The geomagnetic field was quiet on July 21. The high latitude magnetometer at Andenes recorded quiet to active conditions.
Solar flux density measured at 20h UT on 2.8 GHz was 93.5 - increasing 12.9 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 77.35). The Potsdam WDC planetary A index was 6 (STAR Ap - based on the mean of three hour interval ap indices: 5.8). Three hour interval K indices: 22112210 (planetary), 33122210 (Boulder), 43114421 (Andenes).
The background x-ray flux is at the class B2 level (GOES 16).
At the time of counting spots (see image time), spots were observed in 10 active regions using 2K resolution (SN: 173) and in 7 active regions using 1K resolution (SN: 99) SDO/HMI images.
Region 12842 [N25W66] was quiet and decayed
significantly losing more than half of its area.
Region 12844 [S42E04] reemerged with tiny spots.
Region 12845 [S15W59] developed as new flux
emerged. A C1.3 flare was recorded at 20:05 UT
Region 12846 [N25E49] was quiet and stable.
Region 12847 [S28E61] was quiet and stable.
New region 12848 [N20E16] was first observed with spots on July 18,
then decayed. New flux emerged on July 20 and the region was numbered the
next day by SWPC. Slow decay was observed after noon on July 21.
New region 12849 [S17E75] rotated into view with a single small spot
and produced a C1.2 flare at 16:04 UT.
Spotted regions not observed (or interpreted
differently) by SWPC:
New region S7001 [N21E04] emerged with tiny spots.
New region S7002 [N27E23] emerged with tiny spots.
New region S7003 [S12W18] emerged with a tiny spot.
C2+ flares:
| Magnitude | Peak time (UT) | Location | AR | Recorded by | Comment |
July 19-21: 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]
No obvious coronal holes are currently in or near Earth facing locations.
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 fair.
The geomagnetic field is expected to be quiet on July 22-24.
| 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 red colored.
| 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 | ||||||||||
| 12842 | 2021.07.09 2021.07.10 |
7 | 17 | 7 | N25W66 | 0080 | DSI | DSI |
 |
 |
|
| S6981 | 2021.07.13 | N20W45 | |||||||||
| S6984 | 2021.07.14 | N14W51 | |||||||||
| S6985 | 2021.07.14 | S21W37 | |||||||||
| 12844 | 2021.07.15 2021.07.16 |
3 | S43W04 | 0004 | AXX |
 |
location: S42E04 | ||||
| 12845 | 2021.07.17 2021.07.17 |
4 | 15 | 6 | S15W61 | 0060 | DSO | DRI |
 |
 |
location: S15W59 |
| S6991 | 2021.07.17 | S31E04 | |||||||||
| S6993 | 2021.07.17 | N35W39 | |||||||||
| S6994 | 2021.07.18 | N17W43 |
 |
||||||||
| 12848 | 2021.07.18 2021.07.21 |
4 | 9 | 5 | N20E16 | 0010 | BXO | DRO |
 |
 |
location: N21E18 area: 0050 |
| S6996 | 2021.07.18 | N24W20 | |||||||||
| 12846 | 2021.07.19 2021.07.19 |
7 | 19 | 6 | N25E49 | 0090 | CSO | CAI |
 |
 |
|
| S6998 | 2021.07.19 | N22W28 | |||||||||
| 12847 | 2021.07.20 2021.07.20 |
3 | 4 | 2 | S28E61 | 0020 | CRO | DRO |
 |
 |
|
| S7001 | 2021.07.21 | 2 | 2 | N21E04 | 0010 | BXO |
 |
||||
| S7002 | 2021.07.21 | 2 | N27E23 | 0002 | BXO |
 |
|||||
| S7003 | 2021.07.21 | 1 | S12W18 | 0002 | AXX |
 |
|||||
| 12849 | 2021.07.21 2021.07.21 |
1 | 1 | 1 | S18E75 | 0000 | AXX | AXX |
 |
area: 0010 | |
| Total spot count: | 26 | 73 | 29 | ||||||||
| Sunspot number: | 86 | 173 | 99 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 44 | 92 | 48 | (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): | 95 | 95 | 79 | k * (sunspot number) As of May 7, 2016: k = 1.1 for SWPC, k = 0.55 for STAR 2K, k = 0.80 for STAR 1K |
|||||||
| 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 (cycle 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 |
| 2020.01 | 72.2 | 69.9 | 6.4 | 2.2 (+0.4) | 4.39 |
| 2020.02 | 71.0 | 69.3 | 0.4 | 2.7 (+0.5) | 6.16 |
| 2020.03 | 70.2 | 69.5 | 1.5 | 3.0 (+0.3) | 5.63 |
| 2020.04 | 69.5 | 70.0 | 5.4 | 3.6 (+0.6) | 5.32 |
| 2020.05 | 69.0 | 70.6 | 0.2 | 5.6 (+2.0) | 3.80 |
| 2020.06 | 69.5 | 71.7 | 5.8 | 7.9 (+2.3) | 3.75 |
| 2020.07 | 69.5 | 71.8 | 6.3 | 9.0 (+1.1) | 4.28 |
| 2020.08 | 71.6 | 73.4 | 7.6 | 9.5 (+0.5) | 5.68 |
| 2020.09 | 70.7 | 71.4 | 0.7 | 10.5 (+1.0) | 8.59 |
| 2020.10 | 74.6 | 74.2 | 14.6 | 11.9 (+1.4) | 6.13 |
| 2020.11 | 89.9 | 88.0 | 34.5 | 13.6 (+1.7) | 4.77 |
| 2020.12 | 86.9 | 84.2 | 23.1 | 15.3 (+1.7) | 4.72 |
| 2021.01 | 76.0 | 73.6 | 10.4 | (17.5 projected, +2.2) | 4.39 |
| 2021.02 | 74.3 | 72.4 | 8.3 | (20.3 projected, +2.8) | 9.50 |
| 2021.03 | 76.0 | 75.2 | 17.3 | (23.7 projected, +3.4) | 10.17 |
| 2021.04 | 75.9 | 76.4 | 24.5 | (27.8 projected, +4.1) | 8.40 |
| 2021.05 | 75.3 | 77.1 | 21.2 | (30.5 projected, +2.7) | 6.50 |
| 2021.06 | 79.4 | 81.8 | 25.3 | (33.7 projected, +3.2) | 5.52 |
| 2021.07 | 81.1 (1) | 28.4 (2A) / 41.9 (2B) / 50.9 (2C) | (38.3 projected, +4.6) | (5.5) | |
| 2021.08 | (43.0 projected, +4.7) | ||||
| 2021.09 | (48.6 projected, +5.6) | ||||
| 2021.10 | (53.0 projected, +4.4) | ||||
| 2021.11 | (57.6 projected, +4.6) | ||||
| 2021.12 | (63.5 projected, +5.9) | ||||
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.
