SDO HMI 2011-10-21 21:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.41 | 185.18 | 62.86 | 481.85 | 9.30 | 53.91 | 79.24 | 278.47 | 0.9793 | -0.0 | -3.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.57 | 113.56 | 17.03 | 356.57 | 8.43 | 56.05 | 81.38 | 277.69 | 0.9876 | 264.0 | 20.5 | |
| 10.88 | -1.00 | 31.51 | -1.00 | 8.51 | 55.52 | 80.85 | 277.74 | 0.9861 | -369.2 | 999999 | |
| 0.00 | 2.35 | 0.00 | 6.02 | 9.48 | 54.24 | 79.57 | 278.63 | 0.9820 | -559.0 | -480.2 | |
| 0.00 | 6.27 | 0.00 | 15.88 | 9.92 | 54.14 | 79.46 | 279.07 | 0.9816 | -563.0 | -438.8 | |
| 0.00 | 1.13 | 0.00 | 2.12 | 9.35 | 50.00 | 75.33 | 278.25 | 0.9657 | -250.0 | -208.8 | |
| 0.00 | 3.83 | 0.00 | 7.23 | 9.65 | 50.08 | 75.40 | 278.56 | 0.9660 | -289.0 | -271.8 | |
| 0.00 | 1.39 | 0.00 | 2.43 | 10.64 | 48.85 | 74.18 | 279.53 | 0.9601 | 210.0 | 115.8 | |
| 0.00 | 0.78 | 0.00 | 1.34 | 10.51 | 48.55 | 73.87 | 279.38 | 0.9586 | 398.0 | 393.2 | |
| 0.00 | 1.22 | 0.00 | 2.06 | 10.42 | 48.26 | 73.59 | 279.27 | 0.9573 | 89.0 | 195.6 | |
| 8.96 | 46.90 | 14.32 | 75.71 | 12.18 | 47.31 | 72.64 | 281.08 | 0.9520 | 512.7 | 27.1 | |
| 0.00 | 4.53 | 0.00 | 7.38 | 13.83 | 47.71 | 73.04 | 282.82 | 0.9539 | -108.0 | -76.6 | |
| 0.00 | 2.52 | 0.00 | 4.02 | 13.46 | 47.32 | 72.65 | 282.43 | 0.9519 | 504.0 | 427.1 | |
| 0.00 | 0.70 | 0.00 | 1.09 | 13.10 | 46.94 | 72.27 | 282.04 | 0.9500 | 362.0 | 426.6 | |
| 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. | |