SDO HMI 2013-08-21 21:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.42 | 307.22 | 25.44 | 158.20 | -6.89 | 139.34 | 7.76 | 209.44 | 0.2745 | 955.6 | 431.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.89 | 0.00 | 0.99 | -9.02 | 143.72 | 12.14 | 217.35 | 0.3439 | 808.0 | 645.9 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -7.23 | 141.09 | 9.51 | 213.99 | 0.2944 | -732.0 | -537.0 | |
| 0.00 | 1.26 | 0.00 | 0.66 | -9.23 | 140.95 | 9.37 | 210.12 | 0.3216 | 855.0 | 755.6 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -9.39 | 140.89 | 9.31 | 209.72 | 0.3233 | 830.0 | 628.5 | |
| 0.00 | 0.63 | 0.00 | 0.32 | -4.95 | 140.68 | 9.10 | 217.62 | 0.2593 | -509.0 | -580.4 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -7.09 | 140.71 | 9.13 | 213.18 | 0.2891 | 692.0 | 439.2 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -4.73 | 140.58 | 9.01 | 217.85 | 0.2554 | -847.0 | -697.6 | |
| 49.42 | 290.49 | 25.44 | 149.50 | -6.75 | 139.35 | 7.77 | 209.68 | 0.2724 | 1463.5 | 459.2 | |
| 0.00 | 1.89 | 0.00 | 1.00 | -12.09 | 139.18 | 7.61 | 201.71 | 0.3514 | -886.0 | -720.0 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -14.10 | 137.36 | 5.78 | 195.24 | 0.3730 | -827.0 | -701.0 | |
| 0.00 | 3.05 | 0.00 | 1.57 | -7.59 | 136.81 | 5.23 | 199.84 | 0.2674 | 964.0 | 786.0 | |
| 0.00 | 1.35 | 0.00 | 0.71 | -13.05 | 136.71 | 5.13 | 194.31 | 0.3538 | -863.0 | -599.1 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -9.67 | 134.28 | 2.70 | 189.22 | 0.2908 | -937.0 | -635.7 | |
| 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. | |