SDO HMI 2011-10-14 02:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.63 | 104.94 | 15.05 | 57.12 | 19.93 | 98.04 | 20.60 | 306.90 | 0.4152 | -212.9 | -195.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.97 | 8.75 | 1.63 | 4.80 | 20.18 | 99.30 | 21.86 | 305.82 | 0.4329 | -751.8 | -476.4 | |
| 10.84 | 57.19 | 5.93 | 31.24 | 19.57 | 99.05 | 21.60 | 304.88 | 0.4247 | -1016.2 | -452.1 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 19.94 | 99.06 | 21.62 | 305.62 | 0.4279 | -469.0 | -435.3 | |
| 0.00 | 5.16 | 0.00 | 2.82 | 20.01 | 98.77 | 21.32 | 306.10 | 0.4247 | -921.0 | -721.2 | |
| 4.64 | -2.00 | 2.53 | -2.00 | 19.55 | 98.63 | 21.19 | 305.32 | 0.4192 | -1064.8 | 999999 | |
| 0.00 | 1.57 | 0.00 | 0.86 | 19.84 | 98.33 | 20.89 | 306.26 | 0.4178 | -815.0 | -658.3 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 19.81 | 98.16 | 20.72 | 306.42 | 0.4153 | -758.0 | -648.1 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 19.45 | 97.91 | 20.46 | 305.97 | 0.4091 | -819.0 | -620.2 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 18.76 | 97.51 | 20.07 | 304.96 | 0.3982 | 748.0 | 616.7 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 19.42 | 96.99 | 19.55 | 307.05 | 0.3971 | -788.0 | -610.0 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 21.31 | 96.09 | 18.64 | 312.14 | 0.4034 | 624.0 | 485.3 | |
| 9.18 | 15.04 | 4.96 | 8.12 | 21.00 | 95.98 | 18.54 | 311.69 | 0.3991 | 1001.8 | 668.0 | |
| 0.00 | 3.32 | 0.00 | 1.79 | 20.42 | 95.87 | 18.43 | 310.65 | 0.3922 | 951.0 | 805.3 | |
| 0.00 | 1.40 | 0.00 | 0.75 | 20.36 | 94.82 | 17.38 | 312.07 | 0.3789 | 726.0 | 603.6 | |
| 0.00 | 6.65 | 0.00 | 3.55 | 20.17 | 94.74 | 17.29 | 311.82 | 0.3760 | 952.0 | 835.2 | |
| 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. | |