SDO HMI 2011-10-18 10:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.68 | 27.82 | 6.14 | 21.32 | 23.70 | 332.13 | -48.17 | 63.49 | 0.7638 | -407.6 | -405.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.26 | 0.00 | 0.18 | 21.22 | 337.75 | -42.55 | 65.09 | 0.6974 | -612.0 | -553.0 | |
| 0.00 | 1.05 | 0.00 | 0.75 | 22.55 | 335.50 | -44.80 | 64.01 | 0.7264 | -648.0 | -604.5 | |
| 0.00 | 0.96 | 0.00 | 0.71 | 25.11 | 334.25 | -46.05 | 61.05 | 0.7474 | -650.0 | -566.4 | |
| 0.00 | 0.87 | 0.00 | 0.63 | 22.66 | 335.36 | -44.94 | 63.90 | 0.7282 | -601.0 | -562.9 | |
| 2.01 | 4.27 | 1.49 | 3.17 | 23.45 | 333.89 | -46.41 | 63.31 | 0.7460 | -643.3 | -614.3 | |
| 0.00 | 1.13 | 0.00 | 0.85 | 24.10 | 333.54 | -46.76 | 62.58 | 0.7515 | -488.0 | -425.6 | |
| 0.00 | 3.84 | 0.00 | 2.84 | 23.11 | 333.95 | -46.35 | 63.74 | 0.7444 | -809.0 | -747.8 | |
| 0.00 | 0.96 | 0.00 | 0.71 | 23.25 | 333.74 | -46.56 | 63.62 | 0.7469 | -588.0 | -512.9 | |
| 0.00 | 3.93 | 0.00 | 2.90 | 22.82 | 333.89 | -46.41 | 64.14 | 0.7442 | -713.0 | -566.2 | |
| 0.00 | 0.79 | 0.00 | 0.60 | 22.96 | 331.80 | -48.49 | 64.54 | 0.7660 | -381.0 | -348.7 | |
| 0.00 | 1.57 | 0.00 | 1.22 | 22.92 | 331.23 | -49.07 | 64.74 | 0.7717 | 424.0 | 403.2 | |
| 0.00 | 0.87 | 0.00 | 0.68 | 22.75 | 330.71 | -49.59 | 65.08 | 0.7765 | 610.0 | 470.9 | |
| 5.67 | 6.45 | 4.65 | 5.30 | 24.72 | 328.78 | -51.52 | 63.10 | 0.7996 | -523.4 | -437.7 | |
| 0.00 | 0.87 | 0.00 | 0.78 | 26.94 | 325.38 | -54.92 | 61.23 | 0.8344 | 455.0 | 453.5 | |
| 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. | |