SDO HMI 2011-11-29 06:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.68 | 211.39 | 48.40 | 205.62 | 7.77 | 129.56 | -59.18 | 81.64 | 0.8610 | -162.9 | -123.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.62 | 0.00 | 1.42 | 7.32 | 133.32 | -55.41 | 81.90 | 0.8270 | -170.0 | -211.2 | |
| 2.99 | 111.43 | 2.73 | 101.45 | 8.64 | 131.80 | -56.93 | 80.45 | 0.8423 | 320.6 | -298.6 | |
| 19.75 | -2.00 | 18.01 | -2.00 | 7.51 | 131.83 | -56.91 | 81.79 | 0.8413 | -788.7 | 999999 | |
| 0.00 | 0.68 | 0.00 | 0.63 | 8.84 | 131.31 | -57.43 | 80.25 | 0.8470 | -187.0 | -145.2 | |
| 5.22 | 16.93 | 4.87 | 15.90 | 6.45 | 130.81 | -57.93 | 83.11 | 0.8503 | -644.6 | -418.8 | |
| 0.00 | 1.54 | 0.00 | 1.45 | 7.04 | 130.58 | -58.16 | 82.43 | 0.8526 | -567.0 | -482.8 | |
| 0.00 | 1.45 | 0.00 | 1.39 | 7.75 | 130.20 | -58.53 | 81.62 | 0.8564 | -218.0 | -222.1 | |
| 1.71 | 2.74 | 1.63 | 2.61 | 7.09 | 130.17 | -58.57 | 82.39 | 0.8563 | -246.9 | -189.8 | |
| 2.48 | 3.25 | 2.39 | 3.13 | 7.41 | 129.75 | -58.98 | 82.04 | 0.8602 | -362.5 | -387.1 | |
| 0.00 | 1.20 | 0.00 | 1.17 | 7.38 | 129.35 | -59.39 | 82.11 | 0.8637 | 4.0 | 1.4 | |
| 2.22 | 3.42 | 2.17 | 3.35 | 6.99 | 129.26 | -59.48 | 82.57 | 0.8643 | -230.2 | -236.9 | |
| 2.99 | 12.40 | 3.12 | 12.89 | 8.93 | 127.31 | -61.43 | 80.47 | 0.8817 | 597.8 | 415.1 | |
| 7.87 | 54.73 | 8.56 | 60.23 | 8.19 | 125.90 | -62.83 | 81.39 | 0.8925 | 817.4 | 159.4 | |
| 4.45 | -13.00 | 4.92 | -13.00 | 8.12 | 125.46 | -63.28 | 81.49 | 0.8960 | 368.8 | 999999 | |
| 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. | |