SDO HMI 2011-09-04 10:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.40 | 134.97 | 20.62 | 141.51 | 23.21 | 303.22 | 62.20 | 292.65 | 0.8807 | -128.8 | -17.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.27 | 105.22 | 18.00 | 116.61 | 22.64 | 305.19 | 64.17 | 291.74 | 0.8962 | -762.1 | -121.9 | |
| 0.00 | 1.97 | 0.00 | 1.69 | 25.69 | 295.28 | 54.25 | 296.45 | 0.8191 | 462.0 | 331.9 | |
| 0.00 | 1.07 | 0.00 | 0.91 | 25.14 | 294.91 | 53.89 | 295.85 | 0.8149 | 472.0 | 429.8 | |
| 0.00 | 3.04 | 0.00 | 2.57 | 25.05 | 294.75 | 53.72 | 295.78 | 0.8132 | 650.0 | 506.7 | |
| 0.00 | 1.61 | 0.00 | 1.37 | 25.55 | 294.96 | 53.93 | 296.35 | 0.8160 | 435.0 | 428.7 | |
| 0.00 | 0.89 | 0.00 | 0.76 | 25.85 | 294.64 | 53.61 | 296.77 | 0.8136 | 402.0 | 335.6 | |
| 0.00 | 2.32 | 0.00 | 1.94 | 25.51 | 294.02 | 53.00 | 296.48 | 0.8075 | 572.0 | 536.7 | |
| 1.34 | 2.23 | 1.12 | 1.87 | 25.83 | 294.17 | 53.15 | 296.83 | 0.8094 | 525.8 | 429.0 | |
| 0.00 | 1.70 | 0.00 | 1.44 | 26.60 | 294.63 | 53.61 | 297.68 | 0.8150 | 317.0 | 237.7 | |
| 1.43 | 2.41 | 1.21 | 2.04 | 26.66 | 294.38 | 53.36 | 297.80 | 0.8129 | 469.4 | 296.8 | |
| 0.00 | 0.89 | 0.00 | 0.75 | 25.86 | 293.85 | 52.83 | 296.94 | 0.8065 | 414.0 | 368.2 | |
| 0.00 | 2.06 | 0.00 | 1.70 | 25.79 | 293.58 | 52.56 | 296.90 | 0.8039 | 705.0 | 543.4 | |
| 0.36 | 1.07 | 0.29 | 0.88 | 25.27 | 293.15 | 52.13 | 296.36 | 0.7989 | 470.2 | 444.6 | |
| 0.00 | 4.29 | 0.00 | 3.55 | 26.23 | 293.42 | 52.40 | 297.48 | 0.8033 | 563.0 | 454.2 | |
| 0.00 | 1.16 | 0.00 | 0.96 | 25.93 | 293.12 | 52.10 | 297.18 | 0.7999 | 511.0 | 577.6 | |
| 0.00 | 0.36 | 0.00 | 0.30 | 26.75 | 293.15 | 52.12 | 298.17 | 0.8018 | 602.0 | 571.8 | |
| 0.00 | 0.89 | 0.00 | 0.73 | 26.26 | 292.78 | 51.75 | 297.66 | 0.7974 | 661.0 | 537.6 | |
| 0.00 | 1.79 | 0.00 | 1.44 | 26.19 | 292.03 | 51.01 | 297.75 | 0.7903 | 602.0 | 458.9 | |
| 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. | |