| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.54 | 331.80 | 56.28 | 289.57 | -8.97 | 319.17 | -53.49 | 105.29 | 0.8232 | 569.9 | 268.4 | |
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back to the solar disc SDO HMI 2014-10-14 01:00:31 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.61 | 285.63 | 19.66 | 238.43 | -8.60 | 321.06 | -51.60 | 105.34 | 0.8057 | 1055.6 | 345.5 | |
| 32.97 | -1.00 | 27.64 | -1.00 | -9.11 | 320.86 | -51.80 | 105.89 | 0.8090 | 876.8 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.60 | -8.08 | 319.51 | -53.14 | 104.28 | 0.8196 | 416.0 | 301.1 | |
| 0.00 | 1.49 | 0.00 | 1.33 | -9.87 | 318.45 | -54.20 | 106.08 | 0.8338 | 486.0 | 382.4 | |
| 0.00 | 1.22 | 0.00 | 1.22 | -8.57 | 313.97 | -58.68 | 103.42 | 0.8705 | -601.0 | -572.5 | |
| 0.00 | 0.61 | 0.00 | 0.59 | -5.03 | 314.27 | -58.38 | 99.47 | 0.8620 | -434.0 | -388.1 | |
| 0.00 | 0.26 | 0.00 | 0.27 | -9.82 | 313.09 | -59.56 | 104.61 | 0.8799 | -458.0 | -444.3 | |
| 0.00 | 2.89 | 0.00 | 3.02 | -10.09 | 312.76 | -59.89 | 104.84 | 0.8830 | -591.0 | -448.1 | |
| 0.00 | 0.79 | 0.00 | 0.83 | -10.33 | 312.50 | -60.15 | 105.04 | 0.8855 | -328.0 | -292.8 | |
| 0.00 | 1.57 | 0.00 | 1.67 | -10.19 | 312.43 | -60.23 | 104.86 | 0.8858 | -406.0 | -383.1 | |
| 0.00 | 1.05 | 0.00 | 1.12 | -10.08 | 312.21 | -60.44 | 104.70 | 0.8873 | -299.0 | -255.2 | |
| 6.21 | 19.33 | 6.97 | 21.74 | -8.92 | 310.40 | -62.25 | 103.02 | 0.8992 | -582.3 | -150.2 | |
| 1.75 | 6.91 | 2.01 | 7.91 | -9.80 | 309.92 | -62.73 | 103.87 | 0.9040 | -319.1 | -226.4 | |
| 0.00 | 1.66 | 0.00 | 1.92 | -10.15 | 309.80 | -62.85 | 104.22 | 0.9054 | 134.0 | 132.8 | |
| 0.00 | 2.01 | 0.00 | 2.34 | -9.78 | 309.53 | -63.13 | 103.76 | 0.9068 | 387.0 | 326.4 | |
| 0.00 | 5.68 | 0.00 | 6.58 | -9.22 | 309.58 | -63.07 | 103.16 | 0.9056 | 318.0 | 305.5 | |
| 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. | |