Last major update issued on June 7, 2014 at 05:30 UTC.
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4th SSN Workshop, Locarno, 2014]
The geomagnetic field was quiet on June 6. Solar wind speed at SOHO ranged between 333 and 350 km/s.
Solar flux at 20h UTC on 2.8 GHz was 133.0 (decreasing 19.1 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 139.2. The Potsdam WDC planetary A index was 4 (STAR Ap - based on the mean of three hour interval ap indices: 4.0). Three hour interval K indices: 21001212 (planetary), 21012322 (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: 292) and 13 active regions using 1K resolution (SN: 221) SDO images on the visible solar disk.
Region 12077 [S03W22] developed significantly and
could produce C flares.
Region 12079 [N12E00] was quiet and stable.
Region 12080 [S12E18] developed further and has 2 magnetic delta
structures in the trailing spot section. Further M class flaring is possible.
Region 12081 [N05E10] was quiet and stable.
Region 12082 [N17E27] developed quickly and could produce M class flares.
Region 12083 [S12W77] decayed slowly and quietly.
New region 12084 [S11W12] emerged with several spots.
New region 12085 [S20E25] emerged on June 5 and developed quickly on June
6 when it was numbered by SWPC. A minor M class flare is possible.
Spotted regions not numbered (or interpreted differently) by SWPC:
S3492 [N11W23] reemerged with penumbra spots.
S3499 [S10E09] reemerged with penumbra spots.
New region S3507 [N12W11] was observed with a
penumbra spot.
New region S3509 [S15W68] emerged with penumbra spots.
New region S3510 [S12E35] was observed with penumbra spots.
| Magnitude | Time (UTC) | Location | AR |
| C3.6 | 13:11 | S12E25 | 12080 |
| C2.0 | 13:27 | 12080 | |
| M1.4 | 19:31 | S12E25 | 12080 |
| C3.4 | 22:25 | S13E23 | 12080 |
June 5-6: No obviously Earth directed CMEs were observed in LASCO and
STEREO imagery.
June 4: A large filament eruption in the southeast quadrant during the
evening was associated with an asymmetric full halo CME.
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
An extension (CH621) of a large southern hemisphere coronal hole may have been in an Earth facing position on June 6. A small trans equatorial coronal hole (CH622) could rotate into an Earth facing position on June 8.
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.
The geomagnetic field is expected to be quiet to active on June 7-8 due to effects from the June 4 CME. Mostly quiet conditions are likely on June 9.
| 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. 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 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 overlay |
Comment | ||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| SWPC | Magnetic (SDO) |
SWPC | STAR | Current | Previous | ||||||
| 2K | 1K | ||||||||||
| 12077 | 2014.05.30 | 7 | 19 | 11 | S04W24 | 0090 | DSO | DAI |
 |
 |
area: 0190 location: S03W22 |
| 12078 | 2014.05.30 2014.06.01 |
1 | S20W57 | 0000 | AXX |
spotless real location: S19W53 |
|||||
| 12079 | 2014.05.31 2014.06.01 |
1 | 8 | 5 | N12W00 | 0090 | HSX | HSX |
 |
 |
area: 0180 |
| S3492 | 2014.05.31 | 3 | 2 | N11W23 | 0010 | BXO |
 |
||||
| 12081 | 2014.06.01 2014.06.04 |
4 | 2 | N05E04 | 0010 | BXO |
 |
 |
|||
| S3495 | 2014.06.01 | S10W40 | plage | ||||||||
| S3496 | 2014.06.02 | N17W00 | plage | ||||||||
| 12080 | 2014.06.02 2014.06.03 |
15 | 42 | 20 | S12E18 | 0160 | DAI | EAC |
 |
 |
beta-gamma-delta area: 0320 |
| S3499 | 2014.06.03 | 4 | 3 | S10E09 | 0010 | AXX |
 |
||||
| S3500 | 2014.06.04 | S21W57 |
 |
plage | |||||||
| S3501 | 2014.06.04 | S23E16 |
 |
plage | |||||||
| S3502 | 2014.06.04 | S12W01 | plage | ||||||||
| 12082 | 2014.06.04 2014.06.05 |
18 | 26 | 16 | N17E26 | 0170 | DAC | DKC |
 |
 |
area: 0500 |
| 12083 | 2014.06.04 2014.06.05 |
2 | 3 | 2 | S12W76 | 0010 | BXO | CRO |
 |
 |
|
| S3505 | 2014.06.05 | S15E46 |
 |
||||||||
| 12085 | 2014.06.05 2014.06.06 |
6 | 29 | 16 | S21E24 | 0020 | DRI | DAC |
 |
 |
|
| 12084 | 2014.06.06 | 2 | 15 | 8 | S12W13 | 0010 | BXO | DRI |
 |
||
| S3507 | 2014.06.06 | 1 | 1 | N12W11 | 0004 | AXX |
 |
||||
| S3509 | 2014.06.06 | 4 | 2 | S15W68 | 0012 | BXO |
 |
||||
| S3510 | 2014.06.06 | 4 | 3 | S12E35 | 0010 | AXX |
 |
||||
| Total spot count: | 52 | 162 | 91 | ||||||||
| Sunspot number: | 132 | 292 | 221 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 85 | 198 | 127 | (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): | 79 | 102 | 122 | k * (sunspot number). k = 0.6 for SWPC, k = 0.35 for MSN 2K, k = 0.55 for MSN 1K (MSN=Magnetic Sunspot Number) | |||||||
| Month | Average solar flux | International sunspot number (WDC-SILSO) |
Smoothed sunspot number | Average ap (3) |
|
|---|---|---|---|---|---|
| Measured | 1 AU | ||||
| 2013.02 | 104.3 | 101.8 | 38.0 | 58.4 (-0.3) | 6.11 |
| 2013.03 | 111.3 | 110.2 | 57.9 | 57.5 (-0.9) | 10.56 |
| 2013.04 | 124.8 | 125.9 | 72.4 | 57.9 (+0.4) | 5.40 |
| 2013.05 | 131.4 | 134.3 | 78.7 | 59.9 (+2.0) | 9.73 |
| 2013.06 | 110.1 | 113.7 | 52.5 | 62.6 (+2.7) | 12.60 |
| 2013.07 | 115.5 | 119.3 | 57.0 | 65.5 (+2.9) | 9.47 |
| 2013.08 | 114.6 | 118.3 | 66.0 | 69.0 (+3.5) | 8.27 |
| 2013.09 | 102.6 | 103.7 | 36.9 | 73.1 (+4.1) | 5.23 |
| 2013.10 | 132.1 | 131.2 | 85.6 | 75.0 (+1.9) | 7.71 |
| 2013.11 | 148.3 | 145.1 | 77.6 | 75.4 (+0.4) | 5.68 |
| 2013.12 | 147.7 | 143.1 | 90.3 | (75.8 projected, +0.4) | 4.68 |
| 2014.01 | 157.4 | 152.4 | 82.0 | (76.4 projected, +0.6) | 5.44 |
| 2014.02 | 170.3 (cycle peak) |
166.3 | 102.8 (cycle peak) | (76.2 projected, -0.2) | 10.70 |
| 2014.03 | 149.9 | 148.5 | 92.2 | (76.6 projected, +0.4) | 4.88 |
| 2014.04 | 143.9 | 144.8 | 84.7 | (75.8 projected, -0.8) | 7.88 |
| 2014.05 | 129.7 | 132.9 | 75.2 | (73.2 projected, -2.6) | 5.75 |
| 2014.06 | 114.5 (1) | 20.8 (2A) / 92.0 (2B) / 88.0 (2C) | (70.5 projected, -2.7) | (5.8) | |
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). The
official WDC-SILSO international sunspot number is typically 30-50% lower. 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.
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 the UTC day. Comments and suggestions are always welcome.
SDO images are courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.
