SDO HMI 2014-01-10 10:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.35 | 71.00 | 20.53 | 49.98 | 16.83 | 24.88 | -40.61 | 61.35 | 0.7121 | 215.1 | 243.8 | |
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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 |
| 0.34 | 1.36 | 0.22 | 0.90 | 15.20 | 28.56 | -36.93 | 61.40 | 0.6628 | 513.2 | 475.4 | |
| 5.27 | 7.74 | 3.51 | 5.16 | 15.84 | 28.11 | -37.37 | 60.79 | 0.6714 | -849.0 | -627.6 | |
| 0.60 | 1.45 | 0.40 | 0.97 | 15.30 | 27.07 | -38.42 | 62.15 | 0.6803 | -694.1 | -591.2 | |
| 0.00 | 1.19 | 0.00 | 0.80 | 15.25 | 26.80 | -38.69 | 62.37 | 0.6831 | -654.0 | -562.8 | |
| 4.51 | 44.63 | 3.18 | 31.74 | 17.31 | 24.94 | -40.55 | 60.70 | 0.7140 | 874.7 | 452.3 | |
| 11.14 | -5.00 | 7.92 | -5.00 | 17.27 | 24.38 | -41.11 | 61.06 | 0.7198 | 951.6 | 999999 | |
| 0.94 | 1.96 | 0.65 | 1.37 | 15.85 | 24.71 | -40.78 | 62.72 | 0.7093 | -561.5 | -407.1 | |
| 2.81 | 3.91 | 1.96 | 2.73 | 15.50 | 24.71 | -40.78 | 63.17 | 0.7077 | -784.5 | -644.1 | |
| 2.21 | -5.00 | 1.58 | -5.00 | 17.33 | 23.95 | -41.54 | 61.22 | 0.7246 | 551.8 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.80 | 17.28 | 23.55 | -41.94 | 61.49 | 0.7286 | 562.0 | 497.5 | |
| 0.00 | 1.36 | 0.00 | 0.97 | 15.68 | 23.64 | -41.85 | 63.49 | 0.7202 | -597.0 | -527.4 | |
| 0.00 | 1.53 | 0.00 | 1.10 | 16.95 | 23.26 | -42.22 | 62.05 | 0.7301 | 334.0 | 333.2 | |
| 1.53 | 3.74 | 1.11 | 2.71 | 17.21 | 23.11 | -42.38 | 61.80 | 0.7329 | 716.1 | 560.3 | |
| 0.00 | 1.02 | 0.00 | 0.73 | 15.66 | 23.44 | -42.05 | 63.61 | 0.7222 | -481.0 | -416.8 | |
| 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. | |