SDO HMI 2011-12-10 06:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.24 | 349.19 | 43.02 | 287.92 | -17.26 | 352.65 | -51.13 | 111.57 | 0.8018 | 686.1 | 278.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.36 | 1.53 | 1.10 | 1.24 | -18.94 | 354.11 | -49.66 | 114.05 | 0.7918 | -330.4 | -384.5 | |
| 0.00 | 4.01 | 0.00 | 3.26 | -18.91 | 353.64 | -50.14 | 113.87 | 0.7964 | 592.0 | 446.2 | |
| 0.00 | 0.77 | 0.00 | 0.64 | -20.03 | 352.70 | -51.07 | 114.94 | 0.8083 | -667.0 | -592.6 | |
| 11.25 | 331.88 | 9.28 | 273.31 | -18.19 | 352.90 | -50.88 | 112.77 | 0.8016 | 910.1 | 297.3 | |
| 34.18 | -4.00 | 28.10 | -4.00 | -16.92 | 352.71 | -51.07 | 111.17 | 0.8004 | 972.9 | 999999 | |
| 0.00 | 3.92 | 0.00 | 3.29 | -18.22 | 352.04 | -51.74 | 112.57 | 0.8099 | -254.0 | -165.6 | |
| 5.45 | -4.00 | 4.54 | -4.00 | -17.38 | 352.23 | -51.55 | 111.61 | 0.8061 | 439.3 | 999999 | |
| 0.00 | 1.28 | 0.00 | 1.07 | -15.13 | 351.62 | -52.16 | 108.72 | 0.8072 | 519.0 | 392.5 | |
| 0.00 | 1.11 | 0.00 | 0.92 | -14.61 | 351.60 | -52.18 | 108.08 | 0.8064 | -480.0 | -449.5 | |
| 0.00 | 1.11 | 0.00 | 0.94 | -15.25 | 351.07 | -52.71 | 108.74 | 0.8128 | -434.0 | -426.8 | |
| 0.00 | 0.68 | 0.00 | 0.58 | -15.28 | 350.75 | -53.03 | 108.71 | 0.8159 | -617.0 | -553.4 | |
| 0.00 | 1.28 | 0.00 | 1.11 | -16.33 | 350.20 | -53.58 | 109.83 | 0.8231 | -556.0 | -523.5 | |
| 0.00 | 1.62 | 0.00 | 1.56 | -16.93 | 346.20 | -57.58 | 109.69 | 0.8598 | 173.0 | 155.4 | |
| 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. | |