SDO HMI 2011-10-06 00:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.42 | 169.44 | 66.81 | 248.69 | -14.59 | 116.55 | -67.53 | 108.11 | 0.9414 | 42.6 | -82.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.89 | 63.33 | 13.87 | 81.98 | -14.25 | 119.71 | -64.38 | 108.48 | 0.9231 | 622.6 | 276.2 | |
| 0.79 | -1.00 | 1.02 | -1.00 | -14.54 | 119.41 | -64.68 | 108.71 | 0.9254 | -128.8 | 999999 | |
| 0.97 | -1.00 | 1.26 | -1.00 | -14.30 | 119.25 | -64.84 | 108.42 | 0.9261 | 239.0 | 999999 | |
| 7.82 | 9.40 | 10.42 | 12.52 | -14.77 | 118.76 | -65.32 | 108.79 | 0.9297 | -437.4 | -346.8 | |
| 8.34 | -1.00 | 10.87 | -1.00 | -13.94 | 119.07 | -65.01 | 108.00 | 0.9266 | 596.9 | 999999 | |
| 2.37 | -1.00 | 3.17 | -1.00 | -13.85 | 118.45 | -65.64 | 107.75 | 0.9303 | 360.0 | 999999 | |
| 3.07 | 34.61 | 4.43 | 49.59 | -14.99 | 116.99 | -67.09 | 108.60 | 0.9403 | -637.9 | -510.3 | |
| 0.53 | -7.00 | 0.77 | -7.00 | -14.85 | 116.51 | -67.57 | 108.35 | 0.9428 | -624.0 | 999999 | |
| 1.05 | 6.06 | 1.47 | 8.40 | -13.60 | 117.28 | -66.81 | 107.22 | 0.9369 | 171.5 | 255.9 | |
| 1.93 | 4.04 | 3.03 | 6.34 | -15.52 | 115.29 | -68.80 | 108.77 | 0.9502 | -290.4 | -159.5 | |
| 0.00 | 1.93 | 0.00 | 3.15 | -15.01 | 114.42 | -69.67 | 108.06 | 0.9540 | -436.0 | -320.8 | |
| 2.90 | 50.07 | 4.85 | 86.71 | -15.13 | 113.96 | -70.12 | 108.08 | 0.9563 | -244.3 | -88.7 | |
| 5.53 | -12.00 | 9.50 | -12.00 | -14.65 | 113.39 | -70.70 | 107.48 | 0.9586 | -405.0 | 999999 | |
| 1.23 | -12.00 | 2.15 | -12.00 | -14.81 | 113.07 | -71.02 | 107.58 | 0.9602 | 192.5 | 999999 | |
| 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. | |