SDO HMI 2011-07-24 05:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.50 | 39.65 | 9.67 | 20.79 | 24.12 | 78.86 | -0.10 | 359.86 | 0.3293 | -442.4 | -259.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.62 | 9.07 | 3.98 | 4.74 | 23.53 | 81.07 | 2.11 | 353.90 | 0.3186 | -929.2 | -664.1 | |
| 6.80 | 8.89 | 3.56 | 4.65 | 23.66 | 80.64 | 1.68 | 355.18 | 0.3201 | -936.9 | -798.0 | |
| 4.08 | 5.35 | 2.13 | 2.80 | 23.69 | 80.24 | 1.28 | 356.33 | 0.3202 | -971.9 | -828.6 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 22.63 | 79.63 | 0.67 | 357.94 | 0.3021 | -939.0 | -706.2 | |
| 0.00 | 2.27 | 0.00 | 1.18 | 23.56 | 78.94 | -0.02 | 0.06 | 0.3174 | -967.0 | -774.9 | |
| 0.00 | 2.54 | 0.00 | 1.32 | 23.24 | 78.87 | -0.09 | 0.26 | 0.3120 | -746.0 | -694.3 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 25.56 | 77.32 | -1.64 | 4.23 | 0.3514 | -831.0 | -677.5 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 25.79 | 77.25 | -1.71 | 4.36 | 0.3552 | -859.0 | -700.9 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 26.69 | 74.61 | -4.35 | 10.46 | 0.3754 | 775.0 | 578.2 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 26.59 | 73.65 | -5.31 | 12.74 | 0.3768 | 559.0 | 464.7 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 26.23 | 73.60 | -5.36 | 13.10 | 0.3713 | 690.0 | 569.0 | |
| 0.00 | 2.00 | 0.00 | 1.04 | 23.06 | 73.50 | -5.46 | 15.86 | 0.3216 | 721.0 | 650.8 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 24.47 | 73.41 | -5.55 | 14.87 | 0.3444 | 885.0 | 707.9 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 29.69 | 72.58 | -6.38 | 13.07 | 0.4288 | 671.0 | 552.5 | |
| 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. | |