SDO HMI 2011-11-29 13:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.22 | 73.91 | 14.78 | 49.14 | 18.10 | 223.83 | 38.92 | 296.40 | 0.6690 | -469.0 | -295.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 1.06 | 15.67 | 227.11 | 42.20 | 291.60 | 0.6980 | 654.0 | 545.6 | |
| 0.00 | 1.28 | 0.00 | 0.89 | 16.44 | 227.02 | 42.11 | 292.70 | 0.6995 | 556.0 | 426.9 | |
| 0.00 | 1.28 | 0.00 | 0.84 | 14.03 | 224.06 | 39.15 | 290.39 | 0.6559 | 662.0 | 467.6 | |
| 2.99 | 15.81 | 2.01 | 10.61 | 18.07 | 224.71 | 39.80 | 295.93 | 0.6790 | -496.2 | -493.5 | |
| 3.16 | -4.00 | 2.12 | -4.00 | 17.85 | 224.45 | 39.54 | 295.75 | 0.6751 | -869.8 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.70 | 19.75 | 224.78 | 39.87 | 298.21 | 0.6871 | -672.0 | -550.6 | |
| 0.00 | 2.99 | 0.00 | 1.98 | 17.55 | 223.88 | 38.98 | 295.58 | 0.6672 | -821.0 | -630.2 | |
| 0.00 | 2.22 | 0.00 | 1.48 | 17.86 | 223.92 | 39.02 | 296.00 | 0.6690 | -670.0 | -668.2 | |
| 0.00 | 0.85 | 0.00 | 0.57 | 17.86 | 223.76 | 38.86 | 296.07 | 0.6671 | -840.0 | -787.4 | |
| 16.07 | 43.33 | 10.65 | 28.73 | 18.30 | 223.60 | 38.69 | 296.77 | 0.6671 | -932.8 | -330.3 | |
| 0.00 | 1.11 | 0.00 | 0.73 | 20.40 | 222.46 | 37.56 | 300.31 | 0.6641 | -216.0 | -151.6 | |
| 0.00 | 0.85 | 0.00 | 0.54 | 19.20 | 220.23 | 35.32 | 299.89 | 0.6320 | 584.0 | 526.0 | |
| 0.00 | 0.85 | 0.00 | 0.53 | 18.35 | 218.51 | 33.60 | 299.68 | 0.6068 | 717.0 | 598.4 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 20.57 | 217.78 | 32.88 | 303.47 | 0.6115 | 730.0 | 481.6 | |
| 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. | |