SDO HMI 2011-10-11 04:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.19 | 161.37 | 20.37 | 104.80 | 23.48 | 153.76 | 37.83 | 299.60 | 0.6489 | -518.1 | -284.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.86 | 24.63 | 158.84 | 42.92 | 298.98 | 0.7099 | -623.0 | -473.0 | |
| 6.83 | 144.48 | 4.48 | 94.27 | 23.04 | 154.63 | 38.70 | 298.46 | 0.6568 | -783.2 | -361.7 | |
| 24.36 | -2.00 | 15.89 | -2.00 | 23.29 | 154.21 | 38.29 | 299.01 | 0.6531 | -1108.9 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.71 | 26.92 | 155.47 | 39.54 | 303.54 | 0.6833 | -495.0 | -375.9 | |
| 0.00 | 1.31 | 0.00 | 0.89 | 26.84 | 155.21 | 39.29 | 303.55 | 0.6803 | -443.0 | -363.3 | |
| 0.00 | 0.70 | 0.00 | 0.46 | 26.26 | 153.15 | 37.22 | 303.80 | 0.6551 | -670.0 | -584.4 | |
| 0.00 | 1.05 | 0.00 | 0.66 | 22.92 | 150.96 | 35.04 | 300.07 | 0.6133 | 694.0 | 506.4 | |
| 0.00 | 2.45 | 0.00 | 1.51 | 25.26 | 148.34 | 32.42 | 305.21 | 0.5957 | 406.0 | 412.4 | |
| 0.00 | 0.96 | 0.00 | 0.58 | 23.68 | 147.66 | 31.73 | 303.22 | 0.5780 | 691.0 | 470.5 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 25.79 | 144.86 | 28.94 | 308.61 | 0.5597 | 732.0 | 637.7 | |
| 0.00 | 0.96 | 0.00 | 0.58 | 26.78 | 144.94 | 29.02 | 310.05 | 0.5680 | 518.0 | 460.2 | |
| 0.00 | 1.14 | 0.00 | 0.68 | 26.60 | 144.78 | 28.85 | 309.91 | 0.5647 | 877.0 | 762.2 | |
| 0.00 | 0.88 | 0.00 | 0.52 | 26.25 | 144.64 | 28.72 | 309.50 | 0.5606 | 842.0 | 662.6 | |
| 0.00 | 2.80 | 0.00 | 1.68 | 26.89 | 144.71 | 28.78 | 310.42 | 0.5662 | 682.0 | 486.8 | |
| 0.00 | 1.31 | 0.00 | 0.77 | 24.30 | 143.55 | 27.62 | 307.33 | 0.5335 | 630.0 | 463.6 | |
| 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. | |