SDO HMI 2011-10-21 17:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.47 | 228.65 | 71.48 | 496.55 | 9.24 | 54.00 | 77.11 | 278.27 | 0.9715 | 56.7 | -18.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.18 | 140.42 | 5.92 | 357.53 | 7.76 | 57.04 | 80.15 | 276.92 | 0.9842 | 537.5 | 10.4 | |
| 0.00 | 0.61 | 0.00 | 1.53 | 6.74 | 55.97 | 79.09 | 275.81 | 0.9811 | -262.0 | -231.7 | |
| 5.92 | -1.00 | 14.85 | -1.00 | 8.36 | 56.13 | 79.24 | 277.47 | 0.9812 | 324.3 | 999999 | |
| 12.88 | -1.00 | 30.97 | -1.00 | 8.50 | 55.59 | 78.71 | 277.57 | 0.9793 | -431.4 | 999999 | |
| 0.00 | 2.44 | 0.00 | 5.32 | 8.94 | 54.41 | 77.53 | 277.95 | 0.9749 | -401.0 | -365.2 | |
| 0.00 | 10.79 | 0.00 | 23.06 | 9.75 | 54.17 | 77.29 | 278.77 | 0.9738 | -659.0 | -513.1 | |
| 2.00 | 7.92 | 3.27 | 13.10 | 9.65 | 49.89 | 73.01 | 278.44 | 0.9545 | 85.7 | -270.4 | |
| 0.00 | 1.13 | 0.00 | 1.75 | 10.68 | 48.84 | 71.96 | 279.48 | 0.9487 | 121.0 | 47.5 | |
| 0.00 | 1.22 | 0.00 | 1.84 | 10.39 | 48.38 | 71.50 | 279.15 | 0.9462 | 463.0 | 356.7 | |
| 9.66 | 49.51 | 13.86 | 71.44 | 12.18 | 47.35 | 70.47 | 281.03 | 0.9401 | 573.8 | 59.2 | |
| 0.00 | 1.13 | 0.00 | 1.64 | 12.63 | 47.53 | 70.65 | 281.50 | 0.9411 | 315.0 | 239.2 | |
| 0.00 | 0.78 | 0.00 | 1.12 | 13.14 | 47.22 | 70.34 | 282.04 | 0.9392 | 451.0 | 463.6 | |
| 1.83 | 11.83 | 2.61 | 17.23 | 13.41 | 47.31 | 70.43 | 282.33 | 0.9397 | 503.8 | 19.8 | |
| 0.00 | 0.87 | 0.00 | 0.99 | 9.29 | 41.43 | 64.55 | 277.73 | 0.9011 | 292.0 | 299.5 | |
| 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. | |