SDO HMI 2011-10-09 13:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.67 | 225.59 | 16.63 | 122.32 | 23.61 | 154.56 | 17.18 | 318.19 | 0.4094 | -664.1 | -376.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.49 | 27.40 | 156.93 | 19.55 | 320.94 | 0.4735 | -615.0 | -450.1 | |
| 0.00 | 4.12 | 0.00 | 2.31 | 27.34 | 156.63 | 19.26 | 321.26 | 0.4700 | -670.0 | -479.3 | |
| 3.15 | 208.39 | 1.71 | 112.94 | 23.20 | 155.21 | 17.83 | 316.46 | 0.4102 | -1175.4 | -438.5 | |
| 2.19 | -3.00 | 1.19 | -3.00 | 22.98 | 155.11 | 17.73 | 316.21 | 0.4069 | -1195.2 | 999999 | |
| 25.33 | -3.00 | 13.73 | -3.00 | 23.36 | 154.89 | 17.51 | 317.24 | 0.4086 | -1365.5 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 22.89 | 152.89 | 15.51 | 319.63 | 0.3820 | 533.0 | 435.1 | |
| 0.00 | 1.67 | 0.00 | 0.89 | 25.45 | 150.03 | 12.65 | 329.14 | 0.3873 | 714.0 | 569.1 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 25.36 | 149.72 | 12.34 | 329.63 | 0.3836 | 743.0 | 560.7 | |
| 0.00 | 1.84 | 0.00 | 0.98 | 24.66 | 148.70 | 11.33 | 330.66 | 0.3658 | 876.0 | 645.1 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 26.16 | 148.20 | 10.82 | 333.77 | 0.3830 | 612.0 | 491.4 | |
| 0.00 | 1.93 | 0.00 | 1.03 | 25.91 | 147.94 | 10.56 | 333.99 | 0.3776 | 951.0 | 719.3 | |
| 0.00 | 1.40 | 0.00 | 0.75 | 25.87 | 146.25 | 8.87 | 337.61 | 0.3659 | 803.0 | 549.2 | |
| 0.00 | 2.37 | 0.00 | 1.33 | 34.47 | 139.98 | 2.60 | 355.47 | 0.4762 | 549.0 | 545.2 | |
| 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. | |