SDO HMI 2011-10-22 02:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.94 | 37.96 | 7.12 | 19.44 | 18.01 | 324.58 | -7.33 | 28.55 | 0.2529 | 554.8 | 328.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.27 | 8.71 | 2.17 | 4.42 | 17.04 | 326.73 | -5.19 | 23.08 | 0.2217 | -1093.9 | -822.4 | |
| 2.18 | 4.35 | 1.11 | 2.21 | 17.16 | 326.38 | -5.54 | 24.22 | 0.2259 | -945.9 | -709.8 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 18.16 | 325.24 | -6.68 | 26.43 | 0.2493 | 897.0 | 747.6 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 17.57 | 324.82 | -7.09 | 29.01 | 0.2439 | 1032.0 | 756.9 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 13.96 | 324.95 | -6.97 | 38.06 | 0.1919 | 706.0 | 644.1 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 14.35 | 324.91 | -7.01 | 36.96 | 0.1976 | 807.0 | 691.5 | |
| 1.83 | 4.61 | 0.94 | 2.37 | 18.82 | 324.01 | -7.91 | 29.13 | 0.2688 | 1093.2 | 927.5 | |
| 5.22 | 7.40 | 2.68 | 3.80 | 18.39 | 323.93 | -7.98 | 30.21 | 0.2632 | 1156.3 | 939.6 | |
| 0.44 | -8.00 | 0.22 | -8.00 | 18.57 | 323.86 | -8.06 | 30.06 | 0.2664 | 1116.6 | 999999 | |
| 0.00 | 3.22 | 0.00 | 1.66 | 18.53 | 323.58 | -8.34 | 30.99 | 0.2684 | 589.0 | 636.4 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 19.20 | 322.68 | -9.24 | 32.23 | 0.2856 | 861.0 | 692.9 | |
| 0.00 | 0.70 | 0.00 | 0.36 | 18.80 | 322.48 | -9.44 | 33.59 | 0.2818 | 793.0 | 560.0 | |
| 0.00 | 1.65 | 0.00 | 0.87 | 21.76 | 320.73 | -11.19 | 32.38 | 0.3381 | 872.0 | 702.9 | |
| 0.00 | 1.57 | 0.00 | 0.82 | 20.17 | 320.20 | -11.72 | 36.50 | 0.3220 | 876.0 | 690.8 | |
| 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. | |