SDO HMI 2010-08-12 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 |
| 29.79 | 61.56 | 15.95 | 33.11 | 14.14 | 302.17 | -21.98 | 68.71 | 0.3910 | -150.0 | -20.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.67 | 9.84 | 4.06 | 5.21 | 14.17 | 304.58 | -19.56 | 66.69 | 0.3550 | -1017.3 | -674.0 | |
| 2.98 | 26.81 | 1.59 | 14.35 | 14.02 | 303.09 | -21.05 | 68.36 | 0.3766 | -1137.0 | -876.1 | |
| 2.44 | -2.00 | 1.30 | -2.00 | 14.39 | 303.02 | -21.12 | 67.49 | 0.3795 | -810.1 | 999999 | |
| 4.15 | -2.00 | 2.22 | -2.00 | 14.01 | 302.83 | -21.32 | 68.59 | 0.3805 | -1006.3 | 999999 | |
| 5.78 | -2.00 | 3.10 | -2.00 | 14.22 | 302.67 | -21.48 | 68.19 | 0.3839 | -854.8 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 14.61 | 301.78 | -22.36 | 67.91 | 0.3990 | -761.0 | -503.8 | |
| 0.00 | 1.26 | 0.00 | 0.68 | 13.58 | 301.28 | -22.87 | 70.75 | 0.4018 | 904.0 | 693.5 | |
| 0.00 | 1.99 | 0.00 | 1.08 | 13.85 | 301.08 | -23.06 | 70.23 | 0.4059 | 945.0 | 791.2 | |
| 6.77 | 12.28 | 3.68 | 6.67 | 13.58 | 300.60 | -23.55 | 71.16 | 0.4120 | 977.5 | 710.2 | |
| 0.00 | 1.72 | 0.00 | 0.94 | 15.10 | 300.22 | -23.92 | 67.90 | 0.4243 | 660.0 | 425.8 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 14.73 | 300.20 | -23.95 | 68.76 | 0.4230 | 745.0 | 573.7 | |
| 0.00 | 1.53 | 0.00 | 0.84 | 15.09 | 300.02 | -24.13 | 68.06 | 0.4273 | 1030.0 | 775.5 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 14.63 | 300.00 | -24.14 | 69.11 | 0.4254 | 380.0 | 378.3 | |
| 0.00 | 2.98 | 0.00 | 1.63 | 14.99 | 299.79 | -24.36 | 68.44 | 0.4302 | 783.0 | 636.8 | |
| 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. | |