| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.27 | 62.04 | 10.43 | 37.71 | 8.25 | 346.45 | -35.08 | 79.85 | 0.5797 | -39.8 | 79.8 | |
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back to the solar disc SDO HMI 2011-11-14 15:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.64 | 7.40 | 351.50 | -30.02 | 80.33 | 0.5053 | -956.0 | -794.2 | |
| 0.00 | 1.80 | 0.00 | 1.06 | 8.23 | 349.15 | -32.37 | 79.30 | 0.5414 | 470.0 | 423.5 | |
| 6.70 | 9.54 | 3.95 | 5.63 | 7.96 | 348.93 | -32.59 | 79.85 | 0.5441 | -884.0 | -722.0 | |
| 0.26 | -3.00 | 0.15 | -3.00 | 8.13 | 348.66 | -32.86 | 79.60 | 0.5482 | -776.7 | 999999 | |
| 0.00 | 1.80 | 0.00 | 1.07 | 7.80 | 348.69 | -32.83 | 80.19 | 0.5472 | -770.0 | -666.8 | |
| 0.00 | 1.89 | 0.00 | 1.12 | 7.98 | 348.46 | -33.06 | 79.93 | 0.5508 | -758.0 | -593.1 | |
| 0.00 | 0.60 | 0.00 | 0.36 | 8.42 | 348.35 | -33.17 | 79.15 | 0.5533 | 516.0 | 456.3 | |
| 0.00 | 1.20 | 0.00 | 0.72 | 7.27 | 347.63 | -33.89 | 81.36 | 0.5617 | -626.0 | -558.1 | |
| 0.00 | 5.07 | 0.00 | 3.09 | 8.17 | 346.01 | -35.51 | 80.07 | 0.5859 | 907.0 | 790.9 | |
| 0.00 | 3.44 | 0.00 | 2.10 | 8.50 | 345.90 | -35.62 | 79.54 | 0.5880 | 791.0 | 711.2 | |
| 2.15 | 32.66 | 1.32 | 20.10 | 8.19 | 345.68 | -35.84 | 80.10 | 0.5906 | 837.8 | 145.0 | |
| 7.82 | -11.00 | 4.80 | -11.00 | 8.34 | 345.48 | -36.05 | 79.90 | 0.5936 | 851.0 | 999999 | |
| 0.34 | -11.00 | 0.21 | -11.00 | 8.77 | 344.98 | -36.54 | 79.27 | 0.6012 | -449.8 | 999999 | |
| 0.00 | 2.92 | 0.00 | 1.82 | 8.70 | 344.61 | -36.91 | 79.46 | 0.6061 | -688.0 | -544.6 | |
| 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. | |