SDO HMI 2011-12-04 03:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90.81 | 402.54 | 47.61 | 210.93 | 19.52 | 123.75 | -0.73 | 2.24 | 0.3287 | 229.8 | 147.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.48 | 0.00 | 1.33 | 20.00 | 136.79 | 12.31 | 329.00 | 0.3907 | 898.0 | 674.2 | |
| 7.51 | 17.76 | 3.96 | 9.36 | 20.26 | 127.71 | 3.23 | 351.10 | 0.3432 | -980.5 | -689.7 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 20.38 | 127.14 | 2.67 | 352.68 | 0.3439 | -668.0 | -559.4 | |
| 12.46 | 22.71 | 6.55 | 11.94 | 19.91 | 126.92 | 2.44 | 353.13 | 0.3357 | -1126.9 | -848.4 | |
| 1.37 | -4.00 | 0.72 | -4.00 | 20.20 | 126.86 | 2.38 | 353.40 | 0.3402 | -839.2 | 999999 | |
| 0.68 | 3.76 | 0.36 | 1.97 | 19.88 | 126.48 | 2.00 | 354.35 | 0.3344 | -1088.4 | -839.2 | |
| 1.28 | 29.62 | 0.67 | 15.62 | 20.32 | 126.26 | 1.78 | 355.08 | 0.3413 | -995.8 | -739.0 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 19.41 | 126.06 | 1.58 | 355.40 | 0.3261 | -943.0 | -746.8 | |
| 2.13 | -7.00 | 1.13 | -7.00 | 20.92 | 126.05 | 1.57 | 355.81 | 0.3508 | -770.6 | 999999 | |
| 0.00 | 2.39 | 0.00 | 1.25 | 19.19 | 125.87 | 1.39 | 355.89 | 0.3222 | -908.0 | -703.8 | |
| 1.79 | 8.62 | 0.94 | 4.52 | 19.51 | 125.72 | 1.24 | 356.41 | 0.3272 | -1081.8 | -851.5 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 18.70 | 125.56 | 1.08 | 356.73 | 0.3136 | -977.0 | -779.2 | |
| 2.05 | 3.41 | 1.07 | 1.78 | 18.85 | 125.46 | 0.98 | 357.04 | 0.3161 | -991.2 | -958.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 21.11 | 125.45 | 0.97 | 357.43 | 0.3534 | -656.0 | -560.0 | |
| 1.28 | 5.81 | 0.67 | 3.04 | 19.35 | 125.31 | 0.83 | 357.57 | 0.3243 | -1028.3 | -844.0 | |
| 0.00 | 1.96 | 0.00 | 1.03 | 20.20 | 125.31 | 0.84 | 357.67 | 0.3383 | -861.0 | -657.9 | |
| 0.00 | 2.39 | 0.00 | 1.25 | 19.60 | 125.22 | 0.74 | 357.87 | 0.3284 | -675.0 | -563.0 | |
| 0.00 | 2.22 | 0.00 | 1.16 | 18.98 | 125.12 | 0.64 | 358.08 | 0.3180 | -684.0 | -409.8 | |
| 0.00 | 4.10 | 0.00 | 2.14 | 19.29 | 125.00 | 0.52 | 358.48 | 0.3231 | -757.0 | -645.6 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.66 | 124.75 | 0.27 | 359.23 | 0.3292 | -614.0 | -441.6 | |
| 0.00 | 3.93 | 0.00 | 2.05 | 18.60 | 124.31 | -0.17 | 0.52 | 0.3116 | 1114.0 | 856.3 | |
| 1.88 | 6.40 | 0.98 | 3.35 | 19.23 | 124.28 | -0.20 | 0.59 | 0.3219 | 626.0 | -68.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 19.98 | 123.87 | -0.61 | 1.73 | 0.3345 | 800.0 | 496.4 | |
| 0.00 | 2.31 | 0.00 | 1.22 | 20.83 | 123.83 | -0.65 | 1.74 | 0.3485 | -1023.0 | -757.0 | |
| 0.85 | 263.37 | 0.45 | 137.71 | 19.66 | 123.12 | -1.36 | 3.91 | 0.3299 | -294.9 | 459.7 | |
| 14.34 | -25.00 | 7.51 | -25.00 | 19.38 | 123.09 | -1.39 | 4.06 | 0.3253 | 998.0 | 999999 | |
| 0.00 | 2.48 | 0.00 | 1.32 | 22.15 | 122.77 | -1.71 | 4.28 | 0.3711 | 774.0 | 702.8 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 22.15 | 122.49 | -1.99 | 4.99 | 0.3715 | 686.0 | 588.2 | |
| 37.90 | -25.00 | 19.82 | -25.00 | 19.10 | 122.40 | -2.08 | 6.14 | 0.3217 | 1252.3 | 999999 | |
| 0.00 | 2.05 | 0.00 | 1.08 | 21.11 | 122.18 | -2.29 | 6.07 | 0.3550 | 782.0 | 555.1 | |
| 2.22 | 3.07 | 1.17 | 1.63 | 20.89 | 121.97 | -2.51 | 6.72 | 0.3518 | 916.7 | 785.7 | |
| 2.73 | -25.00 | 1.43 | -25.00 | 19.79 | 121.95 | -2.53 | 7.17 | 0.3339 | 756.7 | 999999 | |
| 0.34 | 1.28 | 0.18 | 0.68 | 20.42 | 121.82 | -2.66 | 7.30 | 0.3444 | 927.5 | 790.8 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 21.17 | 121.74 | -2.74 | 7.21 | 0.3569 | 805.0 | 583.1 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 20.76 | 121.75 | -2.73 | 7.35 | 0.3502 | 805.0 | 528.1 | |
| 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. | |