SDO HMI 2011-11-11 21:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.27 | 336.11 | 25.37 | 188.73 | 28.11 | 44.05 | -13.70 | 26.38 | 0.4725 | -1076.3 | -444.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.87 | 0.00 | 2.21 | 31.34 | 46.58 | -11.18 | 19.35 | 0.5018 | -898.0 | -709.2 | |
| 0.00 | 1.72 | 0.00 | 0.99 | 31.48 | 46.35 | -11.41 | 19.61 | 0.5048 | -723.0 | -549.7 | |
| 0.00 | 1.12 | 0.00 | 0.65 | 32.69 | 45.47 | -12.29 | 19.99 | 0.5259 | -609.0 | -470.3 | |
| 0.00 | 0.60 | 0.00 | 0.36 | 35.54 | 43.69 | -14.07 | 20.28 | 0.5729 | -675.0 | -563.0 | |
| 38.30 | 316.06 | 21.45 | 177.09 | 27.87 | 44.21 | -13.54 | 26.37 | 0.4681 | -1362.4 | -440.4 | |
| 3.70 | -5.00 | 2.08 | -5.00 | 28.25 | 43.82 | -13.94 | 26.60 | 0.4760 | -858.5 | 999999 | |
| 1.81 | -5.00 | 1.02 | -5.00 | 27.99 | 43.58 | -14.18 | 27.27 | 0.4742 | -798.7 | 999999 | |
| 1.46 | -5.00 | 0.82 | -5.00 | 28.19 | 43.55 | -14.21 | 27.10 | 0.4769 | -585.4 | 999999 | |
| 0.00 | 1.72 | 0.00 | 1.06 | 36.58 | 41.51 | -16.25 | 22.19 | 0.5973 | -753.0 | -634.7 | |
| 0.00 | 1.38 | 0.00 | 0.86 | 37.03 | 40.90 | -16.85 | 22.54 | 0.6061 | -618.0 | -426.6 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 28.36 | 41.71 | -16.05 | 29.73 | 0.4925 | -688.0 | -608.5 | |
| 0.00 | 2.84 | 0.00 | 1.61 | 28.22 | 41.59 | -16.17 | 30.07 | 0.4918 | -785.0 | -532.1 | |
| 0.00 | 4.30 | 0.00 | 2.47 | 29.17 | 41.30 | -16.46 | 29.41 | 0.5059 | -818.0 | -592.3 | |
| 0.00 | 1.55 | 0.00 | 0.89 | 26.89 | 38.15 | -19.60 | 36.55 | 0.5046 | 802.0 | 613.9 | |
| 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. | |