Last major update issued on March 14, 2011 at 04:55 UTC.
[Solar and geomagnetic data - last month (updated
daily)]
[Solar wind and electron fluence charts (updated
daily)
[Solar cycles 21-24 (last update March 2, 2011)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last
update March 2, 2011)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and
24 (last update March 2, 2011)]
[Historical solar and geomagnetic data charts 1954-2006
(last update April 5, 2007)]
[Archived reports since January 2003 (last update March
1, 2011)]
[POES auroral activity level charts since October
2009 - updated March 11, 2011]
Annotated geomagnetic activity charts - Carrington rotation 2105 [Dec-Jan.2011] - 2106 [Jan.-Feb.2011]
NEW
The geomagnetic field was quiet to unsettled on March 13 under the influence of a high speed stream from CH439.
Solar flux measured at 20h UTC on 2.8 GHz was 112.9 (increasing 0.3 over the last solar rotation). The planetary A index was 6 (STAR Ap - based on the mean of three hour interval ap indices: 6.0). Three hour interval K indices: 10021331 (planetary), 10122321 (Boulder).
The background x-ray flux is at the class B4 level.
At midnight UTC the visible solar disk had 6 spotted regions.
Region 11166 decayed quickly losing spots and penumbral area. Flares: C6.7 at 13:33, C6.4 at 14:42 UTC.
Region 11169 decayed further in the trailing spot section. The large
leading penumbra has a couple of small magnetic delta structures along its
southern edge. An M class
flare is possible. Flare: C1.7 at 21:59 UTC.
Region 11171 decayed slowly and could become spotless today.
Region 11172 didn't change significantly and was quiet.
Spotted regions not numbered by NOAA/SWPC:
[S902] This region was mostly unchanged on March 13.
Location at midnight: N07W04.
March 11-13: No obviously Earth directed CMEs were observed in LASCO and STEREO imagery.
Coronal hole history (since late 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.
The darkest areas on the solar disk are likely coronal holes.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over high and upper middle latitudes is poor. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet to unsettled on March 14 due to coronal hole effects and quiet on March 15-16.
| Coronal holes (1) | Coronal mass ejections (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 higher resolution image) 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 (blue-green) 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 polarity overlay |
Comment | |||
|---|---|---|---|---|---|---|---|---|---|---|
| SWPC | STAR SDO | SWPC | STAR | Current | Previous | |||||
| 11166 | 2011.03.02 | 14 | 21 | N10W65 | 0640 | EKC | EAC |
 |
 |
|
| 11169 | 2011.03.05 2011.03.06 |
17 | 27 | N20W34 | 0290 | CRO | CKO |
 |
 |
beta-delta |
| S898 | 2011.03.07 | S13W28 | plage | |||||||
| 11171 | 2011.03.08 | 2 | S19W01 | 0000 | BXO |
 |
 |
location of spots: S20W08 | ||
| S900 | 2011.03.08 | S18W38 |
 |
plage | ||||||
| S902 | 2011.03.10 | 3 | N07W04 | 0010 | BXO |
 |
 |
|||
| 11172 | 2011.03.10 2011.03.11 |
3 | 5 | N12E44 | 0020 | BXO | HRX |
 |
 |
|
| S904 | 2011.03.13 | 1 | S23E24 | 0000 | AXX |
 |
||||
| Total spot count: | 34 | 59 | ||||||||
| Sunspot number: | 64 | 119 | ||||||||
| Month | Average measured solar flux | International sunspot number (SIDC) | Smoothed sunspot number | Average ap (3) |
|---|---|---|---|---|
| 2008.07 | 65.7 (SF minimum) | 0.5 | 2.8 (-0.4) | |
| 2008.12 | 69.2 | 0.8 | 1.7 (-) sunspot minimum |
3.25 |
| 2009.12 | 76.7 | 10.8 | 8.3 (+0.7) | 1.41 / 1.92 |
| 2010.01 | 81.1 | 13.2 | 9.3 (+1.0) | 2.93 / 3.07 |
| 2010.02 | 84.7 | 18.8 | 10.6 (+1.3) | 4.15 / 4.61 |
| 2010.03 | 83.4 | 15.4 | 12.3 (+1.7) | 4.58 / 4.65 |
| 2010.04 | 75.9 | 8.0 | 14.0 (+1.7) | 10.22 / 10.24 |
| 2010.05 | 73.8 | 8.7 | 15.5 (+1.5) | 9.18 / 8.15 |
| 2010.06 | 72.5 | 13.6 | 16.4 (+0.9) | 8.17 / 6.85 |
| 2010.07 | 79.8 | 16.1 | 16.8 (+0.4) | 6.31 / 5.15 |
| 2010.08 | 79.2 | 19.6 | 17.4 (+0.6) | 8.49 / 7.77 |
| 2010.09 | 81.1 | 25.2 | (19.1 predicted, +1.7) | 5.33 / 5.45 |
| 2010.10 | 81.6 | 23.5 | (21.7 predicted, +2.6) | 6.07 / 6.27 |
| 2010.11 | 82.5 | 21.6 | (24.5 predicted, +2.8) | 4.80 / 5.50 |
| 2010.12 | 84.2 | 14.5 | (26.9 predicted, +2.4) | 3.41 / 4.35 |
| 2011.01 | 83.6 | 19.1 | (29.0 predicted, +2.1) | 4.32 |
| 2011.02 | 94.6 | 29.4 | (31.1 predicted, +2.1) | 5.41 |
| 2011.03 | 129.4 (1) | 41.5 (2A) / 99.1 (2B) | (33.0 predicted, +1.9) | (13.73) |
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 SIDC international sunspot number is typically 30-50% lower. 2B) Month
average to date.
3) Running average based on the preliminary daily SWPC ap indices.
Values in red are based on the official NGDC
ap indices.
This report has been prepared by Jan Alvestad. It is based on 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.
