SDO HMI 2011-10-05 08:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.13 | 213.09 | 23.78 | 114.82 | -11.72 | 178.52 | -14.38 | 141.97 | 0.3954 | 426.3 | 274.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.90 | 184.43 | 1.56 | 98.96 | -11.97 | 179.46 | -13.44 | 144.08 | 0.3893 | 881.3 | 414.8 | |
| 1.32 | -1.00 | 0.71 | -1.00 | -11.91 | 179.24 | -13.66 | 143.56 | 0.3906 | 741.9 | 999999 | |
| 33.14 | -1.00 | 17.79 | -1.00 | -11.54 | 179.13 | -13.77 | 142.75 | 0.3868 | 1232.5 | 999999 | |
| 1.32 | 1.67 | 0.71 | 0.90 | -12.19 | 178.50 | -14.40 | 142.52 | 0.4013 | 544.3 | 486.0 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -12.26 | 178.14 | -14.75 | 141.97 | 0.4056 | 442.0 | 278.0 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -12.68 | 176.91 | -15.99 | 140.36 | 0.4231 | -862.0 | -785.4 | |
| 1.23 | 4.04 | 0.67 | 2.21 | -12.79 | 176.58 | -16.32 | 139.95 | 0.4276 | -870.3 | -844.7 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -13.15 | 176.27 | -16.63 | 139.97 | 0.4351 | -744.0 | -556.2 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -12.14 | 174.34 | -18.56 | 135.26 | 0.4439 | -953.0 | -660.2 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -12.44 | 173.96 | -18.94 | 135.16 | 0.4513 | -698.0 | -631.2 | |
| 1.41 | 5.54 | 0.78 | 3.07 | -12.10 | 173.66 | -19.24 | 134.17 | 0.4510 | -1036.1 | -765.3 | |
| 2.81 | 3.69 | 1.56 | 2.05 | -12.58 | 173.59 | -19.31 | 134.83 | 0.4569 | -972.4 | -880.8 | |
| 0.00 | 1.41 | 0.00 | 0.79 | -13.38 | 173.39 | -19.50 | 135.79 | 0.4677 | -893.0 | -678.6 | |
| 0.00 | 2.29 | 0.00 | 1.28 | -13.03 | 173.36 | -19.54 | 135.20 | 0.4643 | -971.0 | -725.8 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -12.65 | 173.36 | -19.54 | 134.60 | 0.4602 | -862.0 | -728.0 | |
| 0.00 | 1.41 | 0.00 | 0.79 | -12.79 | 172.95 | -19.94 | 134.24 | 0.4662 | -661.0 | -493.2 | |
| 0.00 | 2.11 | 0.00 | 1.18 | -11.81 | 172.25 | -20.65 | 131.67 | 0.4640 | -704.0 | -503.5 | |
| 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. | |