SDO HMI 2011-02-15 23:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.85 | 55.28 | 16.22 | 55.79 | 19.67 | 64.93 | 55.28 | 297.30 | 0.8719 | 93.1 | 155.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.51 | 13.62 | 7.34 | 15.40 | 18.86 | 69.04 | 59.39 | 294.92 | 0.9000 | -425.5 | -103.4 | |
| 0.00 | 0.86 | 0.00 | 0.92 | 17.71 | 67.92 | 58.27 | 294.07 | 0.8893 | 162.0 | 103.2 | |
| 0.00 | 1.11 | 0.00 | 1.22 | 18.42 | 68.24 | 58.59 | 294.72 | 0.8933 | -521.0 | -490.7 | |
| 0.00 | 2.14 | 0.00 | 2.38 | 19.06 | 68.48 | 58.83 | 295.32 | 0.8966 | -579.0 | -454.7 | |
| 0.00 | 0.86 | 0.00 | 0.91 | 18.21 | 67.18 | 57.53 | 294.85 | 0.8851 | -402.0 | -387.7 | |
| 0.00 | 1.54 | 0.00 | 1.64 | 18.87 | 67.06 | 57.41 | 295.60 | 0.8860 | -283.0 | -365.1 | |
| 0.43 | 1.89 | 0.43 | 1.87 | 19.08 | 64.73 | 55.08 | 296.67 | 0.8692 | 400.8 | 424.6 | |
| 1.80 | 27.68 | 1.72 | 26.22 | 20.08 | 62.69 | 53.04 | 298.55 | 0.8565 | 572.5 | 437.2 | |
| 2.74 | -8.00 | 2.59 | -8.00 | 19.92 | 62.35 | 52.70 | 298.51 | 0.8532 | 770.3 | 999999 | |
| 4.37 | -8.00 | 4.14 | -8.00 | 20.24 | 62.35 | 52.70 | 298.87 | 0.8543 | 617.4 | 999999 | |
| 0.00 | 1.29 | 0.00 | 1.26 | 21.80 | 63.10 | 53.45 | 300.24 | 0.8654 | -367.0 | -287.5 | |
| 0.00 | 0.86 | 0.00 | 0.80 | 21.24 | 61.18 | 51.53 | 300.45 | 0.8486 | 407.0 | 345.6 | |
| 0.00 | 1.54 | 0.00 | 1.41 | 20.81 | 60.77 | 51.12 | 300.16 | 0.8437 | 587.0 | 370.1 | |
| 0.00 | 1.89 | 0.00 | 1.76 | 21.89 | 61.05 | 51.39 | 301.22 | 0.8499 | 452.0 | 393.8 | |
| 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. | |