| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.58 | 181.35 | 36.68 | 217.47 | -23.73 | 284.00 | -61.81 | 117.66 | 0.9108 | 372.2 | 141.1 | |
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back to the solar disc SDO HMI 2011-11-17 08:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.62 | 138.57 | 26.44 | 154.88 | -23.75 | 286.08 | -59.73 | 118.17 | 0.8986 | 675.6 | 229.6 | |
| 0.00 | 1.63 | 0.00 | 1.94 | -23.41 | 284.15 | -61.66 | 117.29 | 0.9106 | 328.0 | 279.1 | |
| 0.00 | 1.03 | 0.00 | 1.22 | -23.21 | 284.10 | -61.71 | 117.07 | 0.9106 | 379.0 | 341.3 | |
| 0.00 | 0.26 | 0.00 | 0.32 | -23.78 | 283.07 | -62.74 | 117.41 | 0.9181 | 226.0 | 176.0 | |
| 1.37 | 8.08 | 1.70 | 10.04 | -23.49 | 283.03 | -62.78 | 117.09 | 0.9178 | 262.5 | 121.2 | |
| 1.55 | 4.64 | 1.98 | 5.96 | -22.91 | 281.93 | -63.88 | 116.23 | 0.9236 | 326.9 | -228.9 | |
| 0.00 | 1.20 | 0.00 | 1.64 | -24.31 | 280.63 | -65.18 | 117.40 | 0.9332 | -529.0 | -477.8 | |
| 0.00 | 1.46 | 0.00 | 2.03 | -24.33 | 280.14 | -65.67 | 117.31 | 0.9360 | -510.0 | -381.0 | |
| 0.00 | 0.77 | 0.00 | 1.00 | -22.73 | 281.65 | -64.16 | 115.97 | 0.9250 | 399.0 | 272.7 | |
| 0.00 | 0.86 | 0.00 | 1.25 | -24.34 | 279.15 | -66.66 | 117.11 | 0.9413 | -235.0 | -195.3 | |
| 2.06 | 13.40 | 3.36 | 21.74 | -23.97 | 276.50 | -69.31 | 116.19 | 0.9540 | -266.2 | -227.7 | |
| 1.98 | 8.59 | 3.20 | 14.08 | -23.67 | 276.57 | -69.24 | 115.90 | 0.9534 | -317.2 | 106.9 | |
| 0.00 | 0.86 | 0.00 | 1.37 | -23.33 | 276.87 | -68.94 | 115.61 | 0.9516 | -475.0 | -401.4 | |
| 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. | |