Last major update issued on June 15, 2014 at 05:40 UTC.
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The geomagnetic field was quiet on June 14. Solar wind speed at SOHO ranged between 352 and 452 km/s.
Solar flux at 20h UTC on 2.8 GHz was 143.5 (increasing 16.0 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 140.7. The Potsdam WDC planetary A index was 6 (STAR Ap - based on the mean of three hour interval ap indices: 5.5). Three hour interval K indices: 22211121 (planetary), 23322322 (Boulder).
The background x-ray flux is at the class C1 level.
At the time of counting spots (see image time), spots were observed in 9 active regions using 2K resolution (SN: 171) and 7 active regions using 1K resolution (SN: 113) SDO images on the visible solar disk.
Region 12082 [N14W82] rotated quietly to the
northwest limb.
Region 12085 [S19W85] decayed slowly, however, there is a chance of a
major flare while the region is at the southwest limb and just behind the limb.
Region 12087 [S18E18] decayed quickly losing all negative polarity umbrae.
Region 12088 [S10W75] decayed slowly and quietly.
Region 12089 [N18W25] developed as new flux emerged.
C and minor M class flares are possible.
Region 12090 [N25E29] was quiet and stable.
Region 12091 [S11W30] decayed slowly and quietly.
Region 12092 [S20E32] was quiet and stable.
Spotted regions not numbered (or interpreted differently) by SWPC:
S3532 [S29E00] was quiet and stable.
| Magnitude | Time (UTC) | Location | AR |
| C2.4 | 03:48 | S20W70 | 12085 |
| C3.6 (LDE) | 09:46 | S17E30 | 12087 |
| C3.3 | 17:47 | 12089 | |
| M1.4 | 19:29 | SE limb | |
| C2.1 | 23:10 | 12080 |
June 12: At least a partial halo CME was observed after the M3 LDE in AR
12085 late in the day.
June 13-14: No obviously Earth directed CMEs were observed in LASCO and
STEREO 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 hole are currently in or near Earth facing positions.
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 mostly quiet on June 15-17 with a chance of unsettled and active intervals on June 15-16 if the June 13 CME reaches Earth.
| 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 | ||||||||||
| 12080 | 2014.06.02 2014.06.03 |
8 | S11W91 | 0350 | DKI |
 |
rotated out of view |
||||
| 12082 | 2014.06.04 2014.06.05 |
2 | 3 | 2 | N15W80 | 0140 | CAO | DAO |
 |
 |
area: 0250 |
| 12085 | 2014.06.05 2014.06.06 |
13 | 2 | 1 | S19W84 | 0200 | EAI | CAO |
 |
 |
|
| 12088 | 2014.06.06 2014.06.11 |
1 | 1 | S09W74 | 0020 | HRX | AXX |
 |
 |
area: 0010 | |
| 12089 | 2014.06.07 2014.06.11 |
10 | 30 | 19 | N18W25 | 0100 | DAI | DAC |
 |
 |
|
| S3515 | 2014.06.07 | S13W50 | plage | ||||||||
| S3516 | 2014.06.07 | N22W28 | plage | ||||||||
| 12086 | 2014.06.08 | N01W47 | |||||||||
| S3522 | 2014.06.08 | S20W39 |
 |
plage | |||||||
| 12087 | 2014.06.09 2014.06.10 |
24 | 16 | 10 | S18E16 | 0180 | DAI | CSO |
 |
 |
|
| S3524 | 2014.06.09 | S16W23 | plage | ||||||||
| 12090 | 2014.06.10 2014.06.11 |
3 | 7 | 4 | N24E30 | 0120 | CSO | ESO |
 |
 |
area: 0200 |
| 12091 | 2014.06.11 2014.06.12 |
2 | 4 | S08W29 | 0000 | AXX | AXX |
 |
 |
||
| 12092 | 2014.06.11 2014.06.12 |
6 | 15 | 6 | S19E33 | 0010 | BXO | CRI |
 |
 |
area: 0030 |
| S3531 | 2014.06.11 | S22E23 | plage | ||||||||
| S3532 | 2014.06.11 | 3 | 1 | S29E00 | 0007 | AXX |
 |
 |
|||
| S3535 | 2014.06.12 | N01W44 | plage | ||||||||
| S3536 | 2014.06.13 | N18W24 |
 |
plage | |||||||
| S3537 | 2014.06.13 | S19W12 |
 |
plage | |||||||
| Total spot count: | 69 | 81 | 43 | ||||||||
| Sunspot number: | 159 | 171 | 113 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 107 | 109 | 71 | (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 | 60 | 62 | 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 | 136.9 (1) | 63.2 (2A) / 135.4 (2B) / 84.2 (2C) | (70.5 projected, -2.7) | (7.6) | |
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.
