SDO HMI 2011-10-10 20:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.22 | 180.00 | 16.88 | 110.98 | 23.51 | 153.70 | 33.38 | 302.02 | 0.5971 | -480.9 | -302.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.01 | 162.14 | 1.25 | 100.49 | 23.19 | 154.83 | 34.51 | 300.74 | 0.6081 | -819.3 | -400.6 | |
| 1.49 | -1.00 | 0.92 | -1.00 | 22.76 | 154.63 | 34.30 | 300.19 | 0.6035 | -721.1 | 999999 | |
| 0.96 | -1.00 | 0.60 | -1.00 | 22.92 | 154.59 | 34.27 | 300.45 | 0.6039 | -693.5 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.56 | 26.56 | 155.52 | 35.20 | 305.34 | 0.6343 | -503.0 | -408.1 | |
| 22.76 | -1.00 | 14.11 | -1.00 | 23.28 | 154.34 | 34.02 | 301.15 | 0.6028 | -1161.6 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.66 | 26.52 | 154.57 | 34.25 | 305.86 | 0.6236 | -545.0 | -433.9 | |
| 0.00 | 1.66 | 0.00 | 0.97 | 23.47 | 147.74 | 27.42 | 306.10 | 0.5249 | 753.0 | 620.7 | |
| 0.00 | 1.84 | 0.00 | 1.09 | 25.73 | 148.25 | 27.93 | 309.32 | 0.5475 | 602.0 | 496.5 | |
| 0.00 | 2.36 | 0.00 | 1.39 | 25.89 | 147.69 | 27.37 | 310.06 | 0.5424 | 644.0 | 585.2 | |
| 0.00 | 1.40 | 0.00 | 0.81 | 26.25 | 145.99 | 25.67 | 312.21 | 0.5266 | 725.0 | 574.1 | |
| 0.00 | 1.66 | 0.00 | 0.98 | 29.01 | 145.71 | 25.38 | 316.63 | 0.5480 | 619.0 | 532.0 | |
| 0.00 | 1.49 | 0.00 | 0.86 | 25.79 | 144.82 | 24.49 | 312.66 | 0.5097 | 893.0 | 693.8 | |
| 0.00 | 3.59 | 0.00 | 2.07 | 26.37 | 144.65 | 24.33 | 313.76 | 0.5131 | 736.0 | 679.2 | |
| 0.00 | 0.53 | 0.00 | 0.32 | 33.02 | 145.89 | 25.57 | 321.81 | 0.5876 | 480.0 | 463.8 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 24.05 | 142.24 | 21.92 | 312.62 | 0.4652 | 683.0 | 577.4 | |
| 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. | |