SDO HMI 2011-10-18 03:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.92 | 38.14 | 10.85 | 31.91 | 24.11 | 331.61 | -52.52 | 64.09 | 0.8061 | -358.2 | -237.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 0.77 | 20.94 | 337.43 | -46.70 | 66.72 | 0.7422 | -493.0 | -353.3 | |
| 0.00 | 2.88 | 0.00 | 2.24 | 23.94 | 335.04 | -49.09 | 63.48 | 0.7742 | -518.0 | -490.2 | |
| 0.00 | 1.05 | 0.00 | 0.83 | 24.29 | 334.14 | -49.99 | 63.28 | 0.7838 | -490.0 | -476.1 | |
| 0.00 | 1.05 | 0.00 | 0.83 | 24.16 | 334.16 | -49.97 | 63.43 | 0.7834 | -638.0 | -537.8 | |
| 2.01 | 6.98 | 1.59 | 5.56 | 23.45 | 333.98 | -50.15 | 64.37 | 0.7835 | -756.9 | -458.1 | |
| 2.27 | 3.49 | 1.80 | 2.78 | 23.21 | 333.79 | -50.34 | 64.72 | 0.7847 | -696.0 | -602.9 | |
| 0.00 | 0.87 | 0.00 | 0.69 | 22.74 | 333.93 | -50.20 | 65.27 | 0.7824 | -569.0 | -484.6 | |
| 1.31 | 4.10 | 1.04 | 3.27 | 22.82 | 333.69 | -50.44 | 65.23 | 0.7849 | -484.5 | -356.6 | |
| 0.00 | 1.05 | 0.00 | 0.86 | 24.22 | 332.35 | -51.78 | 63.80 | 0.8007 | -342.0 | -241.1 | |
| 0.00 | 0.52 | 0.00 | 0.44 | 23.35 | 330.92 | -53.21 | 65.18 | 0.8123 | 263.0 | 207.7 | |
| 1.31 | 2.01 | 1.10 | 1.69 | 23.00 | 331.01 | -53.12 | 65.58 | 0.8109 | 480.1 | 235.2 | |
| 6.02 | 9.08 | 5.32 | 8.03 | 24.59 | 329.14 | -54.99 | 64.05 | 0.8305 | -540.9 | -222.3 | |
| 0.00 | 2.09 | 0.00 | 2.05 | 27.63 | 325.56 | -58.57 | 61.18 | 0.8648 | 422.0 | 283.2 | |
| 0.00 | 1.92 | 0.00 | 1.87 | 26.79 | 325.69 | -58.44 | 62.13 | 0.8625 | 565.0 | 403.5 | |
| 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. | |