| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.50 | 61.31 | 11.45 | 32.68 | 17.38 | 42.16 | -11.64 | 31.50 | 0.3682 | -333.0 | -321.5 | |
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back to the solar disc SDO HMI 2011-06-01 17:59:10 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.52 | 18.00 | 48.65 | -5.16 | 14.98 | 0.3322 | 824.0 | 672.9 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 17.24 | 44.56 | -9.24 | 26.56 | 0.3445 | -787.0 | -510.3 | |
| 8.04 | 26.92 | 4.26 | 14.28 | 17.97 | 44.01 | -9.80 | 26.90 | 0.3593 | -1047.5 | -394.4 | |
| 0.54 | 10.12 | 0.29 | 5.35 | 17.33 | 43.72 | -10.09 | 28.46 | 0.3523 | -1133.5 | -907.7 | |
| 6.50 | -4.00 | 3.44 | -4.00 | 17.18 | 43.57 | -10.24 | 29.05 | 0.3513 | -985.1 | 999999 | |
| 0.00 | 2.62 | 0.00 | 1.38 | 16.86 | 43.10 | -10.71 | 30.61 | 0.3506 | -1001.0 | -675.4 | |
| 1.63 | 4.15 | 0.86 | 2.20 | 16.10 | 41.59 | -12.21 | 35.24 | 0.3538 | -997.9 | -809.2 | |
| 0.00 | 2.44 | 0.00 | 1.29 | 15.81 | 41.42 | -12.39 | 36.11 | 0.3518 | -875.0 | -750.3 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 15.94 | 41.31 | -12.49 | 36.12 | 0.3544 | -792.0 | -593.2 | |
| 0.00 | 1.35 | 0.00 | 0.72 | 15.47 | 40.11 | -13.70 | 39.47 | 0.3605 | -932.0 | -787.4 | |
| 3.25 | 3.61 | 1.76 | 1.96 | 17.42 | 37.66 | -16.15 | 40.60 | 0.4094 | 906.7 | 821.0 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 16.30 | 36.73 | -17.07 | 44.08 | 0.4067 | 887.0 | 786.8 | |
| 0.00 | 1.63 | 0.00 | 0.90 | 19.35 | 36.39 | -17.41 | 39.59 | 0.4448 | 795.0 | 645.2 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 15.83 | 36.64 | -17.16 | 45.09 | 0.4025 | 947.0 | 793.0 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 17.36 | 34.96 | -18.85 | 44.98 | 0.4380 | 332.0 | 448.4 | |
| 1.54 | 1.72 | 0.84 | 0.94 | 17.11 | 34.95 | -18.85 | 45.43 | 0.4353 | 879.4 | 837.0 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 17.20 | 34.87 | -18.93 | 45.38 | 0.4372 | 631.0 | 563.5 | |
| 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. | |