SDO HMI 2011-10-10 12:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.89 | 195.43 | 22.98 | 115.61 | 23.41 | 154.09 | 29.36 | 304.54 | 0.5483 | -663.6 | -307.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.97 | 179.66 | 4.74 | 106.57 | 23.05 | 154.89 | 30.16 | 303.28 | 0.5551 | -929.1 | -357.5 | |
| 1.93 | -1.00 | 1.14 | -1.00 | 22.79 | 154.60 | 29.87 | 303.05 | 0.5499 | -675.3 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.64 | 26.81 | 155.58 | 30.84 | 308.62 | 0.5879 | -582.0 | -450.3 | |
| 26.45 | -1.00 | 15.68 | -1.00 | 23.30 | 154.46 | 29.73 | 303.99 | 0.5514 | -1227.8 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.46 | 22.10 | 153.95 | 29.22 | 302.36 | 0.5376 | -706.0 | -510.3 | |
| 0.00 | 0.70 | 0.00 | 0.41 | 21.77 | 153.59 | 28.85 | 302.08 | 0.5310 | 404.0 | 297.4 | |
| 0.00 | 1.40 | 0.00 | 0.84 | 26.31 | 153.35 | 28.62 | 309.64 | 0.5597 | -617.0 | -409.7 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 25.65 | 151.82 | 27.09 | 309.93 | 0.5374 | -684.0 | -588.8 | |
| 0.00 | 2.28 | 0.00 | 1.30 | 25.78 | 148.10 | 23.37 | 313.84 | 0.4972 | 641.0 | 613.2 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 26.27 | 147.84 | 23.11 | 314.91 | 0.4990 | 480.0 | 512.2 | |
| 0.00 | 1.49 | 0.00 | 0.85 | 26.12 | 147.59 | 22.86 | 314.96 | 0.4949 | 811.0 | 675.0 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 26.02 | 145.14 | 20.40 | 317.77 | 0.4680 | 759.0 | 636.9 | |
| 0.00 | 1.75 | 0.00 | 0.98 | 26.22 | 144.92 | 20.19 | 318.36 | 0.4679 | 791.0 | 663.9 | |
| 2.54 | 3.68 | 1.42 | 2.05 | 25.87 | 144.79 | 20.05 | 317.98 | 0.4629 | 875.9 | 753.0 | |
| 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. | |