SDO HMI 2011-08-10 14:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.66 | 46.82 | 12.36 | 28.16 | 19.87 | 241.70 | 32.52 | 296.58 | 0.5663 | 306.5 | 145.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.54 | 2.80 | 0.35 | 1.82 | 19.09 | 248.69 | 39.50 | 292.10 | 0.6511 | -721.2 | -539.4 | |
| 1.35 | 1.53 | 0.88 | 0.99 | 19.09 | 248.23 | 39.05 | 292.25 | 0.6455 | -704.5 | -626.0 | |
| 0.00 | 1.35 | 0.00 | 0.87 | 18.58 | 247.80 | 38.62 | 291.63 | 0.6386 | -674.0 | -577.4 | |
| 2.98 | 6.41 | 1.87 | 4.02 | 18.36 | 246.03 | 36.85 | 291.89 | 0.6157 | -802.5 | -757.8 | |
| 1.35 | 1.99 | 0.83 | 1.22 | 18.31 | 244.24 | 35.06 | 292.51 | 0.5925 | -803.3 | -728.7 | |
| 0.00 | 1.53 | 0.00 | 0.94 | 18.92 | 243.60 | 34.42 | 293.78 | 0.5865 | -685.0 | -634.4 | |
| 0.00 | 1.35 | 0.00 | 0.80 | 19.90 | 240.63 | 31.45 | 296.94 | 0.5525 | 662.0 | 592.0 | |
| 0.00 | 4.87 | 0.00 | 2.91 | 21.13 | 240.65 | 31.47 | 299.01 | 0.5589 | 799.0 | 572.5 | |
| 0.00 | 1.08 | 0.00 | 0.64 | 21.38 | 240.29 | 31.10 | 299.64 | 0.5556 | 561.0 | 509.9 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 22.30 | 240.13 | 30.95 | 301.29 | 0.5589 | 497.0 | 463.7 | |
| 6.68 | 12.19 | 3.89 | 7.09 | 19.73 | 238.68 | 29.50 | 297.82 | 0.5261 | 982.9 | 748.6 | |
| 1.62 | -11.00 | 0.95 | -11.00 | 20.01 | 238.63 | 29.45 | 298.36 | 0.5270 | 818.4 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.79 | 20.54 | 238.74 | 29.56 | 299.22 | 0.5313 | 722.0 | 563.6 | |
| 6.14 | 7.76 | 3.59 | 4.54 | 21.05 | 238.62 | 29.44 | 300.18 | 0.5328 | 846.9 | 636.8 | |
| 0.00 | 1.62 | 0.00 | 0.94 | 20.76 | 238.23 | 29.04 | 299.95 | 0.5260 | 784.0 | 728.6 | |
| 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. | |