SDO HMI 2014-10-05 00:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.50 | 348.25 | 36.62 | 189.26 | -1.36 | 154.83 | 22.89 | 251.68 | 0.4112 | 1007.2 | 386.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.26 | 301.39 | 0.14 | 164.17 | -0.93 | 155.27 | 23.33 | 253.05 | 0.4157 | 895.7 | 393.7 | |
| 44.65 | -1.00 | 24.31 | -1.00 | -1.38 | 155.21 | 23.27 | 251.97 | 0.4170 | 1304.1 | 999999 | |
| 6.15 | -1.00 | 3.33 | -1.00 | -1.56 | 154.46 | 22.52 | 250.96 | 0.4067 | 1184.9 | 999999 | |
| 5.10 | 23.82 | 2.75 | 12.86 | -1.90 | 153.95 | 22.00 | 249.71 | 0.4009 | 941.7 | 618.2 | |
| 4.66 | -4.00 | 2.51 | -4.00 | -1.71 | 153.82 | 21.87 | 250.03 | 0.3979 | 1086.6 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -1.16 | 153.71 | 21.77 | 251.25 | 0.3932 | 997.0 | 864.6 | |
| 0.00 | 1.32 | 0.00 | 0.71 | 0.20 | 153.65 | 21.70 | 254.54 | 0.3853 | 812.0 | 639.0 | |
| 6.68 | 10.20 | 3.58 | 5.46 | -0.26 | 153.26 | 21.31 | 253.07 | 0.3816 | 1011.9 | 770.2 | |
| 0.00 | 1.49 | 0.00 | 0.79 | 1.75 | 152.76 | 20.81 | 257.90 | 0.3648 | 773.0 | 588.7 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 0.97 | 152.52 | 20.58 | 255.68 | 0.3643 | 794.0 | 677.1 | |
| 0.00 | 2.20 | 0.00 | 1.16 | -2.22 | 149.93 | 17.98 | 244.57 | 0.3431 | -831.0 | -744.4 | |
| 0.00 | 2.64 | 0.00 | 1.39 | -1.70 | 149.83 | 17.88 | 245.82 | 0.3379 | -768.0 | -654.3 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -1.59 | 148.51 | 16.56 | 244.37 | 0.3174 | -655.0 | -505.8 | |
| 0.00 | 1.58 | 0.00 | 0.82 | -1.60 | 147.91 | 15.97 | 243.48 | 0.3087 | -782.0 | -645.7 | |
| 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. | |