Last major update issued on February 14, 2014 at 05:30 UTC.
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The geomagnetic field was very quiet on February 13. Solar wind speed at SOHO ranged between 313 and 397 km/s.
Solar flux at 20h UTC on 2.8 GHz was 166.6 (increasing 37.8 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 149.7. The Potsdam WDC planetary A index was 1 (STAR Ap - based on the mean of three hour interval ap indices: 1.3). Three hour interval K indices: 10010000 (planetary), 00011211 (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 in 2K resolution (SN: 289) and 9 active regions in 1K resolution (SN: 192) SDO images on the visible solar disk.
Region 11971 [S12W72] decayed slowly and quietly.
Region 11973 [N05W45] decayed quickly and was quiet.
Region 11974 [S12W32] was quiet and stable. SWPC is counting AR S3098 and
this group as one.
Region 11976 [S15E10] was quiet and stable.
Region 11977 [S10E38] developed slowly and could produce C and minor M
class flares.
Region 11978 [N05W67] decayed slowly and quietly.
Spotted regions not numbered (or interpreted differently) by SWPC:
S3098 [S12W24] is a large and complex region with major flare potential.
The region has become better organized over the last day with spots merging into
larger penumbrae, considerable decay was observed in the southeastern section.
There are several magnetic delta structures throughout the region with the most
complex layout in the northern trailing and central sections.
C5+ flares: M1.8 at 01:40, C5.4 at 02:18, C7.4 at
02:29, M1.0 at 02:51, M1.7 at 06:07, M1.0/1N at 08:12, C8.4 at 10:48, M1.4 at
15:57, C6.6 at 19:55 UTC.
S3105 [S14E21] was quiet and stable.
S3118 [N07W62] decayed slowly and quietly.
February 13: No obviously Earth directed CMEs were observed in LASCO and
STEREO imagery.
February 12: A slow symmetric full halo CME was observed after an M2
flare in AR S3098. The CME could reach Earth on February 15.
February 11: A partial halo CME was observed after 11h UTC following a
filament eruption near AR 11978 in the northwest quadrant. It is uncertain if
the CME has any Earth directed components.
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 holes 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 to fair. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet on February 14. Quiet to active conditions with a chance of minor storm intervals is possible on February 15-16 due to CME effects.
| 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: 0-20% probability, Yellow: 20-60% probability, Red: 60-100% 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 | STAR SDO | SWPC | STAR | Current | Previous | ||||||
| 2K | 1K | ||||||||||
| S3082 | 2014.02.01 | N08W56 | plage | ||||||||
| 11971 | 2014.02.03 2014.02.04 |
3 | 2 | 2 | S11W72 | 0040 | CSO | CRO |
 |
 |
|
| S3092 | 2014.02.04 | S08W58 | plage | ||||||||
| 11973 | 2014.02.04 2014.02.05 |
4 | 4 | 2 | N16W43 | 0030 | CSO | CAO |
 |
 |
SWPC location must be a typo real location: N05W45 |
| 11974 | 2014.02.04 2014.02.05 |
47 | 4 | 3 | S07W25 | 0780 | FKC | CAO |
 |
 |
location: S12W32 area: 0150 |
| S3096 | 2014.02.05 | N15W40 | plage | ||||||||
| S3098 | 2014.02.06 | 104 | 55 | S12W24 | 1220 | EKC |
 |
 |
gamma-delta SWPC has this as part of AR 11974 |
||
| 11976 | 2014.02.07 2014.02.08 |
15 | 31 | 14 | S15E13 | 0370 | FKI | DHO |
 |
 |
area: 0370 (SWPC area includes AR S3105) location: S15E23 |
| S3102 | 2014.02.08 | S19W35 |
 |
plage | |||||||
| S3105 | 2014.02.09 | 4 | 3 | S14E21 | 0190 | CSO |
 |
 |
SWPC has this as part of AR 11976 | ||
| S3106 | 2014.02.09 | N26W53 | plage | ||||||||
| 11977 | 2014.02.10 | 16 | 41 | 18 | S09E38 | 0460 | EKC | EKC |
 |
 |
area: 0580 |
| 11978 | 2014.02.10 2014.02.11 |
12 | 7 | 4 | N07W66 | 0030 | DAO | BXO |
 |
 |
location: N05W67 |
| S3110 | 2014.02.10 | S37W46 | plage | ||||||||
| S3111 | 2014.02.11 | N17W30 | plage | ||||||||
| S3112 | 2014.02.11 | S32E22 | plage | ||||||||
| S3113 | 2014.02.11 | N17W23 | plage | ||||||||
| S3114 | 2014.02.11 | N30W36 | plage | ||||||||
| 11979 | 2014.02.11 2014.02.12 |
N13W54 |
 |
plage | |||||||
| S3118 | 2014.02.12 | 2 | 1 | N07W62 | 0010 | CRO |
 |
 |
|||
| S3120 | 2014.02.12 | S25W17 |
 |
plage | |||||||
| S3121 | 2014.02.12 | S21W55 |
 |
plage | |||||||
| Total spot count: | 97 | 199 | 102 | ||||||||
| Sunspot number: | 157 | 289 | 192 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 142 | 250 | 153 | (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): | 94 | 101 | 106 | k * (sunspot number). k = 0.6 for SWPC, k = 0.35 for STAR SDO 2K, k = 0.55 for STAR SDO 1K | |||||||
| Month | Average solar flux | International sunspot number (WDC-SILSO) |
Smoothed sunspot number | Average ap (3) |
|
|---|---|---|---|---|---|
| Measured | 1 AU | ||||
| 2011.11 | 153.5 | 96.7 (cycle peak) | 61.1 (+1.2) | 5.55 | |
| 2012.02 | 106.5 | 32.9 | 66.9 (+1.4) | 8.81 | |
| 2012.11 | 121.3 | 118.3 | 61.8 | 59.7 (+1.1) | 7.08 |
| 2012.12 | 108.6 | 105.0 | 40.8 | 59.6 (-0.1) | 3.44 |
| 2013.01 | 127.1 | 123.1 | 62.9 | 58.7 (-0.9) | 4.69 |
| 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 projected, +3.5) | 8.27 |
| 2013.09 | 102.6 | 103.7 | 36.9 | (73.0 projected, +4.0) | 5.23 |
| 2013.10 | 132.1 | 131.2 | 85.6 | (74.0 projected, +1.0) | 7.71 |
| 2013.11 | 148.3 | 145.1 | 77.6 | (72.9 projected, -1.1) | 5.68 |
| 2013.12 | 147.7 | 143.1 | 90.3 | (71.8 projected, -1.1) | 4.68 |
| 2014.01 | 157.4 (cycle peak) |
152.4 | 82.0 | (71.0 projected, -0.8) | 5.44 |
| 2014.02 | 177.4 (1) | 83.6 (2A) / 180.2 (2B) / 107.9 (2C) | (71.2 projected, +0.2) | (7.4) | |
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 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.
