SDO HMI 2011-10-11 00:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.27 | 170.65 | 16.70 | 107.78 | 23.40 | 153.78 | 35.66 | 300.56 | 0.6232 | -322.6 | -318.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.89 | 156.43 | 1.84 | 99.37 | 23.12 | 154.74 | 36.62 | 299.53 | 0.6328 | -799.5 | -405.6 | |
| 0.88 | -1.00 | 0.56 | -1.00 | 22.84 | 154.65 | 36.53 | 299.16 | 0.6305 | -747.0 | 999999 | |
| 2.36 | -1.00 | 1.50 | -1.00 | 22.63 | 154.50 | 36.38 | 298.92 | 0.6278 | -584.6 | 999999 | |
| 20.14 | -1.00 | 12.80 | -1.00 | 23.30 | 154.35 | 36.23 | 300.00 | 0.6291 | -1029.1 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.65 | 22.93 | 151.69 | 33.57 | 300.87 | 0.5956 | 566.0 | 478.4 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 25.62 | 148.30 | 30.18 | 307.33 | 0.5723 | 536.0 | 496.4 | |
| 0.00 | 0.88 | 0.00 | 0.53 | 25.78 | 148.16 | 30.04 | 307.70 | 0.5718 | 641.0 | 549.9 | |
| 0.00 | 0.88 | 0.00 | 0.53 | 26.04 | 148.07 | 29.96 | 308.16 | 0.5728 | 188.0 | 240.2 | |
| 0.00 | 1.49 | 0.00 | 0.89 | 25.07 | 147.66 | 29.54 | 306.99 | 0.5612 | 702.0 | 559.4 | |
| 0.00 | 0.88 | 0.00 | 0.52 | 26.21 | 145.98 | 27.87 | 310.13 | 0.5506 | 704.0 | 590.3 | |
| 0.00 | 0.88 | 0.00 | 0.51 | 25.79 | 144.83 | 26.71 | 310.51 | 0.5344 | 849.0 | 648.7 | |
| 0.00 | 2.72 | 0.00 | 1.60 | 26.81 | 144.89 | 26.78 | 312.03 | 0.5435 | 664.0 | 558.6 | |
| 0.00 | 2.19 | 0.00 | 1.28 | 26.27 | 144.65 | 26.53 | 311.44 | 0.5363 | 742.0 | 583.4 | |
| 0.00 | 1.23 | 0.00 | 0.72 | 26.50 | 144.59 | 26.47 | 311.84 | 0.5376 | 695.0 | 611.9 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 24.21 | 143.73 | 25.61 | 308.98 | 0.5092 | 715.0 | 533.1 | |
| 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. | |