| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.45 | 28.00 | 2.33 | 14.51 | -20.56 | 68.13 | 9.63 | 211.44 | 0.2957 | 55.2 | 10.1 | |
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back to the solar disc SDO HMI 2011-02-12 06:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.57 | 0.00 | 1.34 | -20.07 | 72.01 | 13.51 | 223.11 | 0.3225 | 1028.0 | 824.6 | |
| 0.00 | 1.80 | 0.00 | 0.94 | -20.38 | 72.00 | 13.50 | 222.42 | 0.3259 | 1074.0 | 752.4 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -20.59 | 71.99 | 13.49 | 221.92 | 0.3283 | 597.0 | 528.4 | |
| 4.45 | 4.62 | 2.33 | 2.42 | -20.14 | 71.72 | 13.22 | 222.37 | 0.3201 | 1046.0 | 889.7 | |
| 0.00 | 3.08 | 0.00 | 1.62 | -21.27 | 71.82 | 13.32 | 220.15 | 0.3345 | 579.0 | 703.0 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -21.70 | 71.50 | 13.00 | 218.61 | 0.3365 | 766.0 | 540.3 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -20.03 | 71.19 | 12.70 | 221.50 | 0.3130 | 836.0 | 655.8 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -20.23 | 70.50 | 12.00 | 219.53 | 0.3079 | 890.0 | 693.2 | |
| 0.00 | 3.77 | 0.00 | 1.93 | -20.79 | 64.58 | 6.08 | 202.08 | 0.2647 | -1119.0 | -816.6 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -19.88 | 64.32 | 5.83 | 202.65 | 0.2489 | -1033.0 | -800.1 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -19.64 | 63.69 | 5.19 | 200.76 | 0.2413 | -749.0 | -549.4 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -20.29 | 63.26 | 4.76 | 198.31 | 0.2491 | -916.0 | -668.9 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -20.72 | 62.29 | 3.79 | 194.31 | 0.2515 | -1078.0 | -793.9 | |
| 0.00 | 1.63 | 0.00 | 0.83 | -21.12 | 62.18 | 3.68 | 193.49 | 0.2576 | -640.0 | -549.5 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -20.82 | 60.39 | 1.90 | 187.21 | 0.2473 | -1033.0 | -798.0 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -21.34 | 60.15 | 1.65 | 186.04 | 0.2555 | -683.0 | -435.5 | |
| 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. | |