SDO HMI 2011-10-22 22:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.38 | 0.00 | 11.90 | 17.64 | 322.13 | 1.20 | 354.05 | 0.2260 | 760.2 | 651.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.26 | 0.00 | 1.13 | 13.01 | 325.86 | 4.93 | 328.13 | 0.1593 | 796.0 | 682.7 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 14.27 | 325.86 | 4.92 | 332.01 | 0.1781 | 931.0 | 750.9 | |
| 0.00 | 5.91 | 0.00 | 3.01 | 17.80 | 324.91 | 3.98 | 343.07 | 0.2278 | 694.0 | 694.9 | |
| 0.00 | 1.74 | 0.00 | 0.89 | 18.94 | 324.30 | 3.37 | 346.75 | 0.2437 | 1090.0 | 922.2 | |
| 0.00 | 1.65 | 0.00 | 0.84 | 18.20 | 324.26 | 3.33 | 346.16 | 0.2314 | 959.0 | 726.6 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 18.84 | 324.05 | 3.12 | 347.63 | 0.2413 | 969.0 | 790.7 | |
| 0.00 | 0.61 | 0.00 | 0.31 | 18.91 | 322.98 | 2.05 | 351.84 | 0.2391 | 860.0 | 676.7 | |
| 0.00 | 1.91 | 0.00 | 0.99 | 21.35 | 320.83 | -0.10 | 0.34 | 0.2780 | 846.0 | 605.9 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 20.45 | 319.88 | -1.05 | 3.77 | 0.2634 | 876.0 | 693.5 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 21.12 | 317.02 | -3.91 | 13.10 | 0.2817 | 743.0 | 521.1 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 16.73 | 317.03 | -3.90 | 18.14 | 0.2100 | -803.0 | -522.1 | |
| 0.00 | 2.44 | 0.00 | 1.23 | 15.75 | 315.87 | -5.06 | 25.00 | 0.2018 | 956.0 | 755.8 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 16.08 | 315.49 | -5.44 | 25.89 | 0.2096 | 965.0 | 707.7 | |
| 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. | |