SDO HMI 2011-09-04 16:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.45 | 119.31 | 23.74 | 140.46 | 23.09 | 303.55 | 65.83 | 292.25 | 0.9066 | -238.8 | -39.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.34 | 93.87 | 1.69 | 116.79 | 22.61 | 305.55 | 67.83 | 291.55 | 0.9208 | 218.5 | -105.1 | |
| 14.20 | -1.00 | 17.61 | -1.00 | 22.58 | 305.18 | 67.46 | 291.53 | 0.9185 | -696.0 | 999999 | |
| 0.00 | 1.25 | 0.00 | 1.48 | 22.86 | 303.85 | 66.14 | 291.89 | 0.9099 | -464.0 | -380.2 | |
| 0.00 | 0.98 | 0.00 | 1.06 | 24.53 | 300.89 | 63.17 | 293.92 | 0.8901 | -397.0 | -320.2 | |
| 0.00 | 0.98 | 0.00 | 1.03 | 24.83 | 299.85 | 62.14 | 294.36 | 0.8827 | -596.0 | -542.0 | |
| 0.00 | 0.80 | 0.00 | 0.79 | 25.18 | 297.84 | 60.13 | 294.97 | 0.8677 | 293.0 | 228.0 | |
| 0.00 | 3.48 | 0.00 | 3.18 | 25.14 | 294.72 | 57.00 | 295.34 | 0.8422 | 551.0 | 465.2 | |
| 0.00 | 0.80 | 0.00 | 0.74 | 25.75 | 295.17 | 57.46 | 295.99 | 0.8468 | 319.0 | 244.7 | |
| 0.00 | 0.89 | 0.00 | 0.82 | 25.57 | 294.97 | 57.26 | 295.81 | 0.8449 | 483.0 | 414.9 | |
| 1.34 | 1.61 | 1.20 | 1.44 | 25.58 | 293.93 | 56.22 | 295.98 | 0.8361 | 531.9 | 473.0 | |
| 0.71 | 3.04 | 0.64 | 2.74 | 25.87 | 294.02 | 56.31 | 296.30 | 0.8372 | 525.9 | 412.1 | |
| 2.86 | 4.29 | 2.60 | 3.90 | 26.60 | 294.26 | 56.55 | 297.13 | 0.8404 | 337.4 | 295.8 | |
| 0.00 | 1.25 | 0.00 | 1.12 | 25.80 | 293.67 | 55.96 | 296.29 | 0.8342 | 651.0 | 526.9 | |
| 0.00 | 0.80 | 0.00 | 0.71 | 25.30 | 293.19 | 55.48 | 295.76 | 0.8293 | 444.0 | 387.7 | |
| 0.00 | 5.27 | 0.00 | 4.66 | 26.08 | 293.21 | 55.49 | 296.69 | 0.8306 | 693.0 | 566.1 | |
| 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. | |