SDO HMI 2011-10-14 15:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.93 | 405.68 | 56.89 | 316.74 | 23.24 | 119.78 | 49.47 | 295.35 | 0.7751 | -861.8 | -326.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.93 | 22.34 | 122.39 | 52.08 | 293.64 | 0.7987 | 499.0 | 403.2 | |
| 0.00 | 0.52 | 0.00 | 0.43 | 22.70 | 122.22 | 51.90 | 294.12 | 0.7977 | 388.0 | 300.2 | |
| 0.00 | 1.31 | 0.00 | 1.06 | 22.30 | 121.59 | 51.27 | 293.76 | 0.7909 | 273.0 | 311.4 | |
| 0.00 | 1.14 | 0.00 | 0.92 | 23.30 | 121.91 | 51.59 | 294.93 | 0.7959 | 381.0 | 397.5 | |
| 0.00 | 0.79 | 0.00 | 0.64 | 23.48 | 121.96 | 51.64 | 295.15 | 0.7968 | 375.0 | 342.0 | |
| 0.87 | 3.23 | 0.69 | 2.55 | 21.52 | 120.64 | 50.32 | 292.98 | 0.7800 | 224.2 | 51.3 | |
| 1.22 | 394.23 | 0.98 | 307.56 | 23.16 | 121.16 | 50.84 | 294.93 | 0.7884 | -187.3 | -345.4 | |
| 3.67 | -7.00 | 2.93 | -7.00 | 23.43 | 120.99 | 50.67 | 295.30 | 0.7873 | 475.2 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.57 | 24.54 | 121.60 | 51.28 | 296.53 | 0.7956 | 324.0 | 293.4 | |
| 1.57 | -7.00 | 1.25 | -7.00 | 22.98 | 120.65 | 50.33 | 294.81 | 0.7831 | -253.6 | 999999 | |
| 0.00 | 2.18 | 0.00 | 1.74 | 24.49 | 120.53 | 50.21 | 296.73 | 0.7853 | 483.0 | 290.4 | |
| 65.60 | -7.00 | 51.04 | -7.00 | 23.25 | 119.62 | 49.31 | 295.40 | 0.7735 | -1159.1 | 999999 | |
| 0.00 | 0.44 | 0.00 | 0.34 | 26.06 | 118.09 | 47.78 | 299.38 | 0.7658 | -531.0 | -417.0 | |
| 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. | |