SDO HMI 2014-10-02 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.77 | 89.47 | 17.15 | 51.85 | -10.18 | 140.16 | -26.43 | 122.31 | 0.5207 | 555.9 | 288.7 | |
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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 | 0.46 | -11.91 | 141.10 | -25.50 | 126.12 | 0.5235 | 742.0 | 511.4 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -13.70 | 140.28 | -26.31 | 127.97 | 0.5485 | 601.0 | 482.0 | |
| 8.63 | 75.65 | 4.96 | 43.56 | -9.21 | 140.60 | -25.99 | 121.17 | 0.5077 | 976.5 | 432.6 | |
| 8.54 | -3.00 | 4.92 | -3.00 | -9.62 | 140.53 | -26.06 | 121.80 | 0.5117 | 1046.0 | 999999 | |
| 10.57 | -3.00 | 6.10 | -3.00 | -9.93 | 140.47 | -26.12 | 122.26 | 0.5149 | 908.1 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.85 | -16.02 | 139.58 | -27.01 | 130.54 | 0.5766 | 614.0 | 397.0 | |
| 2.03 | -3.00 | 1.17 | -3.00 | -9.70 | 140.22 | -26.37 | 121.62 | 0.5163 | 710.2 | 999999 | |
| 0.00 | 1.76 | 0.00 | 1.03 | -11.53 | 139.87 | -26.72 | 124.25 | 0.5351 | 877.0 | 723.7 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -13.54 | 138.07 | -28.52 | 125.52 | 0.5726 | -641.0 | -484.4 | |
| 0.00 | 1.41 | 0.00 | 0.86 | -15.07 | 137.64 | -28.95 | 127.30 | 0.5898 | -725.0 | -627.6 | |
| 0.00 | 2.11 | 0.00 | 1.27 | -12.70 | 137.72 | -28.87 | 123.96 | 0.5701 | -744.0 | -686.0 | |
| 0.00 | 1.41 | 0.00 | 0.85 | -12.06 | 137.17 | -29.43 | 122.52 | 0.5720 | -591.0 | -446.5 | |
| 0.00 | 1.41 | 0.00 | 0.85 | -12.31 | 136.78 | -29.81 | 122.54 | 0.5784 | -719.0 | -578.4 | |
| 0.00 | 1.32 | 0.00 | 0.80 | -12.51 | 136.58 | -30.01 | 122.66 | 0.5823 | -682.0 | -506.1 | |
| 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. | |