SDO HMI 2011-10-13 13:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.57 | 235.20 | 30.55 | 151.13 | -14.73 | 118.58 | 33.97 | 237.96 | 0.6391 | 280.4 | 197.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.49 | 8.74 | 0.99 | 5.83 | -13.80 | 121.94 | 37.33 | 241.64 | 0.6716 | 649.2 | 562.1 | |
| 2.36 | 2.89 | 1.56 | 1.90 | -13.87 | 121.15 | 36.54 | 241.03 | 0.6629 | 672.6 | 535.7 | |
| 0.00 | 2.89 | 0.00 | 1.90 | -14.29 | 120.68 | 36.08 | 240.17 | 0.6602 | 829.0 | 637.8 | |
| 0.00 | 4.55 | 0.00 | 2.95 | -13.55 | 120.02 | 35.41 | 240.73 | 0.6481 | 902.0 | 668.9 | |
| 0.00 | 1.66 | 0.00 | 1.07 | -13.37 | 119.76 | 35.15 | 240.79 | 0.6441 | 845.0 | 665.6 | |
| 1.40 | 155.01 | 0.91 | 101.01 | -14.04 | 119.80 | 35.19 | 239.90 | 0.6486 | 885.8 | 391.1 | |
| 30.34 | -6.00 | 19.80 | -6.00 | -14.74 | 119.86 | 35.25 | 238.98 | 0.6536 | 993.4 | 999999 | |
| 1.05 | -6.00 | 0.68 | -6.00 | -14.93 | 119.32 | 34.72 | 238.34 | 0.6487 | 907.2 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.39 | -11.27 | 118.73 | 34.13 | 243.10 | 0.6192 | 600.0 | 434.7 | |
| 0.00 | 1.75 | 0.00 | 1.10 | -14.53 | 116.80 | 32.19 | 236.99 | 0.6173 | -569.0 | -551.1 | |
| 0.00 | 4.20 | 0.00 | 2.64 | -14.93 | 116.61 | 32.00 | 236.28 | 0.6180 | -630.0 | -546.8 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -15.21 | 116.48 | 31.87 | 235.78 | 0.6184 | -553.0 | -485.1 | |
| 0.00 | 1.05 | 0.00 | 0.66 | -15.11 | 116.35 | 31.74 | 235.82 | 0.6162 | -669.0 | -581.7 | |
| 0.00 | 0.35 | 0.00 | 0.22 | -15.15 | 115.96 | 31.35 | 235.43 | 0.6121 | -507.0 | -552.8 | |
| 0.00 | 1.49 | 0.00 | 0.92 | -14.31 | 115.24 | 30.64 | 236.01 | 0.5978 | -607.0 | -539.2 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -14.14 | 115.08 | 30.47 | 236.11 | 0.5946 | -650.0 | -611.6 | |
| 2.27 | 2.89 | 1.39 | 1.76 | -13.69 | 114.87 | 30.26 | 236.58 | 0.5888 | 797.4 | 728.1 | |
| 0.00 | 1.05 | 0.00 | 0.65 | -16.41 | 114.94 | 30.33 | 232.82 | 0.6102 | -584.0 | -443.2 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -13.35 | 114.43 | 29.82 | 236.70 | 0.5811 | 603.0 | 489.6 | |
| 0.00 | 3.06 | 0.00 | 1.91 | -16.53 | 114.78 | 30.17 | 232.51 | 0.6094 | -596.0 | -481.7 | |
| 0.00 | 1.40 | 0.00 | 0.85 | -13.21 | 114.16 | 29.55 | 236.68 | 0.5768 | 101.0 | 118.4 | |
| 0.00 | 2.97 | 0.00 | 1.83 | -15.79 | 114.33 | 29.72 | 233.11 | 0.5987 | -783.0 | -707.7 | |
| 0.00 | 2.01 | 0.00 | 1.24 | -15.59 | 114.19 | 29.58 | 233.27 | 0.5955 | -755.0 | -617.9 | |
| 6.91 | 8.92 | 4.16 | 5.37 | -12.96 | 113.74 | 29.13 | 236.67 | 0.5700 | 902.6 | 672.8 | |
| 0.00 | 2.27 | 0.00 | 1.41 | -16.49 | 114.19 | 29.59 | 232.03 | 0.6028 | -802.0 | -676.3 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -16.26 | 114.08 | 29.48 | 232.24 | 0.5997 | -766.0 | -672.9 | |
| 0.00 | 0.87 | 0.00 | 0.54 | -16.55 | 114.06 | 29.45 | 231.83 | 0.6018 | -722.0 | -590.2 | |
| 0.00 | 1.49 | 0.00 | 0.91 | -15.93 | 113.89 | 29.28 | 232.52 | 0.5948 | -759.0 | -623.6 | |
| 0.00 | 1.22 | 0.00 | 0.76 | -16.71 | 113.98 | 29.37 | 231.54 | 0.6022 | -839.0 | -636.9 | |
| 0.00 | 0.96 | 0.00 | 0.60 | -17.25 | 113.86 | 29.25 | 230.69 | 0.6053 | -621.0 | -519.2 | |
| 0.00 | 1.22 | 0.00 | 0.76 | -16.91 | 113.58 | 28.98 | 230.89 | 0.5996 | -722.0 | -618.2 | |
| 1.75 | 13.29 | 1.06 | 8.06 | -15.74 | 112.69 | 28.08 | 231.64 | 0.5799 | -741.0 | -593.0 | |
| 0.00 | 0.70 | 0.00 | 0.42 | -15.35 | 112.52 | 27.91 | 232.04 | 0.5748 | -868.0 | -719.5 | |
| 0.00 | 1.40 | 0.00 | 0.84 | -15.05 | 112.41 | 27.80 | 232.35 | 0.5711 | -908.0 | -790.5 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -17.84 | 112.07 | 27.46 | 228.16 | 0.5914 | -694.0 | -547.8 | |
| 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. | |