SDO HMI 2011-01-01 18:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.55 | 180.60 | 34.71 | 122.07 | 34.03 | 267.48 | 22.53 | 332.14 | 0.6821 | -53.2 | -40.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.58 | 91.20 | 12.00 | 62.35 | 33.40 | 270.09 | 25.15 | 328.98 | 0.6908 | -1056.3 | -275.2 | |
| 1.70 | 11.72 | 1.15 | 7.90 | 33.47 | 268.71 | 23.77 | 330.38 | 0.6827 | -645.0 | -608.2 | |
| 6.37 | -2.00 | 4.29 | -2.00 | 33.43 | 268.43 | 23.49 | 330.63 | 0.6805 | -766.1 | 999999 | |
| 0.00 | 2.46 | 0.00 | 1.65 | 33.06 | 268.25 | 23.31 | 330.49 | 0.6755 | -583.0 | -495.9 | |
| 0.00 | 0.93 | 0.00 | 0.63 | 34.62 | 266.87 | 21.93 | 333.18 | 0.6836 | -486.0 | -424.5 | |
| 0.00 | 1.10 | 0.00 | 0.74 | 34.43 | 266.78 | 21.84 | 333.12 | 0.6811 | -565.0 | -544.4 | |
| 0.00 | 1.27 | 0.00 | 0.84 | 33.54 | 264.99 | 20.05 | 334.29 | 0.6611 | 622.0 | 474.5 | |
| 4.84 | 69.12 | 3.23 | 46.12 | 34.90 | 264.41 | 19.47 | 335.95 | 0.6732 | 724.2 | 406.6 | |
| 0.00 | 1.19 | 0.00 | 0.78 | 33.30 | 264.03 | 19.09 | 335.15 | 0.6530 | 685.0 | 621.9 | |
| 0.00 | 1.61 | 0.00 | 1.06 | 33.70 | 263.86 | 18.92 | 335.65 | 0.6566 | 845.0 | 668.5 | |
| 11.72 | -8.00 | 7.85 | -8.00 | 35.31 | 264.06 | 19.12 | 336.62 | 0.6759 | 732.2 | 999999 | |
| 1.61 | -8.00 | 1.07 | -8.00 | 34.40 | 263.73 | 18.78 | 336.32 | 0.6639 | 834.8 | 999999 | |
| 4.67 | -8.00 | 3.09 | -8.00 | 34.66 | 263.52 | 18.58 | 336.73 | 0.6658 | 1111.9 | 999999 | |
| 3.06 | -8.00 | 2.03 | -8.00 | 35.00 | 263.52 | 18.58 | 336.97 | 0.6697 | 790.6 | 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. | |