SDO HMI 2011-07-18 17:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.29 | 258.26 | 18.71 | 136.89 | 16.95 | 168.61 | 16.88 | 308.10 | 0.3564 | -601.9 | -343.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.54 | 13.37 | 173.40 | 21.66 | 293.69 | 0.3938 | -822.0 | -684.5 | |
| 23.77 | 240.75 | 12.61 | 127.65 | 16.64 | 169.22 | 17.49 | 306.34 | 0.3589 | -1313.5 | -421.9 | |
| 0.73 | -2.00 | 0.39 | -2.00 | 17.02 | 169.12 | 17.39 | 307.36 | 0.3610 | -850.9 | 999999 | |
| 5.53 | -2.00 | 2.93 | -2.00 | 16.34 | 169.02 | 17.29 | 305.90 | 0.3536 | -1515.3 | 999999 | |
| 5.26 | -2.00 | 2.78 | -2.00 | 16.65 | 168.79 | 17.05 | 307.00 | 0.3533 | -1300.3 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 19.25 | 164.57 | 12.84 | 320.48 | 0.3310 | 658.0 | 544.1 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 19.06 | 164.42 | 12.69 | 320.41 | 0.3272 | 929.0 | 806.6 | |
| 0.00 | 1.81 | 0.00 | 0.96 | 23.10 | 162.41 | 10.68 | 331.82 | 0.3624 | 796.0 | 612.8 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 21.47 | 162.05 | 10.32 | 330.19 | 0.3368 | 728.0 | 557.6 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 21.54 | 161.69 | 9.96 | 331.15 | 0.3348 | 619.0 | 508.4 | |
| 0.00 | 1.90 | 0.00 | 1.00 | 21.99 | 161.16 | 9.42 | 333.12 | 0.3372 | 974.0 | 742.3 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 22.15 | 161.00 | 9.27 | 333.73 | 0.3384 | 827.0 | 573.7 | |
| 0.00 | 3.27 | 0.00 | 1.70 | 20.44 | 160.33 | 8.60 | 332.87 | 0.3085 | 1045.0 | 842.2 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 23.27 | 158.66 | 6.93 | 340.90 | 0.3403 | 750.0 | 526.8 | |
| 0.00 | 2.63 | 0.00 | 1.41 | 26.14 | 156.51 | 4.78 | 348.49 | 0.3761 | 813.0 | 619.1 | |
| 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. | |