SDO HMI 2011-10-10 23:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.21 | 159.91 | 27.93 | 82.51 | 19.96 | 110.23 | -8.44 | 29.71 | 0.2785 | 105.0 | 185.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.49 | 0.00 | 0.76 | 19.98 | 115.54 | -3.13 | 12.16 | 0.2450 | 790.0 | 635.9 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 22.27 | 112.21 | -6.46 | 20.56 | 0.2978 | 908.0 | 718.1 | |
| 25.66 | 64.89 | 13.17 | 33.33 | 19.98 | 112.21 | -6.46 | 23.86 | 0.2624 | -1125.5 | -323.6 | |
| 1.40 | -3.00 | 0.72 | -3.00 | 19.85 | 111.71 | -6.96 | 25.71 | 0.2640 | -827.9 | 999999 | |
| 0.00 | 1.40 | 0.00 | 0.72 | 19.81 | 111.13 | -7.54 | 27.58 | 0.2678 | -853.0 | -564.6 | |
| 0.00 | 1.40 | 0.00 | 0.72 | 20.30 | 110.56 | -8.11 | 28.40 | 0.2794 | -749.0 | -501.7 | |
| 0.00 | 2.19 | 0.00 | 1.15 | 23.18 | 109.83 | -8.83 | 25.71 | 0.3269 | 904.0 | 740.6 | |
| 0.00 | 0.53 | 0.00 | 0.27 | 20.65 | 109.38 | -9.29 | 31.05 | 0.2942 | -669.0 | -496.2 | |
| 0.00 | 1.93 | 0.00 | 0.99 | 19.45 | 109.32 | -9.35 | 33.60 | 0.2781 | 1102.0 | 900.0 | |
| 6.22 | 80.57 | 3.21 | 41.67 | 19.81 | 109.20 | -9.47 | 33.16 | 0.2842 | 1024.0 | 474.7 | |
| 0.00 | 1.66 | 0.00 | 0.86 | 19.29 | 109.20 | -9.47 | 34.26 | 0.2771 | 1027.0 | 829.7 | |
| 20.93 | -10.00 | 10.83 | -10.00 | 19.74 | 108.59 | -10.08 | 34.93 | 0.2889 | 1103.7 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 19.27 | 108.11 | -10.56 | 37.20 | 0.2875 | 849.0 | 532.8 | |
| 0.00 | 1.66 | 0.00 | 0.90 | 24.99 | 104.55 | -14.12 | 34.22 | 0.3949 | 853.0 | 620.7 | |
| 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. | |