SDO HMI 2014-08-15 03:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.50 | 47.85 | 9.05 | 27.95 | -17.49 | 104.86 | 21.08 | 220.48 | 0.5303 | 421.4 | 339.5 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.25 | 0.00 | 1.33 | -17.57 | 106.06 | 22.28 | 221.96 | 0.5426 | 595.0 | 426.5 | |
| 0.00 | 2.16 | 0.00 | 1.28 | -17.77 | 106.08 | 22.30 | 221.74 | 0.5450 | 423.0 | 374.6 | |
| 0.00 | 1.44 | 0.00 | 0.85 | -17.40 | 105.97 | 22.19 | 222.07 | 0.5399 | 564.0 | 478.1 | |
| 0.54 | 19.38 | 0.32 | 11.36 | -17.56 | 105.81 | 22.04 | 221.67 | 0.5401 | 820.2 | 692.5 | |
| 7.21 | -4.00 | 4.22 | -4.00 | -17.28 | 105.61 | 21.83 | 221.76 | 0.5352 | 991.8 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -20.13 | 105.58 | 21.80 | 218.22 | 0.5657 | 548.0 | 508.7 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -17.32 | 105.10 | 21.32 | 221.04 | 0.5307 | 445.0 | 379.0 | |
| 2.70 | 9.29 | 1.58 | 5.43 | -17.72 | 104.98 | 21.20 | 220.37 | 0.5338 | 940.4 | 569.6 | |
| 2.98 | -8.00 | 1.74 | -8.00 | -17.85 | 104.89 | 21.11 | 220.10 | 0.5344 | 852.6 | 999999 | |
| 2.07 | 3.79 | 1.19 | 2.17 | -16.58 | 103.25 | 19.47 | 219.47 | 0.5047 | -861.1 | -694.6 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -16.97 | 102.96 | 19.18 | 218.54 | 0.5063 | -676.0 | -487.8 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -17.16 | 102.77 | 19.00 | 218.04 | 0.5068 | -392.0 | -357.6 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -16.86 | 102.71 | 18.93 | 218.32 | 0.5027 | -897.0 | -719.0 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -18.45 | 102.68 | 18.90 | 216.30 | 0.5211 | 694.0 | 548.5 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -18.51 | 102.55 | 18.77 | 216.05 | 0.5207 | 743.0 | 584.3 | |
| 0.00 | 1.71 | 0.00 | 0.98 | -17.57 | 101.54 | 17.76 | 215.69 | 0.5006 | -389.0 | -395.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |