SDO HMI 2011-09-03 02:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.47 | 257.21 | 41.11 | 177.66 | 23.92 | 300.97 | 42.36 | 297.62 | 0.6949 | 109.1 | -78.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.61 | 158.41 | 21.35 | 114.33 | 23.04 | 304.28 | 45.67 | 295.02 | 0.7288 | -922.3 | -284.2 | |
| 0.00 | 6.98 | 0.00 | 4.93 | 23.46 | 303.02 | 44.40 | 295.96 | 0.7162 | -755.0 | -628.3 | |
| 0.00 | 0.98 | 0.00 | 0.69 | 23.75 | 302.68 | 44.06 | 296.46 | 0.7133 | -708.0 | -564.4 | |
| 0.00 | 0.98 | 0.00 | 0.68 | 23.61 | 301.30 | 42.68 | 296.71 | 0.6977 | -644.0 | -525.8 | |
| 1.16 | 1.88 | 0.80 | 1.29 | 24.80 | 300.80 | 42.18 | 298.54 | 0.6962 | -680.7 | -514.4 | |
| 0.00 | 1.43 | 0.00 | 0.98 | 26.17 | 299.85 | 41.24 | 300.80 | 0.6910 | -528.0 | -411.5 | |
| 0.00 | 1.34 | 0.00 | 0.91 | 25.98 | 299.05 | 40.44 | 300.86 | 0.6816 | -815.0 | -652.5 | |
| 0.00 | 0.98 | 0.00 | 0.64 | 25.13 | 297.06 | 38.45 | 300.53 | 0.6559 | 628.0 | 529.5 | |
| 0.00 | 1.16 | 0.00 | 0.76 | 25.69 | 296.46 | 37.85 | 301.62 | 0.6516 | 526.0 | 419.9 | |
| 0.00 | 2.24 | 0.00 | 1.44 | 25.42 | 295.73 | 37.11 | 301.59 | 0.6421 | 911.0 | 598.6 | |
| 0.00 | 1.52 | 0.00 | 0.98 | 25.64 | 295.73 | 37.11 | 301.92 | 0.6431 | 674.0 | 581.5 | |
| 0.00 | 4.65 | 0.00 | 2.99 | 25.53 | 295.43 | 36.82 | 301.91 | 0.6393 | 710.0 | 621.5 | |
| 3.67 | 13.77 | 2.38 | 8.91 | 26.85 | 295.67 | 37.05 | 303.69 | 0.6484 | 435.4 | 376.4 | |
| 0.00 | 1.25 | 0.00 | 0.80 | 25.21 | 295.03 | 36.41 | 301.64 | 0.6331 | 588.0 | 474.0 | |
| 0.00 | 0.54 | 0.00 | 0.35 | 26.34 | 295.43 | 36.82 | 303.09 | 0.6433 | 477.0 | 418.7 | |
| 6.89 | -13.00 | 4.45 | -13.00 | 26.67 | 295.39 | 36.77 | 303.59 | 0.6444 | 772.0 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.40 | 25.44 | 294.90 | 36.28 | 302.05 | 0.6328 | 531.0 | 540.7 | |
| 0.00 | 1.07 | 0.00 | 0.69 | 26.17 | 295.16 | 36.54 | 302.98 | 0.6393 | 520.0 | 440.4 | |
| 0.00 | 3.67 | 0.00 | 2.33 | 25.46 | 294.66 | 36.04 | 302.21 | 0.6301 | 886.0 | 726.5 | |
| 1.07 | 7.51 | 0.69 | 4.80 | 25.81 | 294.74 | 36.12 | 302.68 | 0.6328 | 859.0 | 689.5 | |
| 0.00 | 1.97 | 0.00 | 1.26 | 26.23 | 294.76 | 36.15 | 303.28 | 0.6352 | 595.0 | 525.9 | |
| 0.00 | 1.25 | 0.00 | 0.80 | 26.94 | 294.81 | 36.20 | 304.28 | 0.6395 | 676.0 | 498.9 | |
| 0.00 | 1.79 | 0.00 | 1.14 | 26.44 | 294.50 | 35.89 | 303.73 | 0.6334 | 680.0 | 542.8 | |
| 1.43 | 4.56 | 0.91 | 2.89 | 25.62 | 294.17 | 35.56 | 302.71 | 0.6254 | 831.6 | 788.1 | |
| 0.00 | 1.07 | 0.00 | 0.68 | 26.00 | 294.27 | 35.65 | 303.22 | 0.6284 | 788.0 | 642.2 | |
| 7.16 | 8.68 | 4.50 | 5.46 | 25.13 | 293.80 | 35.19 | 302.18 | 0.6186 | 925.3 | 671.2 | |
| 0.00 | 1.16 | 0.00 | 0.74 | 26.50 | 294.19 | 35.57 | 303.99 | 0.6302 | 708.0 | 537.5 | |
| 3.22 | 11.00 | 2.06 | 7.00 | 26.95 | 294.23 | 35.61 | 304.62 | 0.6331 | 631.7 | 642.1 | |
| 4.47 | -28.00 | 2.84 | -28.00 | 26.71 | 293.85 | 35.24 | 304.50 | 0.6276 | 860.9 | 999999 | |
| 1.79 | 2.50 | 1.13 | 1.58 | 26.37 | 293.69 | 35.07 | 304.08 | 0.6239 | 779.5 | 620.1 | |
| 0.00 | 1.34 | 0.00 | 0.86 | 27.36 | 293.92 | 35.30 | 305.40 | 0.6319 | 581.0 | 397.2 | |
| 0.00 | 0.81 | 0.00 | 0.50 | 25.13 | 292.94 | 34.33 | 302.65 | 0.6087 | 593.0 | 509.2 | |
| 0.00 | 1.16 | 0.00 | 0.73 | 25.93 | 292.96 | 34.35 | 303.86 | 0.6133 | 763.0 | 708.2 | |
| 0.00 | 1.97 | 0.00 | 1.16 | 22.38 | 289.15 | 30.54 | 300.57 | 0.5478 | 596.0 | 477.5 | |
| 0.00 | 1.61 | 0.00 | 0.92 | 21.44 | 285.85 | 27.23 | 301.25 | 0.5002 | 695.0 | 576.6 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 22.39 | 285.64 | 27.03 | 303.14 | 0.5038 | 804.0 | 676.4 | |
| 0.00 | 1.34 | 0.00 | 0.76 | 21.22 | 285.26 | 26.64 | 301.31 | 0.4912 | 761.0 | 644.6 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 21.07 | 285.05 | 26.43 | 301.20 | 0.4876 | 737.0 | 631.4 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 23.05 | 281.28 | 22.67 | 308.46 | 0.4547 | 723.0 | 655.8 | |
| 0.00 | 0.89 | 0.00 | 0.51 | 27.81 | 280.00 | 21.38 | 318.09 | 0.4847 | 677.0 | 597.2 | |
| 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. | |