SDO HMI 2011-11-27 07:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.19 | 245.60 | 20.49 | 128.35 | 17.76 | 223.41 | 8.86 | 332.49 | 0.3198 | -753.4 | -369.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.95 | 219.59 | 7.29 | 114.78 | 17.46 | 224.06 | 9.51 | 330.36 | 0.3202 | -1243.2 | -440.3 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 18.45 | 224.05 | 9.51 | 331.92 | 0.3343 | -11.0 | -4.2 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 20.03 | 223.64 | 9.09 | 335.12 | 0.3543 | 714.0 | 582.1 | |
| 25.24 | -1.00 | 13.20 | -1.00 | 17.86 | 223.42 | 8.87 | 332.64 | 0.3210 | -1311.2 | 999999 | |
| 0.00 | 3.51 | 0.00 | 1.80 | 15.11 | 221.90 | 7.36 | 332.49 | 0.2688 | 770.0 | 784.5 | |
| 0.00 | 3.51 | 0.00 | 1.83 | 18.11 | 221.90 | 7.35 | 337.11 | 0.3139 | -971.0 | -802.8 | |
| 0.00 | 3.42 | 0.00 | 1.76 | 15.63 | 221.77 | 7.22 | 333.81 | 0.2755 | 742.0 | 643.4 | |
| 0.00 | 3.34 | 0.00 | 1.76 | 19.88 | 221.82 | 7.27 | 339.45 | 0.3404 | -770.0 | -670.2 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 19.92 | 221.53 | 6.98 | 340.22 | 0.3393 | -793.0 | -748.7 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 19.57 | 221.36 | 6.81 | 340.31 | 0.3331 | -1051.0 | -838.6 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 14.72 | 221.09 | 6.54 | 334.46 | 0.2567 | 852.0 | 659.6 | |
| 0.00 | 3.17 | 0.00 | 1.64 | 17.66 | 219.91 | 5.36 | 342.37 | 0.2953 | 703.0 | 690.5 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 24.13 | 218.75 | 4.20 | 350.19 | 0.3940 | 862.0 | 703.8 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 20.39 | 218.64 | 4.09 | 348.40 | 0.3339 | 846.0 | 698.1 | |
| 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. | |