SDO HMI 2011-09-02 01:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 100.75 | 411.85 | 58.70 | 240.47 | 24.54 | 300.09 | 27.72 | 306.71 | 0.5291 | -45.1 | -27.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.42 | 190.77 | 21.78 | 114.12 | 23.31 | 303.65 | 31.28 | 301.65 | 0.5623 | -1026.1 | -340.8 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 20.42 | 302.92 | 30.54 | 297.20 | 0.5376 | -595.0 | -482.8 | |
| 5.55 | -1.00 | 3.31 | -1.00 | 23.61 | 303.31 | 30.93 | 302.38 | 0.5599 | -1065.0 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.76 | 25.95 | 303.88 | 31.51 | 305.71 | 0.5810 | 712.0 | 571.1 | |
| 1.97 | 4.74 | 1.18 | 2.85 | 24.82 | 303.44 | 31.07 | 304.24 | 0.5687 | -599.4 | -673.2 | |
| 1.52 | -1.00 | 0.90 | -1.00 | 23.41 | 302.99 | 30.61 | 302.26 | 0.5548 | -1071.8 | 999999 | |
| 0.00 | 3.58 | 0.00 | 2.13 | 24.29 | 302.71 | 30.34 | 303.89 | 0.5568 | -762.0 | -709.4 | |
| 0.00 | 1.88 | 0.00 | 1.11 | 23.52 | 302.29 | 29.91 | 302.92 | 0.5468 | -897.0 | -702.0 | |
| 0.00 | 1.25 | 0.00 | 0.75 | 24.49 | 302.50 | 30.13 | 304.37 | 0.5555 | -712.0 | -537.8 | |
| 0.00 | 2.68 | 0.00 | 1.59 | 24.03 | 302.19 | 29.81 | 303.84 | 0.5489 | -782.0 | -628.4 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 23.41 | 301.99 | 29.62 | 302.94 | 0.5426 | -724.0 | -634.6 | |
| 2.06 | 2.68 | 1.21 | 1.58 | 24.26 | 301.60 | 29.22 | 304.65 | 0.5432 | -846.6 | -725.4 | |
| 0.00 | 2.33 | 0.00 | 1.37 | 24.43 | 301.34 | 28.96 | 305.14 | 0.5412 | -668.0 | -466.2 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 24.69 | 300.72 | 28.35 | 306.05 | 0.5356 | -563.0 | -433.0 | |
| 1.88 | 3.94 | 1.09 | 2.27 | 23.53 | 299.80 | 27.43 | 304.83 | 0.5166 | 717.6 | 602.1 | |
| 3.13 | 15.66 | 1.83 | 9.12 | 24.95 | 299.99 | 27.62 | 307.08 | 0.5289 | -704.2 | -356.2 | |
| 1.43 | 5.55 | 0.84 | 3.24 | 25.43 | 300.07 | 27.70 | 307.80 | 0.5333 | -695.6 | -670.0 | |
| 0.00 | 1.25 | 0.00 | 0.73 | 25.21 | 299.94 | 27.57 | 307.55 | 0.5302 | -801.0 | -667.4 | |
| 1.52 | -16.00 | 0.89 | -16.00 | 25.00 | 299.74 | 27.36 | 307.37 | 0.5263 | -710.8 | 999999 | |
| 0.00 | 1.43 | 0.00 | 0.83 | 24.73 | 299.45 | 27.07 | 307.17 | 0.5208 | 551.0 | 344.9 | |
| 0.00 | 1.61 | 0.00 | 0.93 | 23.98 | 299.16 | 26.79 | 306.14 | 0.5120 | 708.0 | 578.9 | |
| 1.70 | 2.59 | 0.98 | 1.49 | 24.13 | 298.71 | 26.34 | 306.79 | 0.5077 | 852.1 | 751.4 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 24.75 | 297.82 | 25.44 | 308.68 | 0.5018 | 747.0 | 558.0 | |
| 0.00 | 2.33 | 0.00 | 1.33 | 25.06 | 297.40 | 25.03 | 309.60 | 0.4995 | 650.0 | 471.6 | |
| 2.59 | 13.33 | 1.48 | 7.58 | 25.25 | 296.67 | 24.30 | 310.67 | 0.4927 | 808.7 | 690.8 | |
| 1.61 | -25.00 | 0.91 | -25.00 | 25.26 | 296.53 | 24.15 | 310.83 | 0.4910 | 841.1 | 999999 | |
| 0.00 | 1.88 | 0.00 | 1.06 | 24.85 | 296.44 | 24.07 | 310.21 | 0.4866 | 768.0 | 545.7 | |
| 0.00 | 1.70 | 0.00 | 0.97 | 25.52 | 296.40 | 24.03 | 311.40 | 0.4918 | 584.0 | 569.5 | |
| 13.33 | 43.93 | 7.62 | 25.15 | 26.69 | 296.25 | 23.88 | 313.49 | 0.5004 | 897.5 | 147.8 | |
| 0.00 | 1.43 | 0.00 | 0.81 | 26.15 | 296.06 | 23.68 | 312.81 | 0.4935 | 637.0 | 483.8 | |
| 0.00 | 2.59 | 0.00 | 1.47 | 25.40 | 295.68 | 23.30 | 311.96 | 0.4826 | 704.0 | 590.0 | |
| 1.16 | 4.65 | 0.66 | 2.65 | 26.81 | 295.79 | 23.42 | 314.17 | 0.4965 | 784.3 | 517.3 | |
| 0.00 | 2.33 | 0.00 | 1.32 | 26.66 | 295.54 | 23.17 | 314.20 | 0.4924 | 871.0 | 725.8 | |
| 22.55 | 86.44 | 12.70 | 48.67 | 25.75 | 294.98 | 22.61 | 313.32 | 0.4780 | 1124.5 | 590.0 | |
| 2.33 | 2.51 | 1.32 | 1.42 | 26.65 | 295.02 | 22.65 | 314.77 | 0.4868 | 775.2 | 679.5 | |
| 0.00 | 1.97 | 0.00 | 1.10 | 25.38 | 293.93 | 21.56 | 313.92 | 0.4628 | 857.0 | 744.8 | |
| 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. | |