SDO HMI 2011-10-19 00:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.66 | 21.89 | 2.64 | 14.73 | 24.09 | 332.69 | -39.89 | 59.98 | 0.6776 | -568.3 | -482.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.87 | 28.29 | 335.88 | -36.71 | 52.58 | 0.6650 | -653.0 | -519.4 | |
| 0.00 | 0.87 | 0.00 | 0.54 | 19.16 | 337.70 | -34.89 | 65.10 | 0.5979 | -616.0 | -471.8 | |
| 0.00 | 1.92 | 0.00 | 1.24 | 23.03 | 335.50 | -37.09 | 60.22 | 0.6418 | -779.0 | -562.2 | |
| 0.00 | 1.31 | 0.00 | 0.85 | 22.79 | 335.09 | -37.50 | 60.78 | 0.6454 | -748.0 | -639.5 | |
| 0.00 | 1.66 | 0.00 | 1.10 | 24.65 | 333.82 | -38.77 | 58.71 | 0.6683 | -600.0 | -562.4 | |
| 0.00 | 1.40 | 0.00 | 0.91 | 22.96 | 334.29 | -38.30 | 60.90 | 0.6554 | -534.0 | -507.2 | |
| 0.00 | 0.87 | 0.00 | 0.58 | 24.32 | 333.64 | -38.94 | 59.26 | 0.6687 | -607.0 | -527.2 | |
| 0.00 | 2.27 | 0.00 | 1.49 | 23.39 | 333.93 | -38.65 | 60.45 | 0.6613 | -837.0 | -586.5 | |
| 0.00 | 1.57 | 0.00 | 1.03 | 22.74 | 334.16 | -38.43 | 61.29 | 0.6559 | -761.0 | -618.7 | |
| 0.00 | 0.87 | 0.00 | 0.57 | 23.01 | 334.06 | -38.52 | 60.93 | 0.6582 | -522.0 | -453.1 | |
| 0.00 | 1.13 | 0.00 | 0.75 | 24.06 | 333.53 | -39.06 | 59.68 | 0.6689 | -649.0 | -501.5 | |
| 0.00 | 0.96 | 0.00 | 0.64 | 23.46 | 332.47 | -40.11 | 61.00 | 0.6781 | -559.0 | -455.8 | |
| 3.66 | 4.88 | 2.64 | 3.52 | 25.21 | 328.29 | -44.30 | 60.29 | 0.7298 | -632.4 | -475.6 | |
| 0.00 | 0.87 | 0.00 | 0.64 | 26.12 | 327.48 | -45.11 | 59.40 | 0.7414 | 646.0 | 562.4 | |
| 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. | |