SDO HMI 2011-10-18 00:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.63 | 34.45 | 7.49 | 29.83 | 24.06 | 331.69 | -54.09 | 64.50 | 0.8201 | -327.6 | -238.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.57 | 0.00 | 1.19 | 20.62 | 337.42 | -48.36 | 67.57 | 0.7590 | -672.0 | -464.2 | |
| 0.00 | 0.52 | 0.00 | 0.43 | 25.86 | 334.59 | -51.19 | 61.67 | 0.7989 | -503.0 | -438.3 | |
| 0.00 | 1.05 | 0.00 | 0.87 | 24.41 | 333.79 | -51.98 | 63.63 | 0.8030 | -483.0 | -436.9 | |
| 2.18 | 13.52 | 1.79 | 11.13 | 23.43 | 333.98 | -51.80 | 64.79 | 0.7992 | -712.0 | -526.0 | |
| 0.00 | 1.22 | 0.00 | 1.00 | 23.03 | 334.15 | -51.63 | 65.25 | 0.7968 | -516.0 | -459.3 | |
| 1.48 | -4.00 | 1.22 | -4.00 | 23.54 | 333.71 | -52.07 | 64.72 | 0.8020 | -421.2 | 999999 | |
| 0.70 | -4.00 | 0.57 | -4.00 | 23.20 | 333.84 | -51.93 | 65.11 | 0.8000 | -754.0 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.79 | 22.76 | 333.92 | -51.85 | 65.63 | 0.7984 | -496.0 | -505.5 | |
| 0.00 | 1.66 | 0.00 | 1.37 | 22.79 | 333.53 | -52.24 | 65.67 | 0.8022 | -634.0 | -447.1 | |
| 0.00 | 0.96 | 0.00 | 0.82 | 24.20 | 332.34 | -53.44 | 64.20 | 0.8159 | -305.0 | -261.5 | |
| 0.00 | 2.09 | 0.00 | 1.84 | 23.09 | 330.83 | -54.95 | 65.83 | 0.8276 | 473.0 | 308.5 | |
| 4.27 | 6.80 | 3.91 | 6.22 | 24.41 | 329.27 | -56.51 | 64.55 | 0.8431 | -311.6 | -208.8 | |
| 0.00 | 2.44 | 0.00 | 2.49 | 27.59 | 325.73 | -60.05 | 61.50 | 0.8758 | 381.0 | 260.0 | |
| 0.00 | 1.66 | 0.00 | 1.68 | 26.77 | 325.85 | -59.93 | 62.40 | 0.8738 | 461.0 | 428.9 | |
| 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. | |