SDO HMI 2011-06-05 16:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.71 | 188.17 | 20.25 | 103.95 | 9.15 | 336.82 | -24.60 | 68.54 | 0.4435 | -656.5 | -331.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.26 | 0.00 | 1.22 | 7.28 | 339.22 | -22.21 | 70.97 | 0.3982 | -853.0 | -550.0 | |
| 0.00 | 2.80 | 0.00 | 1.54 | 11.26 | 338.48 | -22.94 | 62.65 | 0.4323 | -744.0 | -611.8 | |
| 30.11 | 145.59 | 16.61 | 80.29 | 9.28 | 337.05 | -24.37 | 68.09 | 0.4408 | -1212.1 | -386.8 | |
| 2.26 | 25.77 | 1.24 | 14.21 | 7.93 | 336.84 | -24.58 | 71.18 | 0.4371 | 749.1 | -298.9 | |
| 1.81 | -3.00 | 1.00 | -3.00 | 9.47 | 336.63 | -24.80 | 68.01 | 0.4479 | -540.0 | 999999 | |
| 2.53 | -4.00 | 1.40 | -4.00 | 8.39 | 336.67 | -24.75 | 70.28 | 0.4418 | -862.4 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 7.56 | 336.46 | -24.97 | 72.23 | 0.4412 | 695.0 | 456.3 | |
| 0.00 | 2.08 | 0.00 | 1.15 | 8.15 | 336.08 | -25.35 | 71.21 | 0.4495 | -890.0 | -680.0 | |
| 0.00 | 2.71 | 0.00 | 1.50 | 7.47 | 336.02 | -25.40 | 72.70 | 0.4473 | 801.0 | 533.4 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 7.47 | 335.65 | -25.78 | 72.92 | 0.4529 | -702.0 | -510.4 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 10.31 | 333.13 | -28.29 | 68.75 | 0.5023 | 638.0 | 515.9 | |
| 0.00 | 1.54 | 0.00 | 0.91 | 12.46 | 330.56 | -30.86 | 66.48 | 0.5483 | 808.0 | 653.4 | |
| 0.00 | 1.54 | 0.00 | 0.92 | 12.89 | 329.96 | -31.47 | 66.10 | 0.5587 | 790.0 | 640.6 | |
| 0.00 | 0.72 | 0.00 | 0.44 | 9.95 | 327.91 | -33.52 | 72.16 | 0.5735 | 548.0 | 530.6 | |
| 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. | |