SDO HMI 2011-05-31 07:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.03 | 190.08 | 31.19 | 162.57 | -19.99 | 20.32 | -52.23 | 114.21 | 0.8164 | 237.7 | 176.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.72 | -19.21 | 23.41 | -49.13 | 114.17 | 0.7850 | -629.0 | -539.3 | |
| 5.69 | 13.10 | 4.46 | 10.30 | -17.58 | 23.74 | -48.80 | 112.25 | 0.7772 | -696.3 | -546.3 | |
| 0.00 | 0.99 | 0.00 | 0.80 | -19.34 | 22.96 | -49.58 | 114.19 | 0.7898 | -599.0 | -502.2 | |
| 2.89 | -2.00 | 2.28 | -2.00 | -17.80 | 23.47 | -49.08 | 112.44 | 0.7806 | -609.2 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.74 | -19.62 | 22.44 | -50.11 | 114.38 | 0.7956 | -472.0 | -373.1 | |
| 0.00 | 1.17 | 0.00 | 0.93 | -17.77 | 23.09 | -49.46 | 112.29 | 0.7844 | -302.0 | -236.8 | |
| 1.26 | 1.72 | 1.03 | 1.40 | -19.17 | 22.13 | -50.42 | 113.73 | 0.7975 | -612.4 | -587.4 | |
| 0.00 | 1.45 | 0.00 | 1.16 | -17.70 | 22.57 | -49.98 | 112.06 | 0.7894 | -519.0 | -335.8 | |
| 3.16 | 19.79 | 2.60 | 16.37 | -18.52 | 21.58 | -50.96 | 112.79 | 0.8011 | -642.3 | -240.4 | |
| 0.00 | 1.54 | 0.00 | 1.29 | -18.61 | 20.77 | -51.78 | 112.67 | 0.8091 | 310.0 | 219.1 | |
| 20.24 | 146.54 | 17.49 | 127.05 | -20.37 | 19.91 | -52.64 | 114.55 | 0.8213 | 952.2 | 283.0 | |
| 3.79 | -11.00 | 3.33 | -11.00 | -20.72 | 19.30 | -53.25 | 114.79 | 0.8276 | 550.8 | 999999 | |
| 0.00 | 1.17 | 0.00 | 1.07 | -21.89 | 18.17 | -54.37 | 115.84 | 0.8401 | 411.0 | 340.8 | |
| 0.00 | 0.81 | 0.00 | 0.74 | -19.64 | 17.68 | -54.86 | 113.11 | 0.8395 | -578.0 | -535.9 | |
| 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. | |