SDO HMI 2011-08-09 18:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.35 | 31.04 | 1.19 | 15.82 | 19.35 | 224.17 | 3.98 | 344.01 | 0.2371 | -589.8 | -641.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 0.97 | 19.57 | 225.93 | 5.75 | 337.66 | 0.2493 | -1175.0 | -1023.0 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 20.48 | 225.67 | 5.49 | 339.91 | 0.2620 | -902.0 | -695.0 | |
| 0.00 | 8.66 | 0.00 | 4.43 | 19.79 | 225.49 | 5.30 | 339.56 | 0.2501 | -495.0 | -813.2 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 20.13 | 225.43 | 5.25 | 340.25 | 0.2552 | -911.0 | -756.0 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 18.40 | 224.38 | 4.20 | 341.66 | 0.2216 | -965.0 | -645.0 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 19.02 | 224.27 | 4.08 | 342.99 | 0.2311 | -1071.0 | -823.1 | |
| 0.00 | 2.71 | 0.00 | 1.37 | 18.31 | 224.16 | 3.97 | 342.45 | 0.2190 | -952.0 | -777.5 | |
| 0.00 | 1.81 | 0.00 | 0.92 | 20.43 | 224.18 | 3.99 | 345.03 | 0.2536 | -797.0 | -647.7 | |
| 0.00 | 2.98 | 0.00 | 1.51 | 18.59 | 223.74 | 3.56 | 344.53 | 0.2216 | -715.0 | -714.5 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 18.31 | 223.64 | 3.46 | 344.60 | 0.2165 | -958.0 | -745.4 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 20.82 | 221.88 | 1.69 | 353.72 | 0.2529 | -909.0 | -734.3 | |
| 2.35 | 3.61 | 1.19 | 1.83 | 19.13 | 221.47 | 1.29 | 354.54 | 0.2236 | 935.2 | 700.4 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.85 | 221.31 | 1.12 | 355.11 | 0.2186 | 958.0 | 708.1 | |
| 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. | |