| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.27 | 157.66 | 32.02 | 97.74 | 19.95 | 64.10 | 25.91 | 316.95 | 0.6035 | 104.5 | 216.2 | |
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back to the solar disc SDO HMI 2011-02-13 19:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.45 | 42.28 | 14.93 | 26.90 | 19.47 | 67.41 | 29.22 | 312.91 | 0.6307 | -859.9 | -615.9 | |
| 0.00 | 1.46 | 0.00 | 0.92 | 20.14 | 66.57 | 28.38 | 314.54 | 0.6284 | -701.0 | -609.2 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 18.77 | 66.21 | 28.02 | 313.22 | 0.6126 | -515.0 | -451.7 | |
| 1.54 | 4.19 | 0.96 | 2.61 | 18.72 | 65.91 | 27.72 | 313.45 | 0.6092 | -662.2 | -674.0 | |
| 0.00 | 2.14 | 0.00 | 1.32 | 18.91 | 64.61 | 26.42 | 315.04 | 0.5980 | 774.0 | 554.6 | |
| 1.20 | 2.65 | 0.74 | 1.63 | 19.00 | 64.38 | 26.19 | 315.39 | 0.5965 | 805.9 | 710.1 | |
| 0.00 | 1.11 | 0.00 | 0.68 | 19.64 | 63.51 | 25.32 | 317.13 | 0.5944 | 455.0 | 418.1 | |
| 0.00 | 1.20 | 0.00 | 0.75 | 21.94 | 63.62 | 25.43 | 319.70 | 0.6180 | -901.0 | -754.9 | |
| 0.00 | 3.42 | 0.00 | 2.11 | 20.58 | 63.08 | 24.89 | 318.72 | 0.5996 | 494.0 | 386.0 | |
| 5.05 | 89.96 | 3.09 | 55.11 | 19.77 | 62.84 | 24.65 | 318.04 | 0.5893 | 1167.9 | 484.2 | |
| 14.81 | -10.00 | 9.07 | -10.00 | 20.12 | 62.66 | 24.47 | 318.67 | 0.5911 | 1067.2 | 999999 | |
| 1.97 | -10.00 | 1.20 | -10.00 | 20.13 | 62.24 | 24.05 | 319.16 | 0.5874 | 812.8 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.63 | 21.60 | 61.52 | 23.33 | 321.68 | 0.5962 | 710.0 | 551.7 | |
| 3.25 | 4.71 | 2.03 | 2.94 | 22.82 | 61.67 | 23.48 | 322.84 | 0.6103 | 660.7 | 495.2 | |
| 0.00 | 1.37 | 0.00 | 0.83 | 21.95 | 59.68 | 21.49 | 324.29 | 0.5844 | 715.0 | 499.2 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 21.45 | 57.67 | 19.48 | 326.36 | 0.5624 | 527.0 | 403.8 | |
| 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. | |