SDO HMI 2011-06-29 21:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.89 | 64.65 | 13.50 | 51.62 | 15.41 | 350.08 | -50.89 | 72.38 | 0.7867 | 144.4 | 280.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.82 | 19.29 | 358.92 | -42.05 | 64.83 | 0.7008 | -558.0 | -453.2 | |
| 0.00 | 0.82 | 0.00 | 0.57 | 18.79 | 358.42 | -42.55 | 65.70 | 0.7047 | -557.0 | -484.8 | |
| 0.00 | 1.09 | 0.00 | 0.82 | 16.20 | 353.57 | -47.40 | 70.66 | 0.7514 | -443.0 | -413.5 | |
| 0.00 | 1.00 | 0.00 | 0.75 | 15.17 | 352.85 | -48.12 | 72.17 | 0.7571 | -573.0 | -549.6 | |
| 1.82 | 3.90 | 1.38 | 2.98 | 15.85 | 352.49 | -48.48 | 71.37 | 0.7623 | -752.6 | -601.6 | |
| 4.18 | 9.08 | 3.22 | 7.00 | 16.43 | 351.96 | -49.01 | 70.74 | 0.7692 | -578.5 | -455.5 | |
| 0.00 | 1.36 | 0.00 | 1.08 | 17.53 | 350.77 | -50.20 | 69.62 | 0.7837 | -204.0 | -266.4 | |
| 0.00 | 0.91 | 0.00 | 0.73 | 17.35 | 350.29 | -50.68 | 69.95 | 0.7883 | -216.0 | -286.3 | |
| 0.00 | 1.00 | 0.00 | 0.80 | 15.74 | 350.27 | -50.70 | 71.98 | 0.7855 | -181.0 | -92.5 | |
| 0.00 | 0.64 | 0.00 | 0.51 | 16.29 | 349.92 | -51.05 | 71.35 | 0.7900 | 701.0 | 614.9 | |
| 0.00 | 1.09 | 0.00 | 0.88 | 16.00 | 349.67 | -51.30 | 71.77 | 0.7921 | 763.0 | 651.2 | |
| 0.00 | 1.73 | 0.00 | 1.39 | 15.81 | 349.74 | -51.23 | 71.99 | 0.7911 | 591.0 | 609.0 | |
| 0.54 | 1.63 | 0.44 | 1.33 | 15.83 | 349.37 | -51.60 | 72.03 | 0.7948 | 616.5 | 552.1 | |
| 2.18 | 39.22 | 1.77 | 31.96 | 15.23 | 349.18 | -51.79 | 72.82 | 0.7958 | 647.3 | 558.4 | |
| 4.72 | -14.00 | 3.86 | -14.00 | 14.78 | 348.97 | -52.00 | 73.42 | 0.7972 | 858.1 | 999999 | |
| 3.45 | -14.00 | 2.83 | -14.00 | 14.49 | 348.76 | -52.21 | 73.81 | 0.7989 | 625.5 | 999999 | |
| 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. | |