SDO HMI 2011-01-03 23:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.51 | 52.06 | 14.45 | 50.91 | 34.28 | 264.89 | 49.05 | 313.67 | 0.8635 | 29.9 | 36.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.16 | 13.08 | 4.56 | 14.31 | 32.92 | 270.61 | 54.77 | 309.77 | 0.8940 | -440.8 | -271.1 | |
| 1.10 | -1.00 | 1.21 | -1.00 | 33.21 | 270.44 | 54.60 | 310.12 | 0.8938 | -360.5 | 999999 | |
| 0.00 | 1.19 | 0.00 | 1.26 | 32.37 | 269.63 | 53.79 | 309.58 | 0.8862 | -547.0 | -462.7 | |
| 0.00 | 1.44 | 0.00 | 1.39 | 33.40 | 264.81 | 48.97 | 312.71 | 0.8592 | -508.0 | -368.6 | |
| 3.57 | 5.35 | 3.45 | 5.16 | 33.84 | 264.82 | 48.98 | 313.15 | 0.8611 | -339.4 | -354.0 | |
| 0.00 | 3.74 | 0.00 | 3.52 | 34.50 | 263.12 | 47.28 | 314.63 | 0.8530 | 330.0 | 320.7 | |
| 1.95 | 11.38 | 1.82 | 10.66 | 34.76 | 262.42 | 46.58 | 315.25 | 0.8497 | 329.9 | -66.7 | |
| 0.00 | 1.27 | 0.00 | 1.17 | 34.55 | 261.91 | 46.07 | 315.30 | 0.8453 | 664.0 | 546.9 | |
| 1.27 | 5.86 | 1.18 | 5.42 | 35.57 | 261.46 | 45.61 | 316.56 | 0.8475 | 335.1 | 466.2 | |
| 0.00 | 1.44 | 0.00 | 1.32 | 35.26 | 261.12 | 45.28 | 316.41 | 0.8438 | 536.0 | 440.6 | |
| 0.00 | 1.02 | 0.00 | 0.96 | 36.15 | 261.73 | 45.89 | 316.99 | 0.8520 | 307.0 | 226.3 | |
| 0.00 | 1.02 | 0.00 | 0.94 | 35.79 | 261.31 | 45.46 | 316.85 | 0.8476 | 284.0 | 261.8 | |
| 0.00 | 0.85 | 0.00 | 0.78 | 35.73 | 260.85 | 45.01 | 317.03 | 0.8444 | 560.0 | 508.0 | |
| 0.00 | 1.70 | 0.00 | 1.56 | 35.96 | 260.80 | 44.96 | 317.28 | 0.8453 | 474.0 | 418.6 | |
| 2.46 | 2.72 | 2.23 | 2.46 | 35.45 | 260.34 | 44.50 | 317.02 | 0.8396 | 548.0 | 395.3 | |
| 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. | |