| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.76 | 289.28 | 19.10 | 159.02 | 28.13 | 43.15 | 5.70 | 348.36 | 0.4349 | -940.0 | -438.6 | |
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back to the solar disc SDO HMI 2011-11-13 10:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 0.59 | 29.79 | 49.86 | 12.41 | 337.52 | 0.4898 | -634.0 | -478.3 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 28.93 | 49.03 | 11.58 | 338.12 | 0.4731 | -696.0 | -550.3 | |
| 0.00 | 1.38 | 0.00 | 0.80 | 33.12 | 47.50 | 10.05 | 343.75 | 0.5245 | -816.0 | -639.2 | |
| 0.00 | 1.81 | 0.00 | 1.04 | 32.39 | 45.03 | 7.58 | 347.19 | 0.5046 | -804.0 | -585.7 | |
| 0.00 | 1.38 | 0.00 | 0.76 | 27.86 | 44.35 | 6.90 | 345.79 | 0.4347 | -485.0 | -387.6 | |
| 1.98 | 274.81 | 1.09 | 150.99 | 28.02 | 43.99 | 6.54 | 346.60 | 0.4358 | -679.0 | -459.5 | |
| 7.40 | -6.00 | 4.07 | -6.00 | 28.22 | 43.36 | 5.91 | 347.96 | 0.4367 | -1157.8 | 999999 | |
| 19.01 | -6.00 | 10.43 | -6.00 | 27.93 | 43.21 | 5.76 | 348.10 | 0.4317 | -1382.9 | 999999 | |
| 1.72 | -6.00 | 0.95 | -6.00 | 28.22 | 42.92 | 5.47 | 348.83 | 0.4353 | -1003.6 | 999999 | |
| 4.22 | -6.00 | 2.32 | -6.00 | 28.45 | 42.90 | 5.45 | 348.99 | 0.4388 | -875.7 | 999999 | |
| 0.43 | -6.00 | 0.24 | -6.00 | 28.22 | 42.75 | 5.30 | 349.17 | 0.4348 | -954.2 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 26.83 | 41.88 | 4.43 | 350.29 | 0.4106 | -777.0 | -604.0 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 29.62 | 40.50 | 3.05 | 354.10 | 0.4513 | -701.0 | -561.7 | |
| 0.00 | 4.65 | 0.00 | 2.54 | 27.88 | 37.49 | 0.04 | 359.91 | 0.4214 | 788.0 | 538.5 | |
| 0.00 | 1.38 | 0.00 | 0.74 | 25.64 | 36.44 | -1.01 | 2.38 | 0.3858 | 816.0 | 632.6 | |
| 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. | |