SDO HMI 2011-10-21 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 |
| 0.00 | 16.73 | 0.00 | 9.03 | 24.86 | 329.46 | -12.37 | 28.88 | 0.3908 | -227.1 | -142.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.00 | 0.00 | 1.04 | 22.51 | 335.77 | -6.05 | 18.29 | 0.3118 | -814.0 | -673.9 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 22.26 | 335.56 | -6.27 | 19.18 | 0.3090 | -793.0 | -582.7 | |
| 0.00 | 1.22 | 0.00 | 0.64 | 22.69 | 332.76 | -9.06 | 25.97 | 0.3334 | -1013.0 | -814.7 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 24.57 | 332.53 | -9.30 | 24.02 | 0.3625 | -839.0 | -645.7 | |
| 0.00 | 0.87 | 0.00 | 0.46 | 24.70 | 332.32 | -9.51 | 24.34 | 0.3657 | -768.0 | -622.8 | |
| 0.00 | 1.31 | 0.00 | 0.69 | 22.68 | 332.30 | -9.52 | 27.09 | 0.3367 | -757.0 | -515.1 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 22.57 | 330.90 | -10.93 | 30.53 | 0.3461 | -814.0 | -691.3 | |
| 0.00 | 1.39 | 0.00 | 0.75 | 24.28 | 329.75 | -12.07 | 30.36 | 0.3789 | -777.0 | -634.9 | |
| 0.00 | 1.22 | 0.00 | 0.68 | 28.00 | 325.86 | -15.96 | 32.07 | 0.4592 | 822.0 | 670.2 | |
| 0.00 | 1.13 | 0.00 | 0.63 | 28.12 | 325.60 | -16.23 | 32.31 | 0.4630 | 748.0 | 562.5 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 27.64 | 325.64 | -16.19 | 32.90 | 0.4566 | 543.0 | 461.5 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 26.36 | 323.59 | -18.23 | 37.75 | 0.4598 | 758.0 | 550.4 | |
| 0.00 | 2.00 | 0.00 | 1.13 | 26.58 | 322.36 | -19.47 | 39.14 | 0.4741 | 752.0 | 640.2 | |
| 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. | |