SDO HMI 2011-08-10 16:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.36 | 0.00 | 12.79 | 18.76 | 223.07 | 15.00 | 311.88 | 0.3297 | -264.5 | -119.1 | |
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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 | 20.39 | 226.67 | 18.60 | 309.63 | 0.3899 | -631.0 | -547.3 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 20.38 | 226.19 | 18.12 | 310.28 | 0.3838 | -685.0 | -562.7 | |
| 0.00 | 2.17 | 0.00 | 1.14 | 17.81 | 224.57 | 16.49 | 306.84 | 0.3392 | -881.0 | -707.7 | |
| 0.00 | 1.53 | 0.00 | 0.81 | 18.41 | 224.23 | 16.15 | 308.85 | 0.3404 | -823.0 | -667.1 | |
| 0.00 | 2.89 | 0.00 | 1.53 | 19.87 | 224.24 | 16.17 | 312.21 | 0.3551 | -787.0 | -714.2 | |
| 0.00 | 0.72 | 0.00 | 0.38 | 18.29 | 223.88 | 15.81 | 309.14 | 0.3349 | -838.0 | -781.0 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 18.95 | 223.94 | 15.87 | 310.59 | 0.3421 | -676.0 | -569.0 | |
| 0.00 | 2.35 | 0.00 | 1.23 | 18.64 | 223.85 | 15.77 | 310.02 | 0.3378 | -883.0 | -667.6 | |
| 0.00 | 2.17 | 0.00 | 1.14 | 18.48 | 223.73 | 15.66 | 309.85 | 0.3349 | -929.0 | -702.6 | |
| 0.00 | 0.54 | 0.00 | 0.28 | 19.44 | 221.93 | 13.85 | 315.41 | 0.3230 | 697.0 | 586.7 | |
| 0.00 | 1.35 | 0.00 | 0.71 | 19.17 | 221.47 | 13.40 | 315.70 | 0.3147 | 977.0 | 812.9 | |
| 0.00 | 5.14 | 0.00 | 2.67 | 18.22 | 220.74 | 12.67 | 314.94 | 0.2955 | 979.0 | 785.1 | |
| 0.00 | 2.26 | 0.00 | 1.17 | 18.26 | 220.48 | 12.41 | 315.60 | 0.2929 | 1041.0 | 832.3 | |
| 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. | |