SDO HMI 2011-11-14 23:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.22 | 181.06 | 17.65 | 109.28 | 28.34 | 42.13 | 25.03 | 319.35 | 0.5738 | -832.7 | -436.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.95 | 0.00 | 0.62 | 33.68 | 46.44 | 29.34 | 321.74 | 0.6608 | -537.0 | -434.9 | |
| 8.68 | 166.87 | 5.25 | 100.72 | 28.40 | 42.33 | 25.23 | 319.21 | 0.5762 | -1019.0 | -442.5 | |
| 15.30 | -2.00 | 9.23 | -2.00 | 28.10 | 42.26 | 25.16 | 318.90 | 0.5727 | -1231.5 | 999999 | |
| 1.89 | -2.00 | 1.14 | -2.00 | 28.41 | 41.93 | 24.82 | 319.64 | 0.5725 | -938.0 | 999999 | |
| 2.15 | -2.00 | 1.30 | -2.00 | 28.67 | 41.92 | 24.82 | 319.99 | 0.5750 | -779.2 | 999999 | |
| 0.00 | 1.55 | 0.00 | 0.94 | 29.20 | 41.91 | 24.80 | 320.68 | 0.5800 | -361.0 | -305.8 | |
| 1.20 | 1.46 | 0.73 | 0.88 | 28.74 | 41.57 | 24.46 | 320.46 | 0.5724 | -757.6 | -715.7 | |
| 0.00 | 4.04 | 0.00 | 2.43 | 28.48 | 41.43 | 24.32 | 320.27 | 0.5686 | -504.0 | -567.2 | |
| 0.00 | 0.95 | 0.00 | 0.60 | 33.60 | 42.28 | 25.18 | 325.44 | 0.6269 | -693.0 | -563.2 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 28.76 | 40.72 | 23.61 | 321.39 | 0.5649 | -748.0 | -624.2 | |
| 0.00 | 1.20 | 0.00 | 0.72 | 29.71 | 39.76 | 22.66 | 323.62 | 0.5663 | -747.0 | -606.4 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 30.25 | 39.26 | 22.16 | 324.84 | 0.5679 | -685.0 | -496.0 | |
| 0.00 | 1.12 | 0.00 | 0.64 | 26.45 | 36.39 | 19.28 | 323.65 | 0.5010 | 716.0 | 483.8 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 27.16 | 36.37 | 19.27 | 324.61 | 0.5090 | 720.0 | 607.7 | |
| 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. | |