SDO HMI 2011-01-01 00:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.96 | 180.66 | 32.40 | 114.89 | 33.94 | 267.75 | 12.41 | 343.45 | 0.6288 | -7.0 | -40.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.24 | 104.47 | 10.99 | 66.65 | 33.60 | 269.69 | 14.35 | 340.85 | 0.6317 | -1091.5 | -339.5 | |
| 2.12 | -1.00 | 1.35 | -1.00 | 33.41 | 269.11 | 13.77 | 341.44 | 0.6267 | -764.8 | 999999 | |
| 0.00 | 0.76 | 0.00 | 0.48 | 33.00 | 269.01 | 13.67 | 341.32 | 0.6212 | -762.0 | -612.6 | |
| 3.65 | 4.08 | 2.32 | 2.59 | 33.70 | 268.68 | 13.35 | 342.14 | 0.6285 | -791.1 | -657.4 | |
| 0.00 | 1.19 | 0.00 | 0.76 | 34.03 | 268.74 | 13.40 | 342.27 | 0.6330 | -494.0 | -430.7 | |
| 0.00 | 1.36 | 0.00 | 0.84 | 31.75 | 266.79 | 11.45 | 343.46 | 0.5955 | 651.0 | 557.1 | |
| 1.02 | 2.04 | 0.65 | 1.30 | 34.52 | 266.73 | 11.39 | 345.01 | 0.6316 | -820.4 | -625.6 | |
| 1.87 | 11.81 | 1.17 | 7.38 | 33.47 | 265.18 | 9.85 | 346.48 | 0.6126 | 908.5 | 724.0 | |
| 0.00 | 1.27 | 0.00 | 0.81 | 34.96 | 265.22 | 9.88 | 347.10 | 0.6323 | 664.0 | 451.7 | |
| 0.00 | 1.78 | 0.00 | 1.12 | 33.95 | 264.73 | 9.40 | 347.28 | 0.6175 | 675.0 | 536.8 | |
| 4.76 | 10.45 | 3.05 | 6.70 | 35.44 | 264.87 | 9.53 | 347.74 | 0.6376 | 673.3 | 586.5 | |
| 2.55 | 41.45 | 1.61 | 26.26 | 34.28 | 264.74 | 9.40 | 347.42 | 0.6220 | 960.1 | 614.7 | |
| 17.75 | -12.00 | 11.26 | -12.00 | 34.72 | 264.57 | 9.23 | 347.82 | 0.6273 | 864.8 | 999999 | |
| 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. | |