SDO HMI 2014-10-02 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.85 | 65.46 | 9.97 | 36.81 | -10.29 | 140.31 | -22.44 | 126.90 | 0.4723 | 568.7 | 428.1 | |
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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 | 0.44 | -12.30 | 144.27 | -18.49 | 135.82 | 0.4464 | 714.0 | 544.1 | |
| 0.00 | 1.50 | 0.00 | 0.87 | -17.40 | 142.46 | -20.29 | 140.44 | 0.5216 | 657.0 | 593.5 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -11.76 | 141.11 | -21.65 | 130.44 | 0.4764 | 769.0 | 618.1 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -15.44 | 140.20 | -22.55 | 134.84 | 0.5233 | 614.0 | 440.4 | |
| 2.02 | 53.76 | 1.13 | 30.06 | -9.78 | 140.50 | -22.25 | 126.32 | 0.4650 | 1089.8 | 549.1 | |
| 6.42 | -5.00 | 3.58 | -5.00 | -9.19 | 140.51 | -22.24 | 125.28 | 0.4595 | 1052.1 | 999999 | |
| 4.22 | -5.00 | 2.36 | -5.00 | -9.97 | 140.39 | -22.36 | 126.52 | 0.4681 | 978.4 | 999999 | |
| 4.84 | -5.00 | 2.70 | -5.00 | -9.57 | 140.42 | -22.33 | 125.84 | 0.4641 | 1091.9 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.75 | -11.66 | 139.96 | -22.80 | 128.81 | 0.4889 | 826.0 | 692.2 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -11.79 | 139.78 | -22.97 | 128.81 | 0.4923 | 697.0 | 603.0 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -15.76 | 138.26 | -24.49 | 132.93 | 0.5471 | -714.0 | -560.4 | |
| 0.35 | 2.29 | 0.20 | 1.33 | -12.80 | 137.93 | -24.82 | 128.23 | 0.5232 | -913.5 | -786.4 | |
| 0.00 | 0.44 | 0.00 | 0.26 | -13.73 | 137.76 | -24.99 | 129.44 | 0.5336 | -606.0 | -453.4 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -12.41 | 136.78 | -25.97 | 126.38 | 0.5333 | -760.0 | -607.4 | |
| 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. | |