SDO HMI 2011-10-15 04:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.95 | 101.49 | 14.62 | 98.87 | -14.65 | 119.43 | 56.27 | 249.11 | 0.8630 | 204.0 | 218.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.54 | 88.29 | 2.50 | 87.23 | -14.01 | 120.11 | 56.95 | 250.05 | 0.8672 | 563.9 | 310.8 | |
| 0.52 | -1.00 | 0.52 | -1.00 | -14.26 | 120.09 | 56.94 | 249.77 | 0.8677 | 606.7 | 999999 | |
| 7.34 | -1.00 | 7.28 | -1.00 | -14.79 | 120.02 | 56.87 | 249.16 | 0.8684 | 636.9 | 999999 | |
| 3.50 | -1.00 | 3.44 | -1.00 | -14.43 | 119.82 | 56.66 | 249.50 | 0.8658 | 931.0 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.71 | -14.82 | 116.34 | 53.18 | 247.92 | 0.8373 | -399.0 | -370.1 | |
| 0.00 | 3.23 | 0.00 | 2.93 | -15.74 | 116.26 | 53.10 | 246.85 | 0.8393 | -455.0 | -366.1 | |
| 0.00 | 1.14 | 0.00 | 1.03 | -15.92 | 116.22 | 53.07 | 246.63 | 0.8396 | -512.0 | -379.9 | |
| 0.00 | 1.14 | 0.00 | 1.03 | -16.11 | 116.19 | 53.04 | 246.40 | 0.8398 | -472.0 | -383.5 | |
| 0.00 | 0.61 | 0.00 | 0.54 | -16.17 | 115.39 | 52.24 | 246.04 | 0.8330 | -298.0 | -337.6 | |
| 0.00 | 0.70 | 0.00 | 0.60 | -14.31 | 114.44 | 51.28 | 247.83 | 0.8186 | -407.0 | -307.9 | |
| 0.00 | 1.49 | 0.00 | 1.32 | -16.85 | 115.04 | 51.88 | 245.14 | 0.8321 | -484.0 | -413.4 | |
| 0.00 | 0.52 | 0.00 | 0.46 | -16.38 | 114.81 | 51.65 | 245.58 | 0.8285 | -608.0 | -489.5 | |
| 0.00 | 0.61 | 0.00 | 0.53 | -16.30 | 114.28 | 51.12 | 245.46 | 0.8235 | -571.0 | -500.9 | |
| 1.05 | 2.97 | 0.88 | 2.49 | -14.23 | 113.43 | 50.28 | 247.55 | 0.8089 | -614.2 | -574.8 | |
| 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. | |