SDO HMI 2014-10-09 22:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.35 | 0.00 | 10.75 | 14.67 | 92.15 | 25.07 | 292.67 | 0.4465 | 72.0 | 160.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.58 | 9.02 | 102.48 | 35.40 | 276.79 | 0.5783 | -361.0 | -302.1 | |
| 0.00 | 0.44 | 0.00 | 0.26 | 10.81 | 100.81 | 33.73 | 280.13 | 0.5562 | -546.0 | -501.4 | |
| 0.00 | 0.70 | 0.00 | 0.42 | 11.43 | 100.49 | 33.41 | 281.31 | 0.5525 | -617.0 | -479.1 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 11.93 | 98.67 | 31.59 | 282.62 | 0.5272 | -767.0 | -657.0 | |
| 0.00 | 0.61 | 0.00 | 0.36 | 12.29 | 98.71 | 31.63 | 283.28 | 0.5287 | -629.0 | -535.3 | |
| 0.00 | 1.66 | 0.00 | 0.97 | 12.39 | 98.58 | 31.50 | 283.50 | 0.5270 | -765.0 | -664.2 | |
| 0.00 | 2.10 | 0.00 | 1.22 | 11.46 | 98.39 | 31.31 | 281.80 | 0.5224 | -722.0 | -571.8 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 17.62 | 92.63 | 25.55 | 296.76 | 0.4624 | 725.0 | 579.3 | |
| 0.00 | 2.28 | 0.00 | 1.22 | 15.81 | 87.87 | 20.79 | 296.85 | 0.3845 | 839.0 | 713.7 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 14.27 | 87.51 | 20.44 | 293.37 | 0.3702 | 691.0 | 527.6 | |
| 0.00 | 2.72 | 0.00 | 1.44 | 14.96 | 86.95 | 19.88 | 295.65 | 0.3660 | 994.0 | 819.9 | |
| 0.00 | 0.61 | 0.00 | 0.33 | 21.17 | 86.72 | 19.64 | 310.03 | 0.4111 | 663.0 | 622.9 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 22.53 | 85.03 | 17.96 | 315.05 | 0.4048 | 660.0 | 522.3 | |
| 0.00 | 2.63 | 0.00 | 1.39 | 17.07 | 84.20 | 17.12 | 304.34 | 0.3424 | 843.0 | 648.3 | |
| 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. | |