SDO HMI 2011-10-25 17:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.70 | 185.26 | 23.06 | 154.04 | -21.68 | 331.38 | 47.26 | 238.14 | 0.8054 | -447.0 | -275.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.30 | 5.12 | 1.21 | 4.74 | -18.92 | 337.43 | 53.30 | 243.84 | 0.8472 | 457.6 | 419.0 | |
| 0.00 | 0.69 | 0.00 | 0.63 | -17.79 | 336.87 | 52.74 | 244.91 | 0.8390 | 643.0 | 600.9 | |
| 0.00 | 0.95 | 0.00 | 0.88 | -18.78 | 337.20 | 53.08 | 243.92 | 0.8448 | 423.0 | 380.8 | |
| 1.91 | 5.99 | 1.76 | 5.50 | -19.03 | 337.11 | 52.98 | 243.60 | 0.8448 | 687.8 | 570.1 | |
| 0.00 | 1.22 | 0.00 | 1.12 | -19.47 | 336.89 | 52.76 | 243.03 | 0.8443 | 487.0 | 441.0 | |
| 0.00 | 3.65 | 0.00 | 3.33 | -19.73 | 336.54 | 52.42 | 242.60 | 0.8423 | 405.0 | 336.2 | |
| 0.00 | 4.17 | 0.00 | 3.75 | -19.09 | 336.14 | 52.02 | 243.17 | 0.8369 | 661.0 | 590.0 | |
| 0.00 | 0.87 | 0.00 | 0.76 | -20.28 | 334.70 | 50.57 | 241.24 | 0.8286 | -113.0 | -187.7 | |
| 0.00 | 1.39 | 0.00 | 1.16 | -21.71 | 331.56 | 47.44 | 238.24 | 0.8070 | -468.0 | -373.0 | |
| 4.34 | 26.74 | 3.57 | 21.98 | -21.37 | 330.99 | 46.87 | 238.35 | 0.8005 | -727.2 | -354.5 | |
| 1.74 | 2.60 | 1.43 | 2.15 | -21.77 | 330.97 | 46.85 | 237.89 | 0.8021 | -484.4 | -403.5 | |
| 0.78 | 131.87 | 0.64 | 108.04 | -22.08 | 330.73 | 46.60 | 237.42 | 0.8013 | -658.3 | -396.2 | |
| 10.68 | -12.00 | 8.79 | -12.00 | -22.37 | 330.53 | 46.40 | 236.99 | 0.8008 | -812.2 | 999999 | |
| 6.95 | -12.00 | 5.66 | -12.00 | -22.02 | 330.24 | 46.11 | 237.25 | 0.7967 | -1129.0 | 999999 | |
| 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. | |