| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.01 | 121.21 | 35.88 | 156.13 | 7.65 | 129.65 | -67.33 | 82.22 | 0.9240 | -115.3 | -126.2 | |
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back to the solar disc SDO HMI 2011-11-28 15:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.28 | 0.00 | 1.56 | 9.09 | 131.17 | -65.82 | 80.59 | 0.9148 | 297.0 | 249.9 | |
| 11.37 | 73.34 | 13.70 | 88.22 | 7.57 | 131.30 | -65.68 | 82.25 | 0.9134 | -660.7 | -249.0 | |
| 0.00 | 2.91 | 0.00 | 3.67 | 7.28 | 130.12 | -66.87 | 82.62 | 0.9215 | -304.0 | -213.1 | |
| 0.00 | 1.37 | 0.00 | 1.72 | 6.57 | 130.24 | -66.74 | 83.39 | 0.9205 | -317.0 | -270.7 | |
| 1.97 | 3.42 | 2.45 | 4.26 | 5.53 | 130.42 | -66.56 | 84.51 | 0.9191 | -387.3 | -320.8 | |
| 0.00 | 1.11 | 0.00 | 1.41 | 6.89 | 129.92 | -67.06 | 83.05 | 0.9228 | -259.0 | -199.8 | |
| 1.79 | 3.16 | 2.38 | 4.18 | 7.70 | 128.95 | -68.03 | 82.19 | 0.9292 | -169.0 | -55.0 | |
| 1.97 | 4.36 | 2.59 | 5.76 | 6.96 | 129.03 | -67.95 | 82.99 | 0.9286 | -242.1 | -69.3 | |
| 0.00 | 1.79 | 0.00 | 2.41 | 7.34 | 128.67 | -68.32 | 82.59 | 0.9310 | -35.0 | 80.4 | |
| 0.00 | 1.20 | 0.00 | 1.63 | 8.08 | 128.41 | -68.57 | 81.81 | 0.9328 | -240.0 | -129.9 | |
| 2.65 | 4.53 | 3.71 | 6.35 | 8.67 | 127.76 | -69.22 | 81.20 | 0.9368 | 443.5 | 473.8 | |
| 5.21 | 12.14 | 7.85 | 18.26 | 8.28 | 126.24 | -70.74 | 81.66 | 0.9457 | 541.0 | 353.6 | |
| 2.05 | 10.60 | 3.20 | 16.70 | 7.87 | 125.47 | -71.51 | 82.11 | 0.9498 | 365.4 | 37.1 | |
| 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. | |