SDO HMI 2011-10-22 01:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.93 | 46.47 | 7.12 | 23.82 | 17.81 | 324.76 | -7.71 | 30.19 | 0.2530 | 464.2 | 332.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.27 | 15.15 | 3.19 | 7.70 | 16.98 | 326.75 | -5.72 | 25.28 | 0.2244 | -1064.8 | -634.2 | |
| 1.48 | 2.96 | 0.75 | 1.51 | 17.16 | 326.36 | -6.10 | 26.36 | 0.2299 | -1022.4 | -905.2 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 14.27 | 325.49 | -6.98 | 37.11 | 0.1961 | 899.0 | 665.4 | |
| 0.00 | 1.92 | 0.00 | 0.98 | 18.16 | 325.22 | -7.25 | 28.33 | 0.2537 | 949.0 | 728.4 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 17.54 | 324.81 | -7.66 | 30.96 | 0.2482 | 950.0 | 773.0 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 13.99 | 324.94 | -7.53 | 40.10 | 0.1982 | 785.0 | 656.1 | |
| 0.00 | 1.39 | 0.00 | 0.70 | 14.32 | 324.90 | -7.57 | 39.17 | 0.2030 | 878.0 | 676.3 | |
| 2.00 | 5.22 | 1.03 | 2.69 | 18.79 | 324.02 | -8.45 | 30.81 | 0.2728 | 1046.9 | 887.3 | |
| 4.18 | 9.14 | 2.15 | 4.70 | 18.36 | 323.95 | -8.52 | 31.91 | 0.2673 | 1120.3 | 1030.7 | |
| 0.00 | 1.57 | 0.00 | 0.81 | 18.53 | 323.52 | -8.95 | 32.77 | 0.2736 | 886.0 | 730.5 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 18.26 | 323.51 | -8.96 | 33.40 | 0.2700 | 830.0 | 703.7 | |
| 0.00 | 1.65 | 0.00 | 0.87 | 21.79 | 320.72 | -11.75 | 33.58 | 0.3434 | 776.0 | 677.9 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 20.17 | 320.23 | -12.24 | 37.67 | 0.3270 | 850.0 | 688.4 | |
| 0.00 | 2.00 | 0.00 | 1.05 | 20.23 | 319.80 | -12.67 | 38.49 | 0.3321 | 820.0 | 633.8 | |
| 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. | |