SDO HMI 2011-11-14 20:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.63 | 49.68 | 7.45 | 29.22 | 8.37 | 346.51 | -32.25 | 79.02 | 0.5397 | 342.1 | 75.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.55 | 0.00 | 0.86 | 7.34 | 351.60 | -27.16 | 79.68 | 0.4620 | -939.0 | -677.1 | |
| 2.15 | 8.85 | 1.23 | 5.06 | 7.94 | 349.21 | -29.55 | 79.12 | 0.4994 | -904.6 | -754.1 | |
| 0.00 | 1.38 | 0.00 | 0.79 | 8.59 | 349.06 | -29.70 | 77.88 | 0.5032 | 674.0 | 477.3 | |
| 0.00 | 1.98 | 0.00 | 1.13 | 7.81 | 348.88 | -29.88 | 79.47 | 0.5041 | -819.0 | -672.0 | |
| 0.00 | 1.12 | 0.00 | 0.64 | 7.95 | 348.73 | -30.03 | 79.22 | 0.5066 | -592.0 | -512.0 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 8.64 | 346.46 | -32.30 | 78.52 | 0.5413 | 655.0 | 532.2 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 8.24 | 346.14 | -32.62 | 79.32 | 0.5451 | 989.0 | 761.6 | |
| 0.34 | 1.80 | 0.20 | 1.07 | 8.21 | 345.89 | -32.87 | 79.45 | 0.5485 | 972.5 | 786.8 | |
| 4.38 | 25.44 | 2.60 | 15.11 | 8.29 | 345.67 | -33.09 | 79.35 | 0.5519 | 941.9 | 426.6 | |
| 5.76 | -9.00 | 3.42 | -9.00 | 8.28 | 345.42 | -33.34 | 79.42 | 0.5555 | 861.2 | 999999 | |
| 0.00 | 2.58 | 0.00 | 1.54 | 8.81 | 344.97 | -33.79 | 78.59 | 0.5629 | -338.0 | -241.3 | |
| 0.00 | 0.43 | 0.00 | 0.26 | 8.36 | 344.94 | -33.82 | 79.39 | 0.5624 | -35.0 | 13.4 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 9.19 | 343.58 | -35.18 | 78.26 | 0.5832 | 721.0 | 638.9 | |
| 0.00 | 1.20 | 0.00 | 0.76 | 13.55 | 341.89 | -36.87 | 71.58 | 0.6171 | 548.0 | 444.2 | |
| 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. | |