Last major update issued on March 2, 2014 at 07:30 UTC.
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SSN Workshop, Tucson, 2013 (pdf)]
The geomagnetic field was quiet to unsettled on March 1. Solar wind speed at SOHO ranged between 351 and 402 km/s.
Solar flux at 20h UTC on 2.8 GHz was 164.6 (decreasing 25.2 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 153.9. The Potsdam WDC planetary A index was 6 (STAR Ap - based on the mean of three hour interval ap indices: 5.9). Three hour interval K indices: 21221113 (planetary), 11222222 (Boulder).
The background x-ray flux is at the class B7 level.
At the time of counting spots (see image time) spots were observed in 15 active regions in 2K resolution (SN: 339) and 14 active regions in 1K resolution (SN: 240) SDO images on the visible solar disk.
Region 11982 [S09W85] decayed slowly.
C5+ flare: M1.1 at 13:33 UTC.
Region 11986 [N14W51] decayed slowly and quietly.
Region 11987 [S01W32] decayed significantly in the
trailing and intermediate spot sections.
Region 11989 [N08W15] was quiet and stable.
Region 11990 [S12E13] decayed slowly and was mostly quiet as the magnetic
delta structure weakened.
Region 11991 [S24E27] developed as new flux emerged centrally. C and
minor M class flares are possible.
Region 11992 [S19W21] decayed slowly and quietly.
Region 11993 [N16E18] decayed slowly in the trailing and intermediate
spot sections and has polarity intermixing.
Region 11994 [S07W32] lost some small spots while the leader spot
increased its penumbral area.
Region 11995 [S17E06] was quiet and stable.
Spotted regions not numbered (or interpreted differently) by SWPC:
S3156 [N07W09] gained spots and was quiet.
S3163 [S09W08] was quiet and stable.
S3168 [S10W67] decayed slowly and quietly.
S3169 [N11E03] decayed slowly and quietly.
New region S3175 [N12E70] emerged with a few spots.
February 27 - March 1: 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 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. Propagation on long distance northeast-southwest paths is poor to fair.
The geomagnetic field is expected to be quiet to unsettled on March 2 and quiet on March 3-4.
| 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 | ||||||||||
| 11982 | 2014.02.16 2014.02.17 |
3 | 2 | 1 | S11W86 | 0050 | CAO | HRX |
 |
 |
location: S09W85 |
| 11986 | 2014.02.19 2014.02.20 |
3 | N14W55 | 0006 | AXX |
 |
 |
|
|||
| 11987 | 2014.02.21 | 16 | 23 | 12 | S02W29 | 0160 | ESI | DSI |
 |
 |
area: 0200 location: S01W32 |
| 11988 | 2014.02.21 2014.02.22 |
7 | S10W64 | 0170 | DAO |
plage location: S10W57 SWPC has adopted the spots of AR S3168 |
|||||
| S3150 | 2014.02.22 | S15W56 | plage | ||||||||
| 11989 | 2014.02.22 2014.02.23 |
7 | 10 | 4 | N07W13 | 0010 | BXO | CRO |
 |
 |
location: N08W15 |
| S3154 | 2014.02.23 | S27W58 | plage | ||||||||
| 11994 | 2014.02.23 2014.02.28 |
3 | 6 | 3 | S07W31 | 0030 | HAX | CAO |
 |
 |
area: 0070 |
| S3156 | 2014.02.23 | 12 | 7 | N07W09 | 0040 | AXX |
 |
 |
|||
| S3159 | 2014.02.24 | S22W55 | plage | ||||||||
| 11990 | 2014.02.24 | 9 | 16 | 9 | S14E11 | 0210 | DAC | DKC |
 |
 |
beta-delta area: 0420 location: S12E13 |
| 11991 | 2014.02.25 2014.02.26 |
10 | 28 | 18 | S25E26 | 0290 | EKO | EKC |
 |
 |
beta-gamma area: 0580 location: S24E27 |
| 11992 | 2014.02.25 2014.02.26 |
1 | 4 | 1 | S19W19 | 0020 | HSX | CRO |
 |
 |
location: S19W21 |
| S3163 | 2014.02.25 | 3 | 1 | S09W08 | 0010 | AXX |
 |
 |
|||
| S3164 | 2014.02.25 | N21E06 | |||||||||
| 11993 | 2014.02.25 2014.02.26 |
13 | 35 | 15 | N16E16 | 0110 | DAI | DAI |
 |
 |
beta-gamma location: N16E18
|
| S3166 | 2014.02.25 | N06W41 | plage | ||||||||
| S3168 | 2014.02.26 | 8 | 5 | S10W67 | 0180 | EAO |
 |
 |
AR 11988 for SWPC | ||
| S3169 | 2014.02.26 | 4 | 1 | N11E03 | 0012 | BXO |
 |
 |
|||
| S3171 | 2014.02.27 | N01W55 | plage | ||||||||
| 11995 | 2014.02.28 | 8 | 29 | 19 | S17E06 | 0060 | CAO | DRI |
 |
 |
area: 0080 |
| S3173 | 2014.02.28 | N15E35 |
 |
plage | |||||||
| S3174 | 2014.02.28 | S08W25 |
 |
plage | |||||||
| S3175 | 2014.03.01 | 6 | 4 | N12E70 | 0035 | CRO |
 |
||||
| Total spot count: | 77 | 189 | 100 | ||||||||
| Sunspot number: | 177 | 339 | 240 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 127 | 244 | 155 | (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): | 106 | 119 | 132 | 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 | ||||
| 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 (+3.5) | 8.27 |
| 2013.09 | 102.6 | 103.7 | 36.9 | (72.8 projected, +3.8) | 5.23 |
| 2013.10 | 132.1 | 131.2 | 85.6 | (73.8 projected, +1.0) | 7.71 |
| 2013.11 | 148.3 | 145.1 | 77.6 | (72.7 projected, -1.1) | 5.68 |
| 2013.12 | 147.7 | 143.1 | 90.3 | (71.6 projected, -1.1) | 4.68 |
| 2014.01 | 157.4 | 152.4 | 82.0 | (71.6 projected, 0.0) | 5.44 |
| 2014.02 | 170.3 (cycle peak) |
166.3 | 102.8 (cycle peak) | (70.9 projected, -0.7) | 10.8 |
| 2014.03 | 164.2 (1) | 5.7 (2A) / 177 (2B) / 120.6 (2C) | (71.0 projected, +0.1) | (5.9) | |
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.
