The geomagnetic field was quiet on June 10. The high latitude magnetometer at Andenes recorded quiet to unsettled levels.
Solar flux density measured at 20h UT on 2.8 GHz was 110.5 - decreasing 42.2 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 100.43). The Potsdam WDC planetary A index was 4 (STAR Ap - based on the mean of three hour interval ap indices: 3.9). Three hour interval K indices: 21112001 (planetary), 211131** (Boulder), 31023202 (Andenes).
The background x-ray flux is at the class B5 level (GOES 16).
At the time of counting spots (see image time), spots were observed in 10 active regions using 2K resolution (SN: 152) and in 7 active regions using 1K resolution (SN: 90) SDO/HMI images.
Region 13028 [N14W28] reemerged with a tiny spot.
Region 13029 [S23W02] decayed slowly and
quietly. Note that SWPC has moved AR 13029 westwards to the position of AR
S7622.
New region 13030 [N20E62] rotated into view early on June 9 and
developed slowly that day. Slow decay was observed on June 10. For unknown
reasons SWPC seems to have included the spots of AR S7626 in this group.
Spotted regions not observed (or interpreted
differently) by SWPC:
S7609 [S27W50] was quiet and stable.
S7622 [S16W27] decayed slowly and quietly.
S7626 [N20E74] was unstable during the first half of the day
producing several C flares and one M class flare. C1 flare: C1.1 @ 03:21 UT
S7627 [N19E01] decayed slowly and quietly.
New region S7628 [S13E37] was observed with tiny spots in an old
plage area.
New region S7629 [N18E48] was observed with tiny spots in an
old plage area.
New region S7630 [S27E50] emerged with tiny
spots.
C2+ flares:
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C3.7 | 05:46 | N21E75 | 13030 | GOES16 | |
| C4.1 | 08:32 | N25E90 | S7626 | GOES16 | attributed to AR 13030 by SWPC |
| M1.2 | 10:54 | N18E87 | S7626 | GOES16 | LDE, attributed to AR 13030 by SWPC |
| C2.3 | 14:32 | N20E80 | S7626 | GOES16 | LDE, attributed to AR 13030 by SWPC |
June 8-10: No obviously Earth directed CMEs were observed in available LASCO imagery.
[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]
A recurrent trans equatorial coronal hole (CH1081) will likely rotate into an Earth facing position on June 12-13.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle and high latitudes is fair. Propagation on long distance northeast-southwest paths is poor.
Quiet geomagnetic conditions are likely on June 11-13.
| Coronal holes (1) | Coronal mass ejection (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 | ||||||||||
| S7609 | 2022.06.02 | 4 | S27W50 | 0005 | BXO |
 |
 |
||||
| S7611 | 2022.06.02 | N12W59 | |||||||||
| 13029 | 2022.06.03 2022.06.04 |
8 | 10 | 3 | S17W26 | 0030 | BXO | BXO |
 |
 |
location: S23W02 area: 0015 Note that SWPC has moved the location of this group to that of AR S7622 |
| S7614 | 2022.06.04 | S19W52 | |||||||||
| 13028 | 2022.06.04 2022.06.04 |
1 | N14W32 | 0002 | AXX |
 |
location: N14W28 | ||||
| S7616 | 2022.06.04 | N04W59 | |||||||||
| S7622 | 2022.06.08 | 12 | 6 | S16W27 | 0025 | CRO |
 |
 |
|||
| S7623 | 2022.06.08 | S21E36 | |||||||||
| 13030 | 2022.06.09 2022.06.10 |
5 | 7 | 5 | N20E65 | 0140 | EAO | DAO |
 |
 |
area: 0070 location: N20E62 |
| S7625 | 2022.06.09 | N19W14 |
 |
||||||||
| S7626 | 2022.06.09 | 2 | 2 | N20E74 | 0100 | HAX |
 |
 |
|||
| S7627 | 2022.06.09 | 2 | 1 | N19E01 | 0004 | BXO |
 |
 |
|||
| S7628 | 2022.06.10 | 4 | 1 | S13E37 | 0007 | AXX |
 |
||||
| S7629 | 2022.06.10 | 3 | N18E48 | 0005 | BXO |
 |
|||||
| S7630 | 2022.06.10 | 7 | 2 | S27E50 | 0012 | BXO |
 |
||||
| Total spot count: | 13 | 52 | 20 | ||||||||
| Sunspot number: | 33 | 152 | 90 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 18 | 65 | 33 | (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): | 36 | 84 | 72 | ||||||||
| 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 (solar max) | 7.88 |
| 2017.09 | 91.3 | 92.3 | 43.6 | 18.2 (-1.3) | 18.22 (cycle 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 |
| 2020.12 | 86.9 | 84.2 | 23.1 | 15.3 (+1.7) | 4.72 |
| 2021.01 | 76.0 | 73.6 | 10.4 | 17.3 (+2.0) | 4.39 |
| 2021.02 | 74.3 | 72.4 | 8.2 | 19.0 (+1.7) | 9.50 |
| 2021.03 | 76.0 | 75.2 | 17.2 | 21.7 (+2.7) | 10.17 |
| 2021.04 | 75.9 | 76.4 | 24.5 | 24.8 (+3.1) | 8.40 |
| 2021.05 | 75.3 | 77.1 | 21.2 | 25.8 (+1.0) | 6.50 |
| 2021.06 | 79.4 | 81.8 | 25.0 | 27.6 (+1.8) | 5.52 |
| 2021.07 | 81.0 | 83.6 | 34.3 | 31.3 (+3.7) | 5.51 |
| 2021.08 | 77.7 | 79.7 | 22.0 | 35.3 (+4.0) | 6.19 |
| 2021.09 | 87.0 | 88.2 | 51.3 | 40.0 (+4.7) | 6.33 |
| 2021.10 | 88.9 | 88.3 | 37.4 | 45.0 (+5.0) | 7.38 |
| 2021.11 | 86.2 | 84.4 | 34.8 | 50.6 (+5.6) | 9.83 |
| 2021.12 | 103.0 | 99.8 | 67.5 | (55.7 projected, +5.1) | 6.40 |
| 2022.01 | 103.8 | 100.5 | 54.0 | (60.4 projected, +4.7) | 8.92 |
| 2022.02 | 109.1 | 106.5 | 59.7 | (66.9 projected, +6.5) | 10.46 |
| 2022.03 | 117.0 | 115.8 | 78.5 | (72.4 projected, +5.5) | 10.20 |
| 2022.04 | 130.8 | 131.7 | 84.1 | (77.6 projected, +5.2) | 11.79 |
| 2022.05 | 133.8 | 136.8 | 96.5 | (84.1 projected, +6.5) | 7.48 |
| 2022.06 | 101.7 (1) | 14.0 (2A) / 42.0 (2B) / 99.3 (2C) | (89.9 projected, +5.8) | (4.7) | |
| 2022.07 | (97.2 projected, +7.3) | ||||
| 2022.08 | (103.8 projected, +6.6) | ||||
| 2022.09 | (108.8 projected, +5.0) | ||||
| 2022.10 | (112.0 projected, +3.2) | ||||
| 2022.11 | (114.8 projected, +2.8) | ||||
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: SIDC-SILSO.
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.
