SDO HMI 2011-08-25 07:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.03 | 0.00 | 12.72 | 7.05 | 348.52 | -26.26 | 88.39 | 0.4406 | -364.6 | -441.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.53 | 6.95 | 352.32 | -22.45 | 88.82 | 0.3808 | -899.0 | -746.4 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 5.38 | 352.35 | -22.42 | 92.97 | 0.3818 | -756.0 | -615.9 | |
| 0.00 | 2.16 | 0.00 | 1.16 | 7.01 | 352.18 | -22.59 | 88.66 | 0.3830 | -1075.0 | -852.8 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 7.68 | 351.05 | -23.72 | 86.90 | 0.4010 | -809.0 | -714.3 | |
| 0.00 | 2.52 | 0.00 | 1.37 | 7.04 | 350.41 | -24.36 | 88.46 | 0.4112 | -810.0 | -518.0 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 7.22 | 350.30 | -24.47 | 88.02 | 0.4129 | -768.0 | -648.8 | |
| 0.00 | 2.07 | 0.00 | 1.14 | 7.57 | 348.32 | -26.46 | 87.13 | 0.4440 | -695.0 | -597.5 | |
| 0.00 | 5.48 | 0.00 | 3.04 | 6.85 | 347.95 | -26.82 | 88.73 | 0.4499 | -712.0 | -655.2 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 6.60 | 347.76 | -27.01 | 89.27 | 0.4530 | -829.0 | -676.2 | |
| 0.00 | 1.80 | 0.00 | 1.00 | 6.56 | 347.56 | -27.21 | 89.34 | 0.4562 | -772.0 | -602.2 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 8.26 | 343.93 | -30.84 | 85.66 | 0.5108 | 895.0 | 694.1 | |
| 0.00 | 0.54 | 0.00 | 0.31 | 8.40 | 343.81 | -30.96 | 85.37 | 0.5126 | 582.0 | 560.5 | |
| 0.00 | 1.35 | 0.00 | 0.78 | 8.06 | 343.70 | -31.07 | 86.04 | 0.5143 | 890.0 | 648.8 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 7.08 | 343.10 | -31.67 | 87.92 | 0.5235 | 654.0 | 508.1 | |
| 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. | |