SDO HMI 2011-01-01 02:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.57 | 180.70 | 33.66 | 115.86 | 34.04 | 267.61 | 13.90 | 341.69 | 0.6366 | 54.7 | -47.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.82 | 99.14 | 10.81 | 63.80 | 33.57 | 269.79 | 16.08 | 338.77 | 0.6397 | -1045.9 | -307.2 | |
| 0.76 | -1.00 | 0.49 | -1.00 | 33.79 | 269.53 | 15.83 | 339.22 | 0.6411 | -773.4 | 999999 | |
| 1.44 | -1.00 | 0.92 | -1.00 | 33.34 | 269.27 | 15.56 | 339.24 | 0.6344 | -882.9 | 999999 | |
| 2.72 | 4.67 | 1.74 | 2.99 | 33.59 | 268.72 | 15.02 | 340.05 | 0.6349 | -744.2 | -626.0 | |
| 0.00 | 1.36 | 0.00 | 0.88 | 34.25 | 268.40 | 14.69 | 340.85 | 0.6416 | -515.0 | -387.0 | |
| 0.00 | 1.95 | 0.00 | 1.25 | 34.53 | 266.83 | 13.12 | 342.90 | 0.6384 | -860.0 | -640.0 | |
| 0.00 | 1.53 | 0.00 | 0.98 | 34.71 | 266.53 | 12.82 | 343.37 | 0.6395 | -589.0 | -458.2 | |
| 0.00 | 1.02 | 0.00 | 0.64 | 33.15 | 265.57 | 11.86 | 343.71 | 0.6158 | 591.0 | 557.8 | |
| 1.61 | 7.65 | 1.01 | 4.80 | 33.36 | 264.84 | 11.13 | 344.76 | 0.6158 | 935.2 | 679.4 | |
| 0.00 | 3.65 | 0.00 | 2.34 | 34.80 | 265.00 | 11.29 | 345.28 | 0.6352 | 510.0 | 478.5 | |
| 1.78 | 58.88 | 1.15 | 37.63 | 35.10 | 264.93 | 11.22 | 345.51 | 0.6388 | 743.5 | 533.5 | |
| 7.39 | -11.00 | 4.77 | -11.00 | 35.48 | 264.87 | 11.16 | 345.76 | 0.6434 | 715.9 | 999999 | |
| 4.59 | -11.00 | 2.91 | -11.00 | 34.35 | 264.61 | 10.90 | 345.55 | 0.6280 | 944.6 | 999999 | |
| 15.46 | -11.00 | 9.86 | -11.00 | 34.72 | 264.36 | 10.66 | 346.03 | 0.6320 | 944.4 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.55 | 35.51 | 264.14 | 10.43 | 346.67 | 0.6414 | 376.0 | 331.0 | |
| 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. | |