SDO HMI 2011-11-14 04:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.32 | 51.53 | 26.37 | 51.56 | 19.45 | 87.03 | 59.48 | 290.74 | 0.8705 | -56.3 | -83.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.19 | 18.84 | 6.53 | 19.73 | 19.32 | 88.82 | 61.28 | 290.34 | 0.8846 | -432.3 | -391.3 | |
| 3.70 | -1.00 | 3.83 | -1.00 | 19.26 | 88.26 | 60.71 | 290.34 | 0.8801 | -633.4 | 999999 | |
| 8.95 | 11.79 | 8.65 | 11.40 | 18.36 | 85.98 | 58.44 | 289.64 | 0.8608 | 547.0 | 296.2 | |
| 0.00 | 1.20 | 0.00 | 1.20 | 19.79 | 86.75 | 59.20 | 291.17 | 0.8688 | 29.0 | 8.5 | |
| 0.00 | 1.20 | 0.00 | 1.18 | 19.31 | 86.40 | 58.85 | 290.67 | 0.8653 | 152.0 | 120.1 | |
| 0.00 | 2.67 | 0.00 | 2.60 | 19.41 | 86.21 | 58.67 | 290.81 | 0.8639 | 456.0 | 307.6 | |
| 0.00 | 1.12 | 0.00 | 1.11 | 19.99 | 86.56 | 59.01 | 291.42 | 0.8675 | 348.0 | 255.6 | |
| 1.03 | 1.72 | 0.99 | 1.64 | 18.40 | 85.59 | 58.05 | 289.75 | 0.8575 | 420.8 | 416.2 | |
| 0.00 | 1.20 | 0.00 | 1.16 | 18.74 | 85.66 | 58.11 | 290.14 | 0.8585 | -248.0 | -283.8 | |
| 1.98 | 9.38 | 1.97 | 9.27 | 21.31 | 86.59 | 59.04 | 292.93 | 0.8695 | -381.0 | -393.2 | |
| 4.47 | -10.00 | 4.40 | -10.00 | 21.36 | 86.18 | 58.64 | 293.05 | 0.8663 | -579.6 | 999999 | |
| 0.00 | 1.46 | 0.00 | 1.38 | 19.15 | 84.87 | 57.33 | 290.73 | 0.8524 | 515.0 | 371.8 | |
| 0.00 | 0.95 | 0.00 | 0.89 | 19.59 | 84.76 | 57.22 | 291.27 | 0.8521 | 271.0 | 212.3 | |
| 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. | |