SDO HMI 2011-12-01 11:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.42 | 256.36 | 15.51 | 161.46 | 20.33 | 192.95 | 33.30 | 303.34 | 0.6184 | -70.5 | -218.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.06 | 199.03 | 3.89 | 127.12 | 19.86 | 194.97 | 35.32 | 301.11 | 0.6374 | -820.8 | -375.6 | |
| 16.40 | -1.00 | 10.45 | -1.00 | 19.68 | 194.54 | 34.89 | 301.11 | 0.6314 | -1212.2 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.76 | 21.73 | 193.27 | 33.62 | 304.88 | 0.6293 | -705.0 | -627.1 | |
| 0.00 | 1.37 | 0.00 | 0.85 | 19.63 | 192.18 | 32.53 | 302.60 | 0.6035 | -696.0 | -516.3 | |
| 0.00 | 2.82 | 0.00 | 1.74 | 21.37 | 190.95 | 31.30 | 306.06 | 0.6008 | -781.0 | -662.2 | |
| 0.00 | 1.45 | 0.00 | 0.89 | 20.84 | 190.71 | 31.07 | 305.46 | 0.5944 | -868.0 | -790.2 | |
| 0.00 | 1.54 | 0.00 | 0.96 | 22.16 | 191.03 | 31.38 | 307.13 | 0.6072 | -654.0 | -545.7 | |
| 0.00 | 1.11 | 0.00 | 0.68 | 21.41 | 190.36 | 30.72 | 306.57 | 0.5944 | -801.0 | -697.8 | |
| 0.00 | 2.56 | 0.00 | 1.50 | 15.42 | 188.95 | 29.31 | 298.21 | 0.5376 | -646.0 | -544.1 | |
| 0.00 | 1.11 | 0.00 | 0.65 | 15.61 | 188.70 | 29.05 | 298.72 | 0.5355 | -736.0 | -546.9 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 19.91 | 187.90 | 28.25 | 306.39 | 0.5550 | 611.0 | 442.8 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 23.01 | 188.09 | 28.44 | 310.81 | 0.5815 | 101.0 | 164.3 | |
| 0.00 | 0.85 | 0.00 | 0.52 | 22.38 | 187.73 | 28.08 | 310.23 | 0.5724 | 470.0 | 458.5 | |
| 0.00 | 0.85 | 0.00 | 0.51 | 21.90 | 187.59 | 27.94 | 309.67 | 0.5670 | 812.0 | 709.3 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 22.06 | 186.83 | 27.18 | 310.62 | 0.5599 | 629.0 | 561.8 | |
| 0.00 | 1.62 | 0.00 | 0.97 | 22.03 | 186.54 | 26.89 | 310.85 | 0.5565 | 834.0 | 724.1 | |
| 1.96 | 2.82 | 1.17 | 1.68 | 22.38 | 186.54 | 26.89 | 311.36 | 0.5594 | 684.6 | 620.6 | |
| 0.00 | 3.42 | 0.00 | 2.03 | 22.23 | 186.33 | 26.68 | 311.34 | 0.5558 | 888.0 | 714.9 | |
| 0.00 | 2.22 | 0.00 | 1.31 | 21.88 | 186.04 | 26.39 | 311.11 | 0.5497 | 778.0 | 656.6 | |
| 0.00 | 1.28 | 0.00 | 0.76 | 22.55 | 186.04 | 26.39 | 312.09 | 0.5554 | 772.0 | 596.6 | |
| 0.00 | 1.79 | 0.00 | 1.06 | 22.17 | 185.82 | 26.17 | 311.76 | 0.5497 | 877.0 | 662.5 | |
| 0.00 | 2.82 | 0.00 | 1.70 | 25.25 | 185.62 | 25.97 | 316.28 | 0.5753 | 546.0 | 525.8 | |
| 0.00 | 3.76 | 0.00 | 2.22 | 22.93 | 185.05 | 25.40 | 313.67 | 0.5482 | 777.0 | 722.8 | |
| 0.00 | 3.50 | 0.00 | 2.08 | 23.74 | 184.92 | 25.28 | 314.93 | 0.5543 | 777.0 | 735.6 | |
| 0.00 | 1.28 | 0.00 | 0.76 | 23.03 | 184.67 | 25.03 | 314.20 | 0.5452 | 821.0 | 626.5 | |
| 0.00 | 3.08 | 0.00 | 1.83 | 24.06 | 184.85 | 25.20 | 315.46 | 0.5565 | 598.0 | 528.1 | |
| 0.00 | 1.45 | 0.00 | 0.85 | 22.87 | 184.47 | 24.82 | 314.19 | 0.5415 | 687.0 | 629.7 | |
| 0.00 | 1.37 | 0.00 | 0.83 | 25.94 | 184.98 | 25.33 | 317.85 | 0.5755 | 761.0 | 596.5 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 26.17 | 184.99 | 25.34 | 318.13 | 0.5778 | 684.0 | 532.2 | |
| 0.00 | 1.96 | 0.00 | 1.20 | 26.89 | 184.98 | 25.33 | 319.06 | 0.5847 | 724.0 | 553.8 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 24.00 | 184.16 | 24.51 | 316.11 | 0.5489 | 812.0 | 663.6 | |
| 0.00 | 1.20 | 0.00 | 0.72 | 25.39 | 184.31 | 24.66 | 317.84 | 0.5638 | 817.0 | 652.9 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 26.24 | 184.35 | 24.71 | 318.89 | 0.5724 | 753.0 | 661.1 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 21.48 | 182.95 | 23.30 | 313.82 | 0.5123 | 768.0 | 600.7 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 25.95 | 181.99 | 22.35 | 321.19 | 0.5476 | 804.0 | 689.3 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 22.80 | 180.58 | 20.94 | 318.66 | 0.5007 | 427.0 | 505.6 | |
| 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. | |