SDO HMI 2011-10-20 08:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.77 | 37.83 | 5.80 | 22.41 | -21.11 | 334.68 | -20.33 | 143.78 | 0.5503 | 38.9 | -115.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.05 | 1.48 | 0.61 | 0.86 | -20.35 | 337.31 | -17.71 | 146.54 | 0.5193 | 765.6 | 666.2 | |
| 0.00 | 3.31 | 0.00 | 1.92 | -20.47 | 336.79 | -18.22 | 145.92 | 0.5250 | 707.0 | 725.8 | |
| 0.00 | 1.66 | 0.00 | 0.97 | -20.81 | 336.58 | -18.43 | 146.01 | 0.5308 | 799.0 | 610.8 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -20.89 | 336.30 | -18.71 | 145.70 | 0.5340 | 605.0 | 419.8 | |
| 0.00 | 1.31 | 0.00 | 0.76 | -20.66 | 336.13 | -18.89 | 145.19 | 0.5327 | 729.0 | 695.4 | |
| 0.00 | 1.57 | 0.00 | 0.91 | -20.09 | 336.13 | -18.88 | 144.55 | 0.5261 | 827.0 | 620.9 | |
| 0.00 | 1.31 | 0.00 | 0.77 | -20.86 | 336.03 | -18.98 | 145.29 | 0.5359 | 663.0 | 493.4 | |
| 1.05 | 1.57 | 0.61 | 0.92 | -20.33 | 334.99 | -20.03 | 143.25 | 0.5388 | 650.8 | 612.7 | |
| 0.00 | 3.49 | 0.00 | 2.08 | -21.49 | 334.17 | -20.84 | 143.52 | 0.5590 | -768.0 | -682.1 | |
| 2.27 | 14.90 | 1.35 | 8.89 | -21.10 | 334.06 | -20.95 | 142.92 | 0.5555 | -801.8 | -670.0 | |
| 0.00 | 1.13 | 0.00 | 0.67 | -20.26 | 334.18 | -20.83 | 142.09 | 0.5451 | 638.0 | 380.0 | |
| 0.00 | 1.31 | 0.00 | 0.79 | -21.98 | 333.68 | -21.33 | 143.45 | 0.5686 | -696.0 | -644.4 | |
| 3.92 | -10.00 | 2.34 | -10.00 | -21.41 | 333.74 | -21.28 | 142.87 | 0.5618 | -920.8 | 999999 | |
| 1.48 | 4.01 | 0.89 | 2.41 | -21.86 | 333.39 | -21.62 | 142.94 | 0.5698 | -623.5 | -504.8 | |
| 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. | |