SDO HMI 2011-09-01 15:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 92.13 | 405.30 | 51.46 | 226.86 | 24.65 | 300.00 | 22.11 | 312.47 | 0.4651 | -5.5 | -20.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.57 | 200.92 | 8.87 | 114.36 | 23.62 | 303.57 | 25.68 | 306.55 | 0.4962 | -1085.2 | -367.1 | |
| 7.42 | -1.00 | 4.21 | -1.00 | 23.29 | 303.28 | 25.39 | 306.23 | 0.4902 | -1349.1 | 999999 | |
| 7.60 | -1.00 | 4.32 | -1.00 | 23.74 | 303.19 | 25.30 | 307.10 | 0.4925 | -1071.5 | 999999 | |
| 1.52 | -1.00 | 0.87 | -1.00 | 24.09 | 303.08 | 25.19 | 307.83 | 0.4939 | -750.4 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 20.42 | 302.28 | 24.39 | 301.74 | 0.4569 | -819.0 | -688.1 | |
| 4.29 | -1.00 | 2.43 | -1.00 | 23.79 | 302.84 | 24.95 | 307.53 | 0.4886 | -1046.0 | 999999 | |
| 0.00 | 1.34 | 0.00 | 0.77 | 25.40 | 303.11 | 25.22 | 310.04 | 0.5047 | 702.0 | 541.7 | |
| 7.60 | -1.00 | 4.30 | -1.00 | 23.81 | 302.48 | 24.58 | 307.91 | 0.4844 | -1103.0 | 999999 | |
| 0.00 | 5.55 | 0.00 | 3.14 | 24.32 | 302.40 | 24.51 | 308.89 | 0.4876 | -518.0 | -590.0 | |
| 0.00 | 2.59 | 0.00 | 1.46 | 23.30 | 301.87 | 23.98 | 307.60 | 0.4730 | -783.0 | -704.8 | |
| 0.00 | 1.34 | 0.00 | 0.75 | 23.37 | 301.74 | 23.85 | 307.86 | 0.4720 | -685.0 | -636.8 | |
| 0.00 | 1.70 | 0.00 | 0.96 | 24.50 | 301.20 | 23.31 | 310.45 | 0.4751 | -606.0 | -608.6 | |
| 0.00 | 1.70 | 0.00 | 0.95 | 24.58 | 300.96 | 23.07 | 310.84 | 0.4729 | -1063.0 | -765.6 | |
| 0.00 | 2.24 | 0.00 | 1.24 | 23.20 | 300.66 | 22.77 | 308.68 | 0.4576 | 637.0 | 404.9 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 25.09 | 300.99 | 23.10 | 311.70 | 0.4777 | 471.0 | 319.5 | |
| 0.00 | 1.88 | 0.00 | 1.04 | 23.37 | 300.23 | 22.34 | 309.48 | 0.4539 | 649.0 | 464.0 | |
| 1.34 | 2.77 | 0.74 | 1.54 | 23.84 | 299.75 | 21.85 | 310.89 | 0.4522 | 840.3 | 586.2 | |
| 1.61 | 6.17 | 0.90 | 3.44 | 24.86 | 299.68 | 21.79 | 312.79 | 0.4608 | -841.6 | -772.9 | |
| 0.00 | 1.43 | 0.00 | 0.80 | 25.85 | 299.69 | 21.80 | 314.48 | 0.4702 | -804.0 | -662.6 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 24.81 | 299.45 | 21.56 | 312.96 | 0.4577 | -754.0 | -720.2 | |
| 0.00 | 2.50 | 0.00 | 1.38 | 24.30 | 298.62 | 20.72 | 313.09 | 0.4435 | 678.0 | 540.1 | |
| 0.00 | 1.79 | 0.00 | 1.00 | 26.54 | 298.70 | 20.81 | 316.82 | 0.4663 | -964.0 | -736.5 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 24.80 | 297.99 | 20.10 | 314.78 | 0.4413 | 643.0 | 339.3 | |
| 1.79 | 9.93 | 0.98 | 5.46 | 24.79 | 297.60 | 19.71 | 315.27 | 0.4368 | 749.7 | 821.5 | |
| 3.13 | -24.00 | 1.72 | -24.00 | 24.89 | 297.37 | 19.48 | 315.77 | 0.4354 | 958.1 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.69 | 24.94 | 296.95 | 19.06 | 316.42 | 0.4313 | 625.0 | 586.8 | |
| 0.00 | 1.52 | 0.00 | 0.84 | 26.09 | 297.11 | 19.22 | 318.16 | 0.4450 | 593.0 | 427.7 | |
| 15.57 | 39.00 | 8.62 | 21.60 | 26.78 | 296.69 | 18.80 | 319.87 | 0.4482 | 963.2 | 344.6 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 26.20 | 296.52 | 18.63 | 319.18 | 0.4403 | 630.0 | 560.2 | |
| 0.00 | 1.70 | 0.00 | 0.93 | 26.09 | 296.18 | 18.29 | 319.47 | 0.4355 | 716.0 | 523.6 | |
| 2.68 | 17.27 | 1.48 | 9.52 | 26.62 | 295.84 | 17.95 | 320.82 | 0.4380 | 940.7 | 450.3 | |
| 22.01 | 91.25 | 12.02 | 49.79 | 25.67 | 295.44 | 17.55 | 319.85 | 0.4234 | 1190.9 | 587.5 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 26.57 | 295.30 | 17.41 | 321.55 | 0.4322 | 732.0 | 601.8 | |
| 0.00 | 1.16 | 0.00 | 0.63 | 25.55 | 294.23 | 16.34 | 321.54 | 0.4099 | 1056.0 | 842.6 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 25.40 | 293.86 | 15.97 | 321.89 | 0.4045 | 786.0 | 602.5 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 25.23 | 290.94 | 13.05 | 326.85 | 0.3751 | -716.0 | -505.2 | |
| 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. | |