SDO HMI 2014-10-02 15:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.43 | 66.42 | 9.77 | 37.54 | -10.26 | 140.01 | -23.29 | 125.86 | 0.4821 | 497.6 | 347.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.58 | 0.00 | 0.89 | -11.79 | 141.12 | -22.18 | 129.79 | 0.4829 | 679.0 | 583.1 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -12.11 | 140.36 | -22.94 | 129.36 | 0.4949 | 831.0 | 672.6 | |
| 2.46 | 44.26 | 1.38 | 24.87 | -9.81 | 140.52 | -22.78 | 125.71 | 0.4719 | 1137.2 | 522.1 | |
| 3.26 | -3.00 | 1.83 | -3.00 | -10.03 | 140.44 | -22.86 | 126.00 | 0.4749 | 888.9 | 999999 | |
| 5.90 | 8.89 | 3.30 | 4.97 | -9.18 | 140.50 | -22.80 | 124.59 | 0.4666 | 1014.8 | 819.2 | |
| 4.31 | -3.00 | 2.42 | -3.00 | -9.53 | 140.44 | -22.86 | 125.13 | 0.4704 | 1053.3 | 999999 | |
| 1.50 | -3.00 | 0.84 | -3.00 | -9.85 | 140.29 | -23.02 | 125.50 | 0.4752 | 947.8 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -11.62 | 139.94 | -23.36 | 128.06 | 0.4953 | 898.0 | 717.5 | |
| 0.00 | 1.32 | 0.00 | 0.75 | -11.79 | 139.76 | -23.55 | 128.11 | 0.4990 | 720.0 | 595.3 | |
| 0.00 | 2.02 | 0.00 | 1.18 | -12.77 | 137.94 | -25.37 | 127.57 | 0.5292 | -875.0 | -778.9 | |
| 0.00 | 2.64 | 0.00 | 1.55 | -13.92 | 137.80 | -25.50 | 129.16 | 0.5410 | -798.0 | -660.5 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -12.60 | 136.86 | -26.44 | 126.17 | 0.5405 | -772.0 | -532.7 | |
| 0.00 | 2.11 | 0.00 | 1.24 | -12.48 | 136.74 | -26.57 | 125.86 | 0.5409 | -780.0 | -601.5 | |
| 0.00 | 0.70 | 0.00 | 0.42 | -11.40 | 133.90 | -29.40 | 121.53 | 0.5667 | -453.0 | -428.5 | |
| 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. | |