SDO HMI 2011-10-15 21:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.80 | 189.11 | 16.44 | 116.74 | -26.80 | 36.70 | -17.12 | 153.99 | 0.5989 | 801.5 | 385.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.80 | 171.47 | 16.44 | 105.11 | -26.62 | 37.40 | -16.42 | 154.64 | 0.5922 | 1197.4 | 400.9 | |
| 0.00 | 1.31 | 0.00 | 0.84 | -28.17 | 33.94 | -19.87 | 151.60 | 0.6322 | 752.0 | 553.5 | |
| 0.00 | 2.27 | 0.00 | 1.44 | -27.64 | 33.65 | -20.17 | 150.79 | 0.6281 | 731.0 | 625.3 | |
| 0.00 | 1.75 | 0.00 | 1.11 | -28.00 | 33.58 | -20.24 | 151.02 | 0.6327 | 703.0 | 509.4 | |
| 0.00 | 2.79 | 0.00 | 1.78 | -27.58 | 33.33 | -20.48 | 150.37 | 0.6295 | 668.0 | 577.7 | |
| 0.00 | 0.61 | 0.00 | 0.39 | -27.84 | 33.10 | -20.71 | 150.33 | 0.6340 | 654.0 | 597.9 | |
| 0.00 | 1.31 | 0.00 | 0.85 | -28.86 | 32.71 | -21.10 | 150.77 | 0.6481 | 583.0 | 504.1 | |
| 0.00 | 1.22 | 0.00 | 0.81 | -29.92 | 32.03 | -21.78 | 150.91 | 0.6639 | 714.0 | 586.5 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -24.59 | 32.51 | -21.31 | 146.56 | 0.6018 | 611.0 | 549.8 | |
| 0.00 | 0.70 | 0.00 | 0.46 | -29.60 | 30.88 | -22.93 | 149.40 | 0.6680 | 703.0 | 595.4 | |
| 0.00 | 0.87 | 0.00 | 0.59 | -28.14 | 27.15 | -26.67 | 144.24 | 0.6795 | -671.0 | -566.8 | |
| 0.00 | 0.96 | 0.00 | 0.64 | -27.47 | 26.91 | -26.90 | 143.35 | 0.6749 | -697.0 | -540.0 | |
| 0.00 | 1.31 | 0.00 | 0.95 | -30.01 | 22.65 | -31.16 | 141.98 | 0.7298 | -56.0 | -152.5 | |
| 0.00 | 1.75 | 0.00 | 1.28 | -30.36 | 21.80 | -32.01 | 141.61 | 0.7389 | -784.0 | -585.7 | |
| 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. | |