SDO HMI 2011-10-18 02:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.17 | 33.26 | 11.21 | 28.25 | 24.08 | 331.40 | -53.28 | 64.30 | 0.8129 | -385.3 | -194.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.35 | 0.00 | 0.26 | 20.59 | 337.38 | -47.30 | 67.35 | 0.7478 | -641.0 | -653.5 | |
| 0.00 | 0.79 | 0.00 | 0.59 | 20.73 | 337.22 | -47.46 | 67.20 | 0.7498 | -482.0 | -363.0 | |
| 0.00 | 0.96 | 0.00 | 0.77 | 24.15 | 334.15 | -50.53 | 63.59 | 0.7887 | -610.0 | -551.0 | |
| 0.00 | 0.79 | 0.00 | 0.64 | 24.41 | 333.75 | -50.93 | 63.37 | 0.7932 | -488.0 | -389.9 | |
| 2.36 | 13.79 | 1.89 | 11.09 | 23.44 | 333.97 | -50.71 | 64.52 | 0.7888 | -810.0 | -533.2 | |
| 2.09 | -5.00 | 1.69 | -5.00 | 23.51 | 333.67 | -51.01 | 64.50 | 0.7919 | -358.6 | 999999 | |
| 1.57 | -5.00 | 1.26 | -5.00 | 23.20 | 333.78 | -50.89 | 64.86 | 0.7901 | -708.4 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.98 | 22.84 | 333.61 | -51.07 | 65.35 | 0.7910 | -677.0 | -496.2 | |
| 0.00 | 0.61 | 0.00 | 0.49 | 22.65 | 333.71 | -50.97 | 65.56 | 0.7897 | -537.0 | -475.9 | |
| 0.61 | 2.09 | 0.52 | 1.79 | 22.98 | 330.91 | -53.77 | 65.74 | 0.8168 | 541.1 | 411.9 | |
| 6.54 | 7.94 | 5.85 | 7.10 | 24.52 | 329.22 | -55.46 | 64.22 | 0.8344 | -510.7 | -257.4 | |
| 0.00 | 0.96 | 0.00 | 0.83 | 23.05 | 330.14 | -54.53 | 65.80 | 0.8238 | 437.0 | 399.1 | |
| 0.00 | 2.01 | 0.00 | 1.99 | 27.59 | 325.62 | -59.05 | 61.32 | 0.8684 | 468.0 | 297.7 | |
| 0.00 | 1.75 | 0.00 | 1.72 | 26.78 | 325.73 | -58.94 | 62.23 | 0.8664 | 479.0 | 392.5 | |
| 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. | |