The geomagnetic field was quiet to unsettled on August 6, after 06h UT under the influence of effects from a high speed stream associated with CH680 (no co-rotating interaction region signature was observed). Solar wind speed at SOHO ranged between 349 and 602 km/s.
Solar flux at 17h UTC on 2.8 GHz was 116.9 (decreasing 12.1 over the last solar rotation, the measurement at 20h UT was enhanced by a C1.6 flare peaking at 19:58 UT with an origin in the northern part of AR 12396). The 90 day 10.7 flux at 1 AU was 118.4. The Potsdam WDC planetary A index was 10 (STAR Ap - based on the mean of three hour interval ap indices: 10.0). Three hour interval K indices: 21233223 (planetary), 31353223 (Boulder).
The background x-ray flux is at the class B4 level.
At the time of counting spots (see image time), spots were observed in 13 active regions using 2K resolution (SN: 228) and 9 active regions using 1K resolution (SN: 130) SDO images on the visible solar disk.
Region 12393 [N18W45] decayed slowly and quietly.
Region 12394 [N12W22] was quiet and stable.
Region 12395 [N12E27] decayed quietly.
Region 12396 [S18E16] developed gaining spots and penumbral area. There's weak polarity intermixing in the central section.
An M class flare is possible.
Region 12397 [S12W55] decayed losing the trailing spots.
Spotted regions not numbered (or interpreted differently) by SWPC:
S4648 [S23W35] was quiet and stable.
S4667 [S18E41] reemerged with penubra spots.
New region S4669 [N15E75] rotated into view.
New region S4670 [N22E34] emerged with a penumbra spot.
New region S4671 [N08W26] was split off from AR 12394.
New region S4672 [S15W31] emerged with penumbra spots.
New region S4673 [N05E03] emerged with a penumbra
spot.
New region S4674 [N19W64] emerged with penumbra spots.
C2+ flares:
| Magnitude | Peak time (UTC) | Location | AR | Recorded by | Comment |
| C2.1 | 19:21 | S17E34 | 12396 | GOES15 |
August 4-6: No obviously Earth directed CMEs were observed.
[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 (CH680) was in an Earth facing position on August 3. A small coronal hole (CH681) near the equator was in an Earth facing location on August 6 and may be capable of causing a weak disturbance on August 9-10.
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 August 7-8 due to a high speed stream associated with CH680 and quiet on August 9-10. Effects from a small coronal hole (CH681) could reach Earth on August 9 and cause a few unsettled intervals.
| 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 | ||||||||||
| 12391 | 2015.07.26 2015.07.27 |
N07W62 |
 |
||||||||
| 12392 | 2015.07.27 2015.07.29 |
S05W67 | location: S05W54 | ||||||||
| 12393 | 2015.07.27 2015.07.30 |
1 | 3 | 1 | N18W46 | 0020 | HAX | CRO |
 |
 |
|
| S4648 | 2015.07.28 | 2 | S23W35 | 0003 | AXX |
 |
 |
||||
| 12394 | 2015.07.29 2015.07.30 |
6 | 19 | 7 | N11W25 | 0100 | CAO | DAO |
 |
 |
area: 0190 |
| S4653 | 2015.07.30 | S25W57 | |||||||||
| S4655 | 2015.08.01 | N33W21 | |||||||||
| S4656 | 2015.08.01 | S06W42 | |||||||||
| 12395 | 2015.08.02 2015.08.03 |
1 | 4 | 2 | N12E25 | 0020 | HAX | CRO |
 |
 |
|
| S4660 | 2015.08.02 | N06W37 | |||||||||
| 12396 | 2015.08.03 | 20 | 52 | 22 | S17E15 | 0550 | EKC | EKC |
 |
 |
area: 1020 |
| S4663 | 2015.08.03 | S10W03 | |||||||||
| S4664 | 2015.08.03 | S18W02 | |||||||||
| 12397 | 2015.08.03 2015.08.05 |
1 | 2 | 1 | S12W54 | 0010 | HAX | HRX |
 |
 |
|
| S4667 | 2015.08.04 | 2 | S18E41 | 0003 | AXX |
 |
|||||
| S4668 | 2015.08.05 | S27W21 |
 |
||||||||
| S4669 | 2015.08.06 | 1 | 1 | N15E75 | 0030 | HRX |
 |
||||
| S4670 | 2015.08.06 | 1 | 1 | N22E34 | 0003 | AXX |
 |
||||
| S4671 | 2015.08.06 | 7 | 4 | N08W26 | 0018 | CRO |
 |
||||
| S4672 | 2015.08.06 | 2 | S15W31 | 0003 | BXO |
 |
|||||
| S4673 | 2015.08.06 | 1 | 1 | N05E03 | 0003 | AXX |
 |
||||
| S4674 | 2015.08.06 | 2 | N19W64 | 0002 | BXO |
 |
|||||
| Total spot count: | 29 | 98 | 40 | ||||||||
| Sunspot number: | 79 | 228 | 130 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 59 | 128 | 70 | (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): | 87 | 125 | 111 | 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 |
| 2014.03 | 149.9 | 148.5 | 128.7 | 114.3 (+3.8) | 4.88 |
| 2014.04 | 143.9 | 144.8 | 112.5 | 116.4 (+2.1) (solar max) | 7.88 |
| 2014.05 | 129.7 | 132.9 | 112.5 | 115.0 (-1.4) | 5.75 |
| 2014.06 | 122.0 | 125.8 | 102.9 | 114.1 (-0.9) | 6.72 |
| 2014.07 | 137.4 | 141.8 | 100.2 | 112.6 (-1.5) | 4.50 |
| 2014.08 | 124.7 | 127.9 | 106.9 | 108.3 (-4.3) | 7.71 |
| 2014.09 | 146.6 | 148.1 | 130.0 | 101.9 (-6.4) | 9.78 |
| 2014.10 | 153.4 | 152.9 | 90.0 | 97.4 (-4.5) | 8.96 |
| 2014.11 | 154.8 | 151.4 | 103.6 | 95.0 (-2.4) | 9.33 |
| 2014.12 | 158.7 | 153.8 | 112.9 | 92.6 (-2.4) | 11.24 |
| 2015.01 | 141.9 | 137.3 | 93.0 | 89.8 (-2.8) | 9.46 |
| 2015.02 | 129.1 | 126.0 | 66.7 | (86.8 projected, -3.0) | 9.92 |
| 2015.03 | 125.9 | 124.6 | 54.5 | (83.1 projected, -3.7) | 16.14 |
| 2015.04 | 128.8 | 129.7 | 78.0 | (79.8 projected, -3.3) | 10.73 |
| 2015.05 | 120.0 | 122.6 | 90.0 | (77.4 projected, -2.4) | 8.29 |
| 2015.06 | 122.3 | 126.1 | 68.3 | (73.9 projected, -3.5) | 13.15 |
| 2015.07 | 107.0 | 110.8 | 66.4 | (70.2 projected, -3.7) | 8.8 |
| 2015.08 | (107.7) | 13.5 (2A) / 69.5 (2B) / 77.3 (2C) | (69.0 projected, -1.2) | (7.0) | |
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.
