The geomagnetic field was very quiet on November 24. The high latitude magnetometer at Andenes recorded quiet to unsettled conditions.
Solar flux at 20h UT on 2.8 GHz was 100.4 - increasing 12.8 over the previous solar rotation. (Centered 1 year average SF at 1 AU: Minimum of 69.13 on November 17, 2019. Current: 71.74). The Potsdam WDC planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 3.0). Three hour interval K indices: 11001101 (planetary), 11121211 (Boulder), 12001003 (Andenes).
The background x-ray flux is at the class B4 level (GOES 16).
At the time of counting spots (see image time), spots were observed in 7 active regions using 2K resolution (SN: 102) and in 5 active regions using 1K resolution (SN: 64) SDO/HMI images.
Region 12783 [S21W20]
decayed slowly and quietly.
Region 12785 [S21E46] was mostly quiet and stable.
Region 12786 [S16E61] rotated fully into view revealing trailing
spots with a nearly 20 degrees longitudinal separation from the huge
asymmetric leader spot. A major flare is possible. The region was mostly
quiet producing only a long during C1.1 even peaking at 06:06 UT (After
careful analysis of SDO/AIA imagery it became clear that SWPC
wrongly attributed this event to AR 12785 and erroneously split the LDE into
two C1 events). A more significant C3.4 flare was recorded at 04:02 UT on
November 25.
Spotted regions not observed (or interpreted
differently) by SWPC:
S6618 [S22W40] reemerged with tiny spots.
New region S6629 [S19E31] emerged with tiny
spots.
New region S6630 [S21W65] emerged with tiny spots.
New region S6631 [N28E18] emerged with a tiny spot.
A full halo CME became visible in LASCO C2 imagery after 12:48 UT. While its origin was in the southern hemisphere, there was no associated frontside activity to explain this event. This is believed to be a backside event.
C2+ flares:
| Magnitude | Peak time (UT) | Location | AR | Recorded by | Comment |
November 22-24: 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 northern hemisphere coronal hole (CH980) was Earth facing on November 18-22.
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.
The geomagnetic field is expected to be quiet to unsettled on November 25-26 due to effects from CH980 and quiet on November 27-28.
| 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 | ||||||||||
| 12783 | 2020.11.16 2020.11.17 |
4 | 15 | 7 | S20W19 | 0100 | CSO | CSO |
 |
 |
|
| S6616 | 2020.11.17 | N19W41 | |||||||||
| S6618 | 2020.11.17 | 2 | S22W40 | 0002 | AXX |
 |
|||||
| S6621 | 2020.11.19 | S18W15 | |||||||||
| 12784 | 2020.11.20 2020.11.21 |
N32W13 |
 |
||||||||
| 12785 | 2020.11.22 2020.11.22 |
1 | 2 | 1 | S20E44 | 0140 | HSX | HSX |
 |
 |
area: 0170 location: S21E46 |
| S6624 | 2020.11.22 | N08W57 | |||||||||
| 12786 | 2020.11.22 2020.11.23 |
2 | 8 | 4 | S15E59 | 0380 | CKO | FKO |
 |
 |
area: 0840 location: S16E61 |
| S6626 | 2020.11.23 | N27E15 |
 |
||||||||
| S6627 | 2020.11.23 | N07W13 |
 |
||||||||
| S6628 | 2020.11.23 | S34W32 |
 |
||||||||
| S6629 | 2020.11.24 | 2 | 1 | S19E31 | 0003 | AXX |
 |
||||
| S6630 | 2020.11.24 | 2 | 1 | S21W65 | 0005 | BXO |
 |
||||
| S6631 | 2020.11.24 | 1 | N28E18 | 1 | AXX |
 |
|||||
| Total spot count: | 7 | 32 | 14 | ||||||||
| Sunspot number: | 37 | 102 | 64 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 27 | 52 | 34 | (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): | 41 | 56 | 51 | k * (sunspot number) As of May 7, 2016: k = 1.1 for SWPC, k = 0.55 for MSN 2K, k = 0.80 for MSN 1K (MSN=Magnetic Sunspot Number) |
|||||||
| 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) |
| 2019.05 | 71.3 | 72.8 | 9.9 | 3.9 (-0.4) | 6.98 |
| 2019.06 | 68.1 | 70.3 | 1.2 | 3.7 (-0.2) | 4.26 |
| 2019.07 | 67.1 | 69.3 | 0.9 | 3.5 (-0.2) | 5.36 |
| 2019.08 | 67.0 | 68.7 | 0.5 | 3.4 (-0.1) | 6.79 |
| 2019.09 | 67.9 | 68.7 | 1.1 | 3.1 (-0.3) | 9.81 |
| 2019.10 | 67.4 | 67.0 | 0.4 | 2.6 (-0.5) | 7.53 |
| 2019.11 | 70.2 | 68.7 | 0.5 | 2.0 (-0.6) (November 17, 2019 is the solar minimum using 365d smoothing for 1 AU solar flux, NOAA SN and both of STAR 1K and 2K SN) |
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 | 2.8 (+0.6) | 6.16 |
| 2020.03 | 70.2 | 69.5 | 1.5 | 3.0 (+0.2) | 5.63 |
| 2020.04 | 69.5 | 70.0 | 5.4 | 3.6 (+0.6) | 5.32 |
| 2020.05 | 69.0 | 70.6 | 0.2 | (4.7 projected, +1.1) | 3.80 |
| 2020.06 | 69.5 | 71.7 | 5.8 | (5.9 projected, +1.2) | 3.75 |
| 2020.07 | 69.5 | 71.8 | 6.3 | (6.9 projected, +1.0) | 4.28 |
| 2020.08 | 71.6 | 73.4 | 7.6 | (8.2 projected, +1.3) | 5.68 |
| 2020.09 | 70.7 | 71.4 | 0.7 | (10.2 projected, +2.0) | 8.59 |
| 2020.10 | 74.6 | 74.2 | 14.4 | (11.7 projected, +1.5) | 6.13 |
| 2020.11 | (85.2) (1) | 17.1 (2A) / 21.4 (2B) / 27.2 (2C) | (13.1 projected, +1.4) | (4.6) | |
| 2020.12 | (15.2 projected, +2.1) | ||||
| 2021.01 | (17.2 projected, +2.0) | ||||
| 2021.02 | (19.2 projected, +2.0) | ||||
| 2021.03 | (21.4 projected, +2.2) | ||||
| 2021.04 | (23.5 projected, +2.1) | ||||
1) Running average based on the daily 20:00 UTC observed solar flux value at 2800 MHz.
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.
