SDO HMI 2011-10-08 14:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.43 | 241.88 | 19.46 | 125.83 | 23.39 | 155.03 | 5.01 | 344.69 | 0.3065 | -826.9 | -383.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.51 | 24.35 | 157.12 | 7.10 | 340.05 | 0.3314 | -791.0 | -635.4 | |
| 8.15 | 218.04 | 4.24 | 113.35 | 23.08 | 155.58 | 5.56 | 342.85 | 0.3035 | -1340.9 | -433.7 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 26.68 | 155.68 | 5.66 | 345.81 | 0.3609 | -813.0 | -587.0 | |
| 28.93 | -2.00 | 15.04 | -2.00 | 23.30 | 155.23 | 5.21 | 344.09 | 0.3054 | -1414.4 | 999999 | |
| 0.00 | 3.24 | 0.00 | 1.68 | 22.31 | 154.70 | 4.68 | 344.68 | 0.2871 | -898.0 | -764.3 | |
| 0.00 | 2.45 | 0.00 | 1.27 | 22.85 | 153.06 | 3.04 | 350.26 | 0.2900 | 641.0 | 501.8 | |
| 0.00 | 1.93 | 0.00 | 1.00 | 24.20 | 152.86 | 2.84 | 351.62 | 0.3117 | -993.0 | -762.5 | |
| 0.35 | 3.95 | 0.18 | 2.06 | 24.73 | 152.54 | 2.52 | 352.79 | 0.3198 | -988.8 | -784.2 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 26.39 | 152.14 | 2.12 | 354.47 | 0.3462 | 739.0 | 604.3 | |
| 0.00 | 3.33 | 0.00 | 1.76 | 26.19 | 152.04 | 2.02 | 354.69 | 0.3429 | 933.0 | 609.6 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 26.04 | 151.74 | 1.72 | 355.44 | 0.3399 | 818.0 | 710.6 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 23.67 | 151.05 | 1.03 | 356.84 | 0.2999 | 837.0 | 605.1 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 25.56 | 150.40 | 0.38 | 358.95 | 0.3310 | 930.0 | 772.5 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 25.07 | 145.54 | -4.48 | 12.41 | 0.3308 | 708.0 | 597.3 | |
| 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. | |