| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.53 | 287.63 | 31.23 | 215.56 | 16.14 | 63.63 | 47.63 | 289.05 | 0.7531 | -652.7 | -271.0 | |
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back to the solar disc SDO HMI 2011-11-15 01:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.66 | 14.01 | 64.92 | 48.91 | 285.99 | 0.7631 | -461.0 | -323.5 | |
| 41.53 | 268.54 | 31.23 | 201.80 | 16.03 | 63.81 | 47.81 | 288.86 | 0.7548 | -1003.0 | -302.5 | |
| 0.00 | 2.41 | 0.00 | 1.81 | 18.42 | 63.29 | 47.28 | 292.10 | 0.7547 | 603.0 | 497.2 | |
| 0.00 | 2.84 | 0.00 | 2.11 | 17.51 | 62.88 | 46.87 | 291.03 | 0.7480 | -265.0 | -204.5 | |
| 0.00 | 1.89 | 0.00 | 1.39 | 16.27 | 62.34 | 46.34 | 289.53 | 0.7392 | -777.0 | -674.9 | |
| 0.00 | 1.63 | 0.00 | 1.19 | 16.03 | 62.13 | 46.13 | 289.27 | 0.7363 | -333.0 | -295.8 | |
| 0.00 | 0.86 | 0.00 | 0.63 | 16.67 | 62.24 | 46.24 | 290.09 | 0.7390 | -518.0 | -404.4 | |
| 0.00 | 0.86 | 0.00 | 0.61 | 18.40 | 59.48 | 43.48 | 293.25 | 0.7129 | 566.0 | 480.5 | |
| 0.00 | 1.63 | 0.00 | 1.15 | 19.03 | 59.38 | 43.38 | 294.13 | 0.7138 | 527.0 | 437.1 | |
| 0.00 | 1.12 | 0.00 | 0.78 | 18.92 | 58.87 | 42.87 | 294.17 | 0.7077 | 500.0 | 439.9 | |
| 0.00 | 1.20 | 0.00 | 0.84 | 18.96 | 58.50 | 42.50 | 294.36 | 0.7037 | 741.0 | 557.8 | |
| 0.00 | 1.12 | 0.00 | 0.77 | 18.75 | 58.35 | 42.34 | 294.12 | 0.7012 | 639.0 | 537.3 | |
| 0.00 | 1.72 | 0.00 | 1.18 | 18.31 | 57.66 | 41.66 | 293.76 | 0.6919 | 528.0 | 467.0 | |
| 0.00 | 0.95 | 0.00 | 0.64 | 18.20 | 57.30 | 41.29 | 293.74 | 0.6872 | 705.0 | 568.8 | |
| 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. | |