SDO HMI 2014-10-02 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.51 | 98.82 | 15.49 | 58.06 | -10.15 | 140.32 | -27.92 | 120.87 | 0.5393 | 714.0 | 330.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.48 | -15.99 | 141.05 | -27.18 | 130.33 | 0.5783 | 713.0 | 528.0 | |
| 0.00 | 1.67 | 0.00 | 0.98 | -11.89 | 141.20 | -27.04 | 124.51 | 0.5419 | 753.0 | 531.9 | |
| 0.00 | 2.38 | 0.00 | 1.41 | -11.91 | 140.68 | -27.56 | 124.04 | 0.5484 | 676.0 | 525.8 | |
| 0.00 | 0.44 | 0.00 | 0.26 | -13.81 | 140.31 | -27.93 | 126.51 | 0.5681 | 676.0 | 510.0 | |
| 3.70 | 83.33 | 2.15 | 48.68 | -9.12 | 140.75 | -27.49 | 119.62 | 0.5263 | 1064.6 | 428.8 | |
| 4.84 | -5.00 | 2.84 | -5.00 | -10.04 | 140.53 | -27.71 | 120.93 | 0.5358 | 925.7 | 999999 | |
| 12.95 | -5.00 | 7.57 | -5.00 | -9.69 | 140.56 | -27.68 | 120.39 | 0.5329 | 1126.3 | 999999 | |
| 5.02 | -5.00 | 2.93 | -5.00 | -9.31 | 140.59 | -27.64 | 119.80 | 0.5297 | 1027.2 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -16.17 | 139.54 | -28.70 | 129.07 | 0.5963 | 549.0 | 454.4 | |
| 0.00 | 1.76 | 0.00 | 1.05 | -11.48 | 139.93 | -28.31 | 122.66 | 0.5541 | 889.0 | 764.2 | |
| 0.00 | 3.52 | 0.00 | 2.16 | -13.56 | 137.93 | -30.30 | 123.96 | 0.5936 | -584.0 | -571.9 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -14.99 | 137.61 | -30.63 | 125.69 | 0.6082 | -557.0 | -518.2 | |
| 0.00 | 2.47 | 0.00 | 1.52 | -12.37 | 136.74 | -31.50 | 121.23 | 0.5991 | -740.0 | -637.7 | |
| 0.00 | 0.97 | 0.00 | 0.60 | -12.57 | 136.56 | -31.67 | 121.38 | 0.6025 | -629.0 | -585.6 | |
| 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. | |