SDO HMI 2011-05-31 10:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.40 | 189.40 | 29.69 | 156.57 | -20.02 | 20.19 | -50.71 | 114.68 | 0.8023 | 238.3 | 230.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.33 | 8.40 | 4.06 | 6.39 | -17.56 | 23.65 | -47.26 | 112.70 | 0.7612 | -675.1 | -620.4 | |
| 0.00 | 1.08 | 0.00 | 0.84 | -19.31 | 22.95 | -47.95 | 114.68 | 0.7735 | -614.0 | -483.8 | |
| 3.34 | 4.25 | 2.56 | 3.25 | -17.81 | 23.42 | -47.49 | 112.95 | 0.7644 | -553.8 | -505.6 | |
| 0.00 | 1.08 | 0.00 | 0.85 | -19.37 | 22.73 | -48.17 | 114.69 | 0.7759 | -555.0 | -461.3 | |
| 0.00 | 0.72 | 0.00 | 0.57 | -19.59 | 22.40 | -48.50 | 114.86 | 0.7799 | -446.0 | -326.5 | |
| 0.00 | 1.17 | 0.00 | 0.93 | -19.30 | 22.08 | -48.82 | 114.39 | 0.7822 | -444.0 | -387.5 | |
| 0.00 | 0.99 | 0.00 | 0.77 | -17.71 | 22.59 | -48.31 | 112.56 | 0.7726 | -523.0 | -354.9 | |
| 3.16 | 19.87 | 2.52 | 15.94 | -18.56 | 21.54 | -49.37 | 113.30 | 0.7856 | -659.4 | -84.7 | |
| 0.00 | 0.54 | 0.00 | 0.43 | -18.30 | 21.29 | -49.61 | 112.91 | 0.7873 | -264.0 | -227.0 | |
| 24.57 | 147.60 | 20.55 | 123.37 | -20.41 | 19.73 | -51.17 | 115.02 | 0.8079 | 867.4 | 325.2 | |
| 0.00 | 1.90 | 0.00 | 1.67 | -22.05 | 18.05 | -52.85 | 116.47 | 0.8274 | 365.0 | 294.9 | |
| 0.00 | 1.08 | 0.00 | 0.93 | -19.69 | 18.54 | -52.36 | 113.82 | 0.8171 | 255.0 | 226.6 | |
| 0.00 | 0.72 | 0.00 | 0.63 | -19.71 | 17.62 | -53.29 | 113.60 | 0.8257 | -557.0 | -473.8 | |
| 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. | |