SDO HMI 2011-09-03 08:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.43 | 245.54 | 38.00 | 136.55 | -19.51 | 257.98 | 2.65 | 185.46 | 0.4541 | 100.1 | 22.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.83 | 0.00 | 2.75 | -21.33 | 262.22 | 6.89 | 193.19 | 0.4920 | 1028.0 | 740.2 | |
| 0.00 | 1.61 | 0.00 | 0.91 | -20.99 | 262.21 | 6.88 | 193.33 | 0.4868 | 728.0 | 479.1 | |
| 0.00 | 1.16 | 0.00 | 0.66 | -21.06 | 262.05 | 6.72 | 193.00 | 0.4872 | 885.0 | 688.3 | |
| 0.00 | 0.98 | 0.00 | 0.55 | -19.75 | 261.37 | 6.04 | 192.35 | 0.4654 | 744.0 | 640.8 | |
| 0.00 | 2.06 | 0.00 | 1.16 | -20.77 | 261.19 | 5.86 | 191.51 | 0.4802 | 708.0 | 619.5 | |
| 1.52 | 2.06 | 0.85 | 1.15 | -19.83 | 259.73 | 4.40 | 189.03 | 0.4619 | 884.4 | 826.8 | |
| 0.00 | 1.07 | 0.00 | 0.61 | -21.78 | 259.53 | 4.20 | 187.99 | 0.4912 | 794.0 | 604.7 | |
| 0.00 | 1.34 | 0.00 | 0.77 | -22.83 | 259.56 | 4.23 | 187.74 | 0.5069 | -659.0 | -524.4 | |
| 10.02 | 12.88 | 5.60 | 7.20 | -20.13 | 259.19 | 3.86 | 187.84 | 0.4653 | 862.9 | 521.0 | |
| 0.00 | 1.88 | 0.00 | 1.06 | -21.53 | 258.80 | 3.47 | 186.69 | 0.4860 | 643.0 | 442.5 | |
| 24.15 | 126.23 | 13.45 | 70.25 | -19.72 | 258.73 | 3.40 | 187.03 | 0.4581 | 1097.1 | 255.2 | |
| 2.33 | -11.00 | 1.29 | -11.00 | -19.24 | 258.72 | 3.39 | 187.14 | 0.4507 | 1013.5 | 999999 | |
| 0.00 | 3.40 | 0.00 | 1.88 | -19.04 | 258.39 | 3.06 | 186.52 | 0.4469 | 598.0 | 593.2 | |
| 1.16 | -11.00 | 0.65 | -11.00 | -19.55 | 258.27 | 2.95 | 186.14 | 0.4546 | 819.8 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -17.53 | 258.24 | 2.91 | 186.60 | 0.4230 | -787.0 | -604.1 | |
| 0.00 | 2.86 | 0.00 | 1.65 | -23.17 | 258.18 | 2.86 | 185.18 | 0.5097 | 742.0 | 518.5 | |
| 0.00 | 0.89 | 0.00 | 0.49 | -17.66 | 258.02 | 2.69 | 186.07 | 0.4247 | -887.0 | -716.9 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -17.96 | 257.90 | 2.57 | 185.72 | 0.4292 | -801.0 | -677.8 | |
| 0.00 | 1.52 | 0.00 | 0.84 | -19.17 | 257.88 | 2.55 | 185.41 | 0.4481 | 398.0 | 324.4 | |
| 0.00 | 2.42 | 0.00 | 1.34 | -19.27 | 257.63 | 2.30 | 184.85 | 0.4493 | 91.0 | 5.6 | |
| 1.16 | 15.39 | 0.64 | 8.48 | -18.56 | 257.33 | 2.00 | 184.36 | 0.4379 | -818.8 | -229.1 | |
| 3.58 | -21.00 | 1.97 | -21.00 | -18.83 | 257.30 | 1.97 | 184.25 | 0.4420 | -632.9 | 999999 | |
| 6.80 | -11.00 | 3.76 | -11.00 | -19.23 | 257.21 | 1.88 | 183.98 | 0.4483 | -660.5 | 999999 | |
| 0.81 | -11.00 | 0.45 | -11.00 | -19.44 | 257.21 | 1.88 | 183.95 | 0.4514 | 80.2 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -18.49 | 257.07 | 1.75 | 183.81 | 0.4365 | -1060.0 | -817.8 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -18.22 | 257.01 | 1.68 | 183.71 | 0.4322 | -803.0 | -622.8 | |
| 0.00 | 1.70 | 0.00 | 0.93 | -17.62 | 256.88 | 1.55 | 183.51 | 0.4225 | -906.0 | -805.2 | |
| 2.50 | 3.31 | 1.38 | 1.82 | -18.59 | 256.50 | 1.17 | 182.55 | 0.4376 | -954.6 | -915.9 | |
| 0.00 | 2.33 | 0.00 | 1.29 | -19.43 | 256.35 | 1.02 | 182.14 | 0.4507 | -387.0 | -574.8 | |
| 11.36 | 36.86 | 6.27 | 20.37 | -18.86 | 256.31 | 0.98 | 182.11 | 0.4417 | -1071.6 | -654.4 | |
| 0.00 | 1.16 | 0.00 | 0.65 | -19.91 | 256.32 | 0.99 | 182.04 | 0.4581 | -752.0 | -526.6 | |
| 3.04 | 8.05 | 1.69 | 4.47 | -19.57 | 255.99 | 0.67 | 181.39 | 0.4526 | -719.8 | -710.2 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -18.93 | 255.90 | 0.57 | 181.22 | 0.4425 | -754.0 | -593.5 | |
| 0.00 | 2.15 | 0.00 | 1.19 | -19.70 | 255.35 | 0.02 | 180.05 | 0.4546 | -709.0 | -572.2 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -19.06 | 254.30 | -1.03 | 177.80 | 0.4449 | -633.0 | -571.9 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -17.15 | 254.15 | -1.18 | 177.27 | 0.4148 | -707.0 | -639.1 | |
| 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. | |