SDO HMI 2011-08-18 00:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.71 | 97.68 | 19.74 | 97.54 | -20.70 | 56.58 | -54.54 | 118.59 | 0.8694 | 399.3 | 151.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.81 | 80.13 | 9.60 | 78.94 | -20.86 | 57.39 | -53.73 | 119.06 | 0.8639 | 826.8 | 182.6 | |
| 4.59 | -1.00 | 4.56 | -1.00 | -20.98 | 56.82 | -54.29 | 118.97 | 0.8686 | 350.3 | 999999 | |
| 1.08 | -1.00 | 1.07 | -1.00 | -20.72 | 56.73 | -54.38 | 118.66 | 0.8684 | 281.2 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.69 | -18.62 | 57.01 | -54.11 | 116.49 | 0.8598 | 637.0 | 558.2 | |
| 0.00 | 1.26 | 0.00 | 1.23 | -18.72 | 56.74 | -54.37 | 116.49 | 0.8622 | 495.0 | 460.1 | |
| 1.35 | 2.70 | 1.34 | 2.68 | -19.38 | 56.08 | -55.03 | 116.96 | 0.8693 | 334.9 | 433.8 | |
| 0.00 | 0.99 | 0.00 | 0.98 | -18.70 | 56.19 | -54.92 | 116.27 | 0.8665 | 478.0 | 404.5 | |
| 0.00 | 0.99 | 0.00 | 1.00 | -18.82 | 55.34 | -55.78 | 116.09 | 0.8734 | 288.0 | 245.2 | |
| 0.00 | 1.17 | 0.00 | 1.20 | -19.46 | 54.95 | -56.17 | 116.63 | 0.8781 | 216.0 | 231.5 | |
| 0.00 | 0.99 | 0.00 | 1.00 | -18.62 | 55.38 | -55.73 | 115.88 | 0.8724 | 215.0 | 186.8 | |
| 0.00 | 0.90 | 0.00 | 1.02 | -22.73 | 52.97 | -58.14 | 119.38 | 0.9008 | -319.0 | -299.6 | |
| 1.26 | 1.89 | 1.31 | 1.96 | -19.69 | 54.71 | -56.40 | 116.79 | 0.8805 | 339.3 | 402.9 | |
| 1.62 | 4.32 | 1.86 | 4.95 | -20.77 | 51.74 | -59.37 | 116.90 | 0.9040 | -661.1 | -550.6 | |
| 0.00 | 1.62 | 0.00 | 1.89 | -20.68 | 51.28 | -59.84 | 116.66 | 0.9069 | -433.0 | -397.2 | |
| 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. | |