| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.19 | 48.27 | 20.25 | 69.97 | 18.87 | 315.30 | 69.47 | 289.50 | 0.9405 | -198.1 | -113.1 | |
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back to the solar disc SDO HMI 2011-11-24 22:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 5.05 | 0.00 | 8.07 | 17.68 | 317.41 | 71.57 | 288.05 | 0.9521 | -540.0 | -373.0 | |
| 0.94 | 14.30 | 1.61 | 23.72 | 18.86 | 318.64 | 72.81 | 289.20 | 0.9586 | 210.6 | -417.6 | |
| 5.91 | -2.00 | 9.82 | -2.00 | 18.78 | 318.13 | 72.30 | 289.15 | 0.9561 | -476.1 | 999999 | |
| 2.57 | 5.31 | 3.83 | 7.91 | 19.25 | 315.86 | 70.02 | 289.83 | 0.9446 | -495.2 | -393.4 | |
| 0.00 | 0.68 | 0.00 | 0.93 | 18.08 | 313.93 | 68.09 | 288.77 | 0.9331 | 143.0 | 132.2 | |
| 1.97 | 2.91 | 2.70 | 3.99 | 19.24 | 313.98 | 68.14 | 289.99 | 0.9340 | -386.9 | -484.0 | |
| 0.43 | 7.79 | 0.55 | 10.05 | 18.90 | 312.54 | 66.70 | 289.78 | 0.9251 | 253.6 | 98.6 | |
| 0.00 | 1.11 | 0.00 | 1.47 | 19.79 | 313.12 | 67.28 | 290.68 | 0.9293 | -423.0 | -316.8 | |
| 1.37 | 4.62 | 1.74 | 5.87 | 19.57 | 312.05 | 66.21 | 290.56 | 0.9225 | 491.4 | 439.3 | |
| 0.00 | 1.11 | 0.00 | 1.36 | 18.56 | 311.11 | 65.27 | 289.58 | 0.9157 | 206.0 | 156.5 | |
| 0.00 | 1.37 | 0.00 | 1.75 | 19.91 | 312.09 | 66.26 | 290.93 | 0.9231 | 326.0 | 302.0 | |
| 0.00 | 1.54 | 0.00 | 1.84 | 18.08 | 310.54 | 64.70 | 289.12 | 0.9115 | 195.0 | 272.1 | |
| 0.00 | 1.28 | 0.00 | 1.55 | 19.29 | 310.68 | 64.84 | 290.43 | 0.9134 | 520.0 | 437.6 | |
| 0.00 | 1.20 | 0.00 | 1.46 | 19.72 | 310.94 | 65.10 | 290.87 | 0.9155 | 259.0 | 287.8 | |
| 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. | |