SDO HMI 2011-10-06 13:05:48 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.87 | 219.33 | 59.62 | 243.28 | -14.74 | 117.16 | -60.29 | 110.09 | 0.8950 | 112.2 | 39.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.38 | 107.64 | 7.41 | 109.22 | -15.07 | 120.40 | -57.05 | 111.38 | 0.8722 | 679.2 | 163.4 | |
| 0.79 | -1.00 | 0.81 | -1.00 | -15.08 | 119.64 | -57.81 | 111.16 | 0.8781 | 71.6 | 999999 | |
| 16.77 | -1.00 | 17.08 | -1.00 | -14.62 | 119.78 | -57.67 | 110.70 | 0.8760 | 604.7 | 999999 | |
| 0.00 | 4.65 | 0.00 | 4.72 | -13.89 | 119.78 | -57.67 | 109.89 | 0.8743 | 456.0 | 387.3 | |
| 0.00 | 0.97 | 0.00 | 1.00 | -14.16 | 119.03 | -58.42 | 109.96 | 0.8808 | 391.0 | 321.1 | |
| 1.67 | 2.46 | 1.74 | 2.56 | -13.92 | 118.82 | -58.62 | 109.64 | 0.8818 | 346.9 | 178.8 | |
| 0.88 | 17.12 | 0.92 | 18.27 | -13.71 | 118.43 | -59.02 | 109.30 | 0.8844 | 402.6 | -35.7 | |
| 8.78 | -7.00 | 9.38 | -7.00 | -13.60 | 117.93 | -59.52 | 109.04 | 0.8880 | 327.2 | 999999 | |
| 10.18 | 15.72 | 11.64 | 17.93 | -15.19 | 116.32 | -61.12 | 110.30 | 0.9029 | -486.7 | -453.6 | |
| 0.00 | 0.88 | 0.00 | 1.01 | -14.74 | 116.02 | -61.43 | 109.74 | 0.9041 | -677.0 | -563.8 | |
| 0.00 | 0.70 | 0.00 | 0.82 | -15.08 | 115.79 | -61.66 | 110.04 | 0.9064 | -140.0 | -175.9 | |
| 0.00 | 0.70 | 0.00 | 0.83 | -15.63 | 115.44 | -62.01 | 110.53 | 0.9098 | -255.0 | -207.4 | |
| 0.00 | 1.76 | 0.00 | 2.17 | -15.47 | 114.15 | -63.29 | 110.02 | 0.9180 | -484.0 | -392.1 | |
| 0.00 | 0.97 | 0.00 | 1.21 | -15.44 | 113.89 | -63.55 | 109.91 | 0.9196 | -419.0 | -357.2 | |
| 1.84 | 65.06 | 2.31 | 82.68 | -15.27 | 113.71 | -63.74 | 109.69 | 0.9205 | -565.2 | -48.8 | |
| 6.58 | -15.00 | 8.33 | -15.00 | -14.82 | 113.38 | -64.07 | 109.14 | 0.9219 | -475.3 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.86 | -12.38 | 113.61 | -63.83 | 106.60 | 0.9165 | 181.0 | 59.4 | |
| 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. | |