SDO HMI 2011-10-08 02:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.47 | 319.28 | 44.82 | 218.26 | -14.98 | 118.42 | -38.18 | 119.91 | 0.6896 | 276.7 | 155.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.87 | 182.45 | 22.27 | 119.86 | -15.18 | 121.24 | -35.36 | 121.89 | 0.6602 | 1149.7 | 383.6 | |
| 0.00 | 3.60 | 0.00 | 2.41 | -15.77 | 120.12 | -36.48 | 121.88 | 0.6762 | 693.0 | 506.4 | |
| 0.53 | 2.19 | 0.35 | 1.47 | -15.43 | 119.84 | -36.76 | 121.25 | 0.6772 | 695.0 | 542.4 | |
| 8.69 | 23.61 | 5.83 | 15.84 | -15.12 | 119.71 | -36.89 | 120.76 | 0.6767 | 865.1 | 460.7 | |
| 2.02 | 2.90 | 1.37 | 1.97 | -15.25 | 118.78 | -37.82 | 120.32 | 0.6877 | 535.8 | 318.8 | |
| 0.00 | 1.14 | 0.00 | 0.77 | -14.54 | 118.89 | -37.71 | 119.46 | 0.6824 | 535.0 | 482.6 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -14.91 | 118.10 | -38.50 | 119.45 | 0.6932 | 677.0 | 560.6 | |
| 0.00 | 1.05 | 0.00 | 0.74 | -15.23 | 116.91 | -39.69 | 119.13 | 0.7078 | -637.0 | -514.2 | |
| 0.00 | 1.49 | 0.00 | 1.04 | -14.62 | 116.88 | -39.72 | 118.34 | 0.7049 | -748.0 | -624.2 | |
| 0.44 | 2.37 | 0.31 | 1.65 | -14.31 | 116.70 | -39.90 | 117.84 | 0.7052 | -860.4 | -736.3 | |
| 0.00 | 1.32 | 0.00 | 0.93 | -14.70 | 116.25 | -40.35 | 118.07 | 0.7120 | -787.0 | -636.5 | |
| 0.00 | 3.16 | 0.00 | 2.30 | -15.61 | 114.42 | -42.18 | 118.19 | 0.7360 | -650.0 | -519.2 | |
| 0.00 | 3.69 | 0.00 | 2.67 | -14.99 | 114.57 | -42.03 | 117.50 | 0.7314 | -688.0 | -590.0 | |
| 0.00 | 1.76 | 0.00 | 1.26 | -13.74 | 114.70 | -41.90 | 115.98 | 0.7240 | -540.0 | -454.0 | |
| 0.00 | 2.02 | 0.00 | 1.45 | -14.01 | 114.43 | -42.17 | 116.19 | 0.7283 | -727.0 | -623.2 | |
| 1.32 | 2.02 | 0.97 | 1.49 | -15.41 | 113.62 | -42.98 | 117.52 | 0.7434 | -469.9 | -487.6 | |
| 18.60 | 83.72 | 13.72 | 61.87 | -14.55 | 113.24 | -43.36 | 116.25 | 0.7433 | -885.2 | -222.1 | |
| 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. | |