SDO HMI 2011-10-23 22:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.04 | 0.00 | 14.17 | 17.79 | 321.22 | 13.48 | 313.65 | 0.3231 | 713.2 | 623.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.22 | 0.00 | 0.64 | 13.30 | 326.23 | 18.48 | 295.26 | 0.3426 | 676.0 | 482.2 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 14.59 | 325.46 | 17.71 | 299.62 | 0.3402 | 694.0 | 566.8 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 17.25 | 324.79 | 17.04 | 307.23 | 0.3531 | 801.0 | 624.2 | |
| 0.00 | 1.83 | 0.00 | 0.97 | 17.66 | 324.46 | 16.72 | 308.67 | 0.3527 | 922.0 | 764.3 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 15.51 | 323.82 | 16.08 | 304.36 | 0.3247 | 719.0 | 537.7 | |
| 0.00 | 3.74 | 0.00 | 1.93 | 12.96 | 321.80 | 14.06 | 300.20 | 0.2751 | 950.0 | 822.0 | |
| 0.00 | 3.83 | 0.00 | 1.97 | 12.51 | 321.71 | 13.97 | 298.87 | 0.2703 | 940.0 | 763.7 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 16.18 | 320.92 | 13.18 | 311.37 | 0.2931 | 744.0 | 563.7 | |
| 0.00 | 1.39 | 0.00 | 0.73 | 20.01 | 321.03 | 13.28 | 320.07 | 0.3378 | 759.0 | 627.2 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 20.85 | 320.64 | 12.90 | 322.51 | 0.3443 | 762.0 | 599.5 | |
| 0.00 | 1.91 | 0.00 | 1.00 | 20.43 | 320.12 | 12.37 | 322.82 | 0.3337 | 864.0 | 664.7 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 20.47 | 319.60 | 11.86 | 324.03 | 0.3291 | 801.0 | 611.8 | |
| 0.00 | 1.56 | 0.00 | 0.83 | 22.34 | 319.19 | 11.45 | 328.22 | 0.3502 | 847.0 | 702.9 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 16.62 | 318.79 | 11.05 | 317.39 | 0.2725 | -643.0 | -540.0 | |
| 0.00 | 1.56 | 0.00 | 0.82 | 21.80 | 317.91 | 10.16 | 330.28 | 0.3320 | 740.0 | 485.3 | |
| 0.00 | 3.04 | 0.00 | 1.63 | 25.71 | 317.55 | 9.81 | 336.42 | 0.3853 | 835.0 | 587.1 | |
| 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. | |