The geomagnetic field was quiet to minor storm on November 4 under the influence of effects from CH697. Solar wind speed at SOHO ranged between 545 and 778 km/s.
Solar flux at 20h UTC on 2.8 GHz was 113.8 (increasing 34.3 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 104.9. The Potsdam WDC planetary A index was 29 (STAR Ap - based on the mean of three hour interval ap indices: 28.9). Three hour interval K indices: 45545222 (planetary), 45654322 (Boulder).
The background x-ray flux is at the class B5 level.
At the time of counting spots (see image time), spots were observed in 6 active regions using 2K resolution (SN: 156) and 5 active regions using 1K resolution (SN: 103) SDO images on the visible solar disk.
Region 12442 [N16W79] produced 2 M flares and is
decaying slowly. This is
AR 12445 to SWPC.
Region 12443 [N06W12] decayed losing penumbral area and spots. The region has
minor polarity intermixing and another M class flare is possible.
Region 12447 [N03E12] decayed in the leading spot section while slow
development was observed in the trailing spot section.
New region 12448 [N06E76] rotated partly into view on November 3 and was
numbered by SWPC the next day.
Spotted regions not numbered (or interpreted differently) by SWPC:
S4860 [N19E01] was quiet and stable.
S4871 [N03E66] was quiet and stable.
C2+ flares:
| Magnitude | Peak time (UTC) | Location | AR | Recorded by | Comment |
| C3.0 | 00:32 | N15W63 | 12442 | GOES15 | |
| M1.9/1N | 03:26 | N15W64 | 12442 | GOES15 | CME, triggered filament eruption |
| C4.6 | 09:00 | N17W65 | 12442 | GOES15 | |
| M2.5/1N | 12:03 | N12W73 | 12442 | GOES15 | |
| M3.7/2B (LDE) | 13:52 | N09W04 | 12443 | GOES15 | M4.7 @ SDO/EVE partial halo CME |
| C5.0 | 15:57 | 12442 | SDO/EVE | ||
| C3.1 | 16:45 | 12442 | SDO/EVE |
November 2-3: No obviously Earth directed CMEs were observed in
available LASCO imagery.
November 4: A partial halo CME was observed after the M3 LDE in AR 12443.
The CME could reach Earth on November 6.
[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 (CH697) was in an Earth facing position on October 30-November 1. The southernmost parts of a large northern hemisphere coronal hole (CH698) will be in a potentially geoeffective position on November 5-8. A recurrent trans equatorial coronal hole (CH699) will likely rotate across the central meridian on November 6-7.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle latitudes is poor. Propagation on long distance northeast-southwest paths is poor to fair.
The geomagnetic field is expected to be quiet to unsettled on November 5 due to effects from CH697. The CME observed on November 4 could reach Earth on November 6 and cause unsettled to minor storm conditions that day and on November 7. Effects from CH698 and CH699 will likely cause unsettled to active conditions on November 8-11.
| 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)
Compare to the previous day's 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 numbered solar regions according to the Solar Region Summary provided by NOAA/SWPC. 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.
| Active region | Date numbered detected |
Spot count | Location at midnight | Area | Classification | SDO / HMI 4K continuum image with magnetic polarity overlays |
Comment | ||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| SWPC | Magnetic (SDO) |
SWPC | STAR | Current | Previous | ||||||
| 2K | 1K | ||||||||||
| 12441 | 2015.10.27 | N15W60 |
 |
||||||||
| 12442 | 2015.10.27 2015.10.28 |
7 | 5 | N16W90 | 0250 | EAO |
 |
 |
beta-gamma location: N16W79
|
||
| 12443 | 2015.10.28 2015.10.29 |
40 | 71 | 39 | N06W09 | 0370 | FKC | FAC |
 |
 |
beta-gamma area: 0550 location: N06W12 |
| 12444 | 2015.10.28 2015.10.29 |
S04W29 | |||||||||
| S4860 | 2015.10.29 | 2 | N19E01 | 0003 | AXX |
 |
  |
||||
| S4861 | 2015.10.30 | N11W27 | |||||||||
| S4862 | 2015.10.30 | S07W48 | |||||||||
| S4865 | 2015.10.31 | S13W30 |
 |
||||||||
| 12446 | 2015.10.31 2015.11.01 |
N15W44 |
 |
||||||||
| S4867 | 2015.10.31 | N32W09 | |||||||||
| S4868 | 2015.10.31 | S01W25 | |||||||||
| 12445 | 2015.11.01 | 6 | N17W80 | 0140 | EAI | part of AR 12442 | |||||
| S4869 | 2015.11.01 | N16W39 |
  |
||||||||
| 12447 | 2015.11.03 | 4 | 8 | 3 | N03E10 | 0010 | CRO | CRO |
 |
 |
area: 0020 location: N03E12 |
| S4871 | 2015.11.03 | 1 | 1 | N03E66 | 0006 | AXX |
 |
 |
|||
| 12448 | 2015.11.03 2015.11.04 |
3 | 7 | 5 | N06E72 | 0060 | DSO | DAO |
 |
 |
area: 0250 location: N06E76 |
| S4873 | 2015.11.03 | S13W07 |
 |
||||||||
| S4874 | 2015.11.03 | S08W55 |
 |
||||||||
| Total spot count: | 53 | 96 | 53 | ||||||||
| Sunspot number: | 93 | 156 | 103 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 76 | 114 | 72 | (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): | 102 | 86 | 88 | k * (sunspot number) As of July 1, 2015: k = 1.1 for SWPC, k = 0.55 for MSN 2K, k = 0.85 for MSN 1K (MSN=Magnetic Sunspot Number) |
|||||||
| Month | Average solar flux | International sunspot number (WDC-SILSO) (4) |
Smoothed sunspot number (4) | Average
ap (3) |
|
|---|---|---|---|---|---|
| Measured | 1 AU | ||||
| 2014.02 | 170.3 (cycle peak) |
166.3 | 146.1 (cycle peak) | 110.5 (+1.2) | 10.70 |
| 2014.04 | 143.9 | 144.8 | 112.5 | 116.4 (+2.1) (solar max) | 7.88 |
| 2014.09 | 146.6 | 148.1 | 130.0 | 101.9 (-6.4) | 9.78 |
| 2014.10 | 153.4 | 152.9 | 90.0 | 97.3 (-4.6) | 8.96 |
| 2014.11 | 154.8 | 151.4 | 103.6 | 94.7 (-2.6) | 9.33 |
| 2014.12 | 158.7 | 153.8 | 112.9 | 92.2 (-2.5) | 11.24 |
| 2015.01 | 141.9 | 137.3 | 93.0 | 89.3 (-2.9) | 9.46 |
| 2015.02 | 129.1 | 126.0 | 66.7 | 86.1 (-3.2) | 9.92 |
| 2015.03 | 125.9 | 124.6 | 54.5 | 82.2 (-3.9) | 16.14 |
| 2015.04 | 128.8 | 129.7 | 75.3 | 78.9 (-3.3) | 10.73 |
| 2015.05 | 120.0 | 122.6 | 88.8 | (76.3 projected, -2.6) | 8.29 |
| 2015.06 | 122.3 | 126.1 | 66.5 | (72.6 projected, -3.7) | 13.15 |
| 2015.07 | 107.0 | 110.8 | 66.4 | (68.9 projected, -3.7) | 8.83 |
| 2015.08 | 105.4 | 108.0 | 64.6 | (67.7 projected, -1.2) | 14.58 |
| 2015.09 | 101.7 | 102.7 | 78.1 | (68.0 projected, +0.3) | 15.78 |
| 2015.10 | 104.1 | 103.3 | 61.7 | (67.1 projected, -0.9) | 14.02 |
| 2015.11 | (119.4) | 12.3 (2A) / 92.5 (2B) / 82.2 (2C) | (65.0 projected, -2.1) | (16.8) | |
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) Updated to new data set from WDC-SILSO on July 1, 2015
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.
