
S9830 [S06E09] was quiet and stable.
S9838 [N25E05] was quiet and stable.
S9840 [N27W12] was quiet and stable.
S9843 [N09E27] was quiet and stable.
New region S9847 [S11E45] emerged with tiny spots.
New region S9848 [N11W19] emerged with tiny spots.
New region S9849 [S16E39] emerged with tiny
spots.
New region S9850 [S13W39] emerged with tiny spots.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C2.4 | 06:11 | 13734 | GOES16 | ||
| C2.3 | 13:13 | 13728 | GOES16 | ||
| C5.9 | 15:38 | 13734 | GOES16 | ||
| C3.0 | 18:19 | 13734 | GOES16 | ||
| C2.3 | 19:12 | 13734 | GOES16 | ||
| C3.1 | 21:06 | 13734 | GOES16 | simultaneous flare in AR 13719 | |
| C2.2 | 22:43 | 13734 | GOES16 | ||
| C2.0 | 22:52 | 13727 | GOES16 | ||
| C2.5 | 23:00 | 13728 | GOES16 | ||
| C2.3 | 23:27 | 13734 | GOES16 | ||
| C2.1 | 00:14 (flare started at 23:59) | 13734 | GOES16 |
June 27: No obviously Earth directed CMEs observed.
June 28: A faint partial halo CME was observed during the first hours
of the day, the source was likely a C6.6 flare in AR 13730 at 23:47 UT on
June 27.
June 29: A faint full halo CME was observed after a large, multi
stage filament
eruption in the southern hemisphere. The eruption may have been
triggered by a C2 flare in AR 13728 that occurred at 13:13 UT. The filament
eruption spread westwards and covered a large area with the peak activity
occurring between 15 and 16 UT. The associated CME was
observed in LASCO C2 imagery from 16:12 UT.
[Coronal hole history (since October 2002)]
[Compare today's report to the situation one solar rotation ago:
28 days ago
27 days ago
26 days ago]
No obvious coronal holes are currently in or near Earth facing positions.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle and high latitudes is poor. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet on June 30. Quiet to active conditions are likely on July 1 due to the June 28 CME. Unsettled to major storm conditions are possible on July 2-3 in response to effects related to the June 29 CME.
| Coronal holes (1) | Coronal mass ejections (2) | M and X class flares (3) |
1) Effects from a coronal hole
could reach Earth within the next 5 days. When the high speed
stream has arrived the color changes to green.
2) Effects from a CME are likely to be observed at Earth within 96 hours.
3) There is a possibility of either M or X class flares within the next 48 hours.
Green: 0-30% probability, Yellow: 30-70% probability, Red: 70-100% probability.
(Click on image for 2K resolution).
4K resolution.
Compare to the previous
day's image. 0.5K image
When available the active region map has a coronal hole polarity overlay where red (pink) is negative and blue is positive.
Data for all officially numbered solar regions according to the Solar Region Summary provided by NOAA/SWPC, all other regions are numbered sequentially as they emerge using the STAR spot number. Comments are my own, as is the STAR spot count (spots observed at or inside a few hours before midnight) and data for regions not numbered by SWPC or where SWPC has observed no spots. SWPC active region numbers in the table below and in the active region map above are the historic SWPC/USAF numbers. SWPC data considered to be not sufficiently precise (location, area, classification) are colored red.
| Active region | SWPC date numbered STAR detected |
Spot count | Location at midnight | Area | Classification | SDO / HMI 4K continuum image with magnetic polarity overlays |
Comment | ||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| SWPC/ USAF |
Magnetic (SDO) |
SWPC | STAR | Current | Previous | ||||||
| 2K | 1K | ||||||||||
| 13719 | 2024.06.19 2024.06.19 |
4 | 4 | 2 | S16W69 | 0240 | CSO | DHO |
 |
 |
area: 0410 location: S17W69 |
| 13720 | 2024.06.19 2024.06.19 |
3 | 12 | 5 | S05W56 | 0030 | CRO | CRO |
 |
 |
location: S05W53 |
| S9815 | 2024.06.19 | N16W58 |
 |
||||||||
| 13725 | 2024.06.20 2024.06.23 |
6 | 2 | N18W43 | 0025 | AXX |
 |
 |
location: N22W42 | ||
| 13721 | 2024.06.21 2024.06.21 |
3 | 16 | 7 | N26W28 | 0090 | HAX | CAO |
 |
 |
area: 0110 location: N27W27 |
| 13722 | 2024.06.21 2024.06.21 |
1 | 7 | 3 | S11W30 | 0090 | HSX | CSO |
 |
 |
area: 0220 location: S13W29 |
| 13723 | 2024.06.22 2024.06.23 |
4 | 13 | 7 | S20W07 | 0020 | BXO | BXO |
 |
 |
location: S21W05 area: 0030 |
| 13726 | 2024.06.22 2024.06.23 |
5 | 3 | S04W25 | 0010 | BXO |
 |
 |
location: S06W14 | ||
| 13724 | 2024.06.23 | 1 | S15W30 | 0080 | HSX | SWPC split this off from AR 13722 | |||||
| 13728 | 2024.06.23 2024.06.25 |
7 | 17 | 9 | S27E04 | 0080 | DAO | DAO |
 |
 |
beta-gamma location: S28E04 |
| 13727 | 2024.06.24 2024.06.25 |
6 | 32 | 14 | S18E09 | 0220 | CSO | DHI |
 |
 |
area: 0400 |
| S9830 | 2024.06.24 | 8 | 1 | S06E09 | 0012 | BXO |
 |
 |
|||
| 13729 | 2024.06.25 2024.06.26 |
10 | 38 | 16 | S05E29 | 0220 | EAO | EAO |
 |
 |
area: 0400 location: S04E27 |
| S9832 | 2024.06.25 | N07W37 | |||||||||
| 13730 | 2024.06.26 2024.06.27 |
4 | 7 | 3 | S18W20 | 0020 | CRO | HRX |
 |
 |
|
| 13731 | 2024.06.26 2024.06.28 |
1 | 4 | 2 | S16E35 | 0010 | AXX | CRO |
 |
 |
area: 0020 |
| S9835 | 2024.06.26 | N51W44 | |||||||||
| S9837 | 2024.06.27 | N09E05 | |||||||||
| S9838 | 2024.06.27 | 7 | N25E05 | 0008 | AXX |
 |
 |
||||
| S9839 | 2024.06.27 | S26W29 | |||||||||
| 13732 | 2024.06.28 | 2 | S19E02 | 0040 | HAX | apparently SWPC has split off the westernmost spots of AR 13727. Magnetically there is no separation | |||||
| S9840 | 2024.06.28 | 4 | 3 | N27W12 | 0015 | HRX |
 |
 |
|||
| 13733 | 2024.06.28 2024.06.29 |
5 | 25 | 11 | N05E28 | 0030 | CAO | DRI |
 |
 |
beta-gamma location: N04E28 |
| 13734 | 2024.06.28 2024.06.29 |
3 | 11 | 5 | N08E70 | 0060 | CAO | ESI |
 |
 |
location: N08E69 area: 0100 |
| S9843 | 2024.06.28 | 2 | 2 | N09E27 | 0005 | AXX |
 |
 |
|||
| S9844 | 2024.06.28 | N12W04 |
 |
||||||||
| S9845 | 2024.06.28 | S31E16 |
 |
||||||||
| 13735 | 2024.06.29 2024.06.29 |
1 | 1 | 1 | N17E75 | 0020 | HSX | HSX |
 |
was AR S9846 area: 0080 location: N17E76 |
|
| S9847 | 2024.06.29 | 4 | S11E45 | 0005 | BXO |
 |
|||||
| S9848 | 2024.06.29 | 2 | N11W19 | 0005 | BXO |
 |
|||||
| S9849 | 2024.06.29 | 2 | 1 | S16E30 | 0005 | AXX |
 |
||||
| S9850 | 2024.06.29 | 2 | S13W39 | 0003 | BXO |
 |
|||||
| Total spot count: | 55 | 229 | 97 | ||||||||
| Sunspot number: | 205 | 459 | 287 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 116 | 294 | 162 | (Sum of total spot count + classification weighting for each AR. Classification weighting: X=0, R=3, A/S=5, H/K=10) | |||||||
| Relative sunspot number (Wolf number): | 226 | 252 | 230 | ||||||||
| Month | Average solar flux | International sunspot number (WDC-SILSO) |
Smoothed sunspot number (4) | Average ap (3) |
|
|---|---|---|---|---|---|
| Measured | 1 AU | ||||
| 2014.02 | 170.3 (cycle peak) |
166.3 | 146.1 (SC24 peak) | 110.5 | 10.70 |
| 2014.04 | 143.9 | 144.8 | 112.5 | 116.4 (SC24 solar max) | 7.88 |
| 2017.09 | 91.3 | 92.3 | 43.6 | 18.2 (-1.3) | 18.22 (SC24 peak) |
| 2019.11 | 70.2 | 68.7 | 0.5 | 2.0 (-0.6) (Solar minimum using 365d smoothing: November 17, 2019) |
4.19 |
| 2019.12 | 70.8 | 68.6 | 1.6 | 1.8 (-0.2) (ISN 13 months smoothed solar minimum) |
3.22 |
| 2022.10 | 133.5 | 132.7 | 95.5 | 98.9 (+2.4) | 11.16 |
| 2022.11 | 123.4 | 120.7 | 80.5 | 101.2 (+2.3) | 9.33 |
| 2022.12 | 147.9 | 143.4 | 112.8 | 106.7 (+5.5) | 10.99 |
| 2023.01 | 182.4 | 176.6 | 144.4 | 113.3 (+6.6) | 8.73 |
| 2023.02 | 167.2 | 163.2 | 111.3 | 117.8 (+3.5) | 14.48 |
| 2023.03 | 157.2 | 155.6 | 123.3 | 121.1 (+3.3) | 14.42 |
| 2023.04 | 145.4 | 146.4 | 97.6 | 122.9 (+1.8) | 13.40 |
| 2023.05 | 155.6 | 159.2 | 137.4 | 124.2 (+1.3) | 10.67 |
| 2023.06 | 161.7 | 166.8 | 160.5 | 125.3 (+1.1) | 8.95 |
| 2023.07 | 176.4 | 182.2 | 160.0 | 124.4 (-0.9) | 8.15 |
| 2023.08 | 153.7 | 157.6 | 114.8 | 124.1 (-0.3) | 7.19 |
| 2023.09 | 154.4 | 156.0 | 134.2 | 123.9 (-0.2) | 14.26 |
| 2023.10 | 142.8 | 141.9 | 99.4 | 124.8 (+0.9) | 8.16 |
| 2023.11 | 153.5 | 150.2 | 105.4 | 127.8 (+3.0) | 12.20 |
| 2023.12 | 151.1 | 146.4 | 114.2 | (128.7 projected, +0.9) | 9.60 |
| 2024.01 | 164.6 | 159.3 | 123.0 | (127.0 projected, -1.7) | 5.46 |
| 2024.02 | 172.5 | 168.3 | 124.7 | (126.2 projected, -0.8) | 5.31 |
| 2024.03 | 154.4 | 152.9 | 104.9 | (125.6 projected, -0.6) | 11.03 |
| 2024.04 | 161.3 | 162.6 | 136.5 | (125.6 projected, -0.0) | 9.69 |
| 2024.05 | 187.7 (cycle peak) |
191.9 | 171.7 (SC25 peak) | (126.7 projected, +1.1) | 23.56 (current SC25 peak) |
| 2024.06 | 184.7 (1) | 150.0 (2A) / 155.2 (2B) / 163.7 (2C) | (125.9 projected, -0.8) | (9.9) | |
| 2024.07 | (124.2 projected, -1.7) | ||||
| 2024.08 | (122.2 projected, -2.0) | ||||
| 2024.09 | (121.0 projected, -1.2) | ||||
| 2024.10 | (119.6 projected, -1.4) | ||||
| 2024.11 | (114.5 projected, -5.1) | ||||
| 2024.12 | (109.1 projected, -5.4) | ||||
1) Running average based on the daily 20:00 UTC observed solar flux value at 2800 MHz
and any corrections applied to that measurement.
2A) Current impact on the monthly sunspot number based on the Boulder (NOAA/SWPC) sunspot number (accumulated daily sunspots / month days).
2B) Boulder SN current month average to date.
2C) STAR SDO 1K Wolf number 30 day average.
3) Running average based on the quicklook and definitive Potsdam WDC ap indices. Values in red
are based on the definitive international
GFZ Potsdam WDC ap indices.
4) Source: WDC-SILSO, Royal Observatory
Of Belgium, Brussels
May 2024 easily became the month with the highest sunspot counts during solar cycle 25, and early June has seen no change in that pattern of many spot groups, some of which are large and complex. The next candidate for solar max is still uncertain, however, May 20-21, 2024 has all of the smoothed 365d sunspot numbers as well as the 365d smoothed solar flux signalling a peak on those days.
--------------------------------------------------------------------------------------
This report has been prepared by Jan Alvestad. It is based on the analysis of data from whatever sources are available at the time the report is prepared. All time references are to Universal Time. Comments and suggestions are always welcome.
SDO images are courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.
