SDO HMI 2011-10-09 22:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.42 | 193.02 | 18.09 | 107.42 | 23.49 | 154.10 | 21.68 | 312.00 | 0.4578 | -399.7 | -361.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.40 | 172.69 | 3.57 | 96.37 | 23.08 | 155.08 | 22.67 | 309.96 | 0.4645 | -1068.7 | -490.5 | |
| 24.88 | -1.00 | 13.89 | -1.00 | 23.35 | 154.71 | 22.29 | 310.86 | 0.4624 | -1292.1 | 999999 | |
| 1.14 | 1.75 | 0.63 | 0.97 | 22.23 | 153.75 | 21.34 | 309.94 | 0.4411 | 414.2 | 534.3 | |
| 0.00 | 1.49 | 0.00 | 0.82 | 23.69 | 152.18 | 19.76 | 314.61 | 0.4368 | 672.0 | 494.9 | |
| 0.00 | 1.31 | 0.00 | 0.72 | 25.81 | 150.45 | 18.04 | 320.60 | 0.4411 | 696.0 | 489.9 | |
| 0.00 | 2.02 | 0.00 | 1.11 | 25.63 | 150.11 | 17.70 | 320.82 | 0.4357 | 875.0 | 675.3 | |
| 0.00 | 1.49 | 0.00 | 0.80 | 23.48 | 148.10 | 15.68 | 320.40 | 0.3906 | 794.0 | 692.8 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 25.85 | 148.16 | 15.75 | 324.21 | 0.4195 | 685.0 | 601.4 | |
| 0.00 | 1.40 | 0.00 | 0.76 | 25.89 | 147.93 | 15.51 | 324.66 | 0.4178 | 853.0 | 704.1 | |
| 0.00 | 1.66 | 0.00 | 0.90 | 23.99 | 147.62 | 15.20 | 322.13 | 0.3919 | 954.0 | 727.0 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 26.40 | 147.89 | 15.48 | 325.49 | 0.4238 | 743.0 | 587.9 | |
| 0.00 | 0.53 | 0.00 | 0.28 | 23.81 | 147.49 | 15.08 | 322.02 | 0.3885 | 830.0 | 623.2 | |
| 0.00 | 2.28 | 0.00 | 1.25 | 28.43 | 146.39 | 13.98 | 330.80 | 0.4373 | 562.0 | 480.4 | |
| 0.00 | 2.45 | 0.00 | 1.32 | 26.12 | 145.10 | 12.69 | 330.02 | 0.3965 | 948.0 | 697.2 | |
| 0.00 | 1.84 | 0.00 | 0.97 | 24.30 | 142.20 | 9.79 | 333.53 | 0.3491 | 863.0 | 654.2 | |
| 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. | |