SDO HMI 2014-10-04 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.58 | 22.31 | 2.36 | 11.71 | -12.21 | 139.31 | 1.85 | 185.70 | 0.3256 | 144.2 | 173.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.41 | 0.00 | 0.76 | -16.51 | 140.68 | 3.22 | 187.84 | 0.3967 | 781.0 | 610.4 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -15.92 | 140.61 | 3.15 | 187.87 | 0.3872 | 750.0 | 532.8 | |
| 2.29 | 8.00 | 1.18 | 4.14 | -10.03 | 140.42 | 2.96 | 190.11 | 0.2909 | 1064.5 | 909.8 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -12.36 | 140.38 | 2.92 | 188.73 | 0.3291 | 792.0 | 680.6 | |
| 1.76 | -3.00 | 0.91 | -3.00 | -10.19 | 140.24 | 2.78 | 189.41 | 0.2929 | 894.7 | 999999 | |
| 0.53 | 1.58 | 0.27 | 0.82 | -9.94 | 140.18 | 2.72 | 189.35 | 0.2886 | 1018.8 | 963.2 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -11.92 | 139.98 | 2.52 | 187.73 | 0.3208 | 769.0 | 596.9 | |
| 0.00 | 1.49 | 0.00 | 0.78 | -11.63 | 139.95 | 2.48 | 187.75 | 0.3160 | 778.0 | 613.0 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -15.53 | 139.21 | 1.74 | 184.46 | 0.3784 | -761.0 | -544.8 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -15.49 | 138.40 | 0.93 | 182.39 | 0.3770 | -861.0 | -700.2 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -14.91 | 137.99 | 0.53 | 181.39 | 0.3673 | -864.0 | -769.1 | |
| 0.00 | 1.67 | 0.00 | 0.89 | -14.65 | 137.87 | 0.40 | 181.08 | 0.3631 | -996.0 | -809.7 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -10.31 | 134.85 | -2.62 | 171.19 | 0.2944 | -818.0 | -668.0 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -10.66 | 133.81 | -3.66 | 168.02 | 0.3033 | -864.0 | -659.8 | |
| 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. | |