| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.01 | 378.43 | 80.51 | 399.97 | -13.76 | 120.62 | -59.67 | 108.12 | 0.8833 | 323.9 | 126.2 | |
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back to the solar disc SDO HMI 2011-11-02 14:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.99 | 231.20 | 8.73 | 229.13 | -14.72 | 123.53 | -56.76 | 109.89 | 0.8623 | 884.2 | 201.8 | |
| 10.29 | -1.00 | 10.22 | -1.00 | -15.17 | 122.89 | -57.40 | 110.22 | 0.8685 | 541.7 | 999999 | |
| 2.94 | -1.00 | 2.94 | -1.00 | -15.52 | 122.67 | -57.62 | 110.56 | 0.8710 | 326.7 | 999999 | |
| 20.58 | -1.00 | 20.32 | -1.00 | -14.63 | 122.94 | -57.35 | 109.63 | 0.8670 | 671.0 | 999999 | |
| 3.03 | -1.00 | 3.09 | -1.00 | -14.98 | 121.92 | -58.37 | 109.75 | 0.8759 | -323.3 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.88 | -13.45 | 121.49 | -58.80 | 107.94 | 0.8764 | 309.0 | 224.3 | |
| 1.73 | 3.03 | 1.81 | 3.18 | -13.57 | 120.60 | -59.69 | 107.86 | 0.8837 | 210.2 | 48.1 | |
| 1.56 | 2.33 | 1.72 | 2.58 | -14.54 | 119.16 | -61.13 | 108.58 | 0.8962 | -527.3 | -492.8 | |
| 0.00 | 4.67 | 0.00 | 5.15 | -13.37 | 118.99 | -61.30 | 107.26 | 0.8955 | -682.0 | -562.9 | |
| 0.00 | 1.21 | 0.00 | 1.41 | -15.03 | 117.87 | -62.42 | 108.82 | 0.9062 | -564.0 | -528.6 | |
| 1.56 | 27.06 | 1.84 | 32.53 | -15.43 | 117.52 | -62.77 | 109.17 | 0.9092 | -574.8 | -82.3 | |
| 1.21 | -11.00 | 1.43 | -11.00 | -15.09 | 117.36 | -62.93 | 108.78 | 0.9098 | -455.8 | 999999 | |
| 0.43 | -11.00 | 0.52 | -11.00 | -15.45 | 117.16 | -63.12 | 109.12 | 0.9117 | -230.2 | 999999 | |
| 1.90 | -11.00 | 2.27 | -11.00 | -15.26 | 117.20 | -63.09 | 108.92 | 0.9112 | -301.8 | 999999 | |
| 1.73 | -11.00 | 2.09 | -11.00 | -15.66 | 116.91 | -63.38 | 109.28 | 0.9137 | -186.4 | 999999 | |
| 1.21 | -11.00 | 1.47 | -11.00 | -15.67 | 116.69 | -63.60 | 109.25 | 0.9152 | 221.6 | 999999 | |
| 2.33 | 4.06 | 2.75 | 4.80 | -13.98 | 117.25 | -63.04 | 107.55 | 0.9089 | -664.8 | -518.3 | |
| 0.00 | 0.95 | 0.00 | 1.18 | -15.40 | 116.07 | -64.22 | 108.83 | 0.9189 | -290.0 | -193.3 | |
| 7.87 | 95.20 | 8.88 | 109.08 | -10.89 | 117.85 | -62.44 | 104.31 | 0.9003 | 748.6 | 109.1 | |
| 0.00 | 0.86 | 0.00 | 1.06 | -14.05 | 116.17 | -64.12 | 107.40 | 0.9164 | 400.0 | 374.9 | |
| 0.00 | 1.21 | 0.00 | 1.45 | -12.76 | 116.60 | -63.69 | 106.09 | 0.9117 | -374.0 | -340.9 | |
| 6.23 | -19.00 | 7.17 | -19.00 | -10.99 | 117.28 | -63.01 | 104.31 | 0.9046 | 327.2 | 999999 | |
| 2.42 | 2.94 | 3.26 | 3.95 | -15.66 | 114.12 | -66.16 | 108.70 | 0.9314 | -364.2 | -404.7 | |
| 0.00 | 0.78 | 0.00 | 0.93 | -10.30 | 116.17 | -64.12 | 103.35 | 0.9116 | 451.0 | 426.1 | |
| 0.00 | 0.86 | 0.00 | 1.17 | -14.96 | 113.87 | -66.42 | 107.91 | 0.9321 | -214.0 | -228.0 | |
| 0.00 | 1.21 | 0.00 | 1.49 | -9.87 | 115.26 | -65.03 | 102.73 | 0.9173 | 233.0 | 210.4 | |
| 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. | |