SDO HMI 2014-01-13 21:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.30 | 233.12 | 33.29 | 120.70 | -17.85 | 30.20 | 10.27 | 215.82 | 0.2905 | 200.0 | 66.7 | |
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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 | 0.93 | 0.00 | 0.49 | -17.68 | 33.04 | 13.11 | 223.05 | 0.3181 | 757.0 | 597.6 | |
| 25.06 | 85.05 | 13.04 | 44.28 | -18.13 | 31.58 | 11.65 | 218.82 | 0.3076 | 1185.4 | 349.3 | |
| 4.67 | 34.24 | 2.42 | 17.74 | -17.31 | 31.37 | 11.44 | 220.13 | 0.2952 | 1202.1 | 708.7 | |
| 7.22 | -3.00 | 3.74 | -3.00 | -17.56 | 31.26 | 11.33 | 219.31 | 0.2970 | 1202.5 | 999999 | |
| 0.00 | 4.59 | 0.00 | 2.37 | -17.08 | 30.54 | 10.61 | 218.59 | 0.2835 | 816.0 | 723.7 | |
| 0.00 | 1.61 | 0.00 | 0.84 | -18.14 | 30.50 | 10.58 | 216.18 | 0.2969 | 836.0 | 625.1 | |
| 0.00 | 4.67 | 0.00 | 2.42 | -18.30 | 30.26 | 10.34 | 215.24 | 0.2966 | 740.0 | 736.8 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -15.98 | 29.60 | 9.68 | 218.74 | 0.2595 | 851.0 | 624.7 | |
| 1.95 | 61.51 | 1.01 | 31.72 | -17.46 | 29.30 | 9.38 | 214.44 | 0.2761 | -1174.3 | -425.4 | |
| 12.23 | -9.00 | 6.30 | -9.00 | -17.80 | 28.91 | 8.99 | 212.63 | 0.2771 | -1162.8 | 999999 | |
| 0.85 | 2.38 | 0.44 | 1.23 | -18.16 | 28.77 | 8.85 | 211.50 | 0.2810 | -893.6 | -732.8 | |
| 0.85 | 1.78 | 0.44 | 0.92 | -17.68 | 28.41 | 8.48 | 211.39 | 0.2710 | -1079.9 | -869.0 | |
| 11.47 | 34.83 | 5.90 | 17.91 | -17.81 | 27.94 | 8.02 | 209.75 | 0.2688 | -1263.1 | -558.1 | |
| 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. | |