SDO HMI 2014-10-02 04:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.03 | 100.68 | 17.73 | 59.77 | -10.14 | 140.37 | -28.97 | 119.95 | 0.5525 | 732.1 | 319.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.15 | 0.00 | 0.67 | -10.96 | 142.36 | -26.98 | 123.12 | 0.5339 | 699.0 | 506.3 | |
| 0.00 | 1.85 | 0.00 | 1.13 | -15.35 | 140.72 | -28.61 | 128.05 | 0.5886 | 666.0 | 483.7 | |
| 0.00 | 2.47 | 0.00 | 1.47 | -12.00 | 140.68 | -28.65 | 123.15 | 0.5623 | 708.0 | 577.6 | |
| 6.43 | 84.12 | 3.78 | 49.67 | -9.24 | 140.69 | -28.64 | 118.81 | 0.5420 | 1019.3 | 376.8 | |
| 4.84 | -4.00 | 2.87 | -4.00 | -10.02 | 140.58 | -28.75 | 119.98 | 0.5490 | 922.4 | 999999 | |
| 15.59 | -4.00 | 9.21 | -4.00 | -9.71 | 140.58 | -28.75 | 119.48 | 0.5468 | 1117.6 | 999999 | |
| 3.17 | -4.00 | 1.87 | -4.00 | -9.40 | 140.61 | -28.72 | 119.00 | 0.5442 | 1004.4 | 999999 | |
| 0.00 | 1.76 | 0.00 | 1.07 | -12.78 | 139.81 | -29.52 | 123.52 | 0.5786 | 809.0 | 565.5 | |
| 0.00 | 2.20 | 0.00 | 1.32 | -11.47 | 139.94 | -29.40 | 121.68 | 0.5674 | 853.0 | 751.3 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -10.97 | 139.36 | -29.97 | 120.42 | 0.5709 | 565.0 | 454.4 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -15.08 | 137.70 | -31.63 | 124.96 | 0.6201 | -560.0 | -476.0 | |
| 0.00 | 1.76 | 0.00 | 1.10 | -13.56 | 137.87 | -31.46 | 122.99 | 0.6071 | -680.0 | -528.2 | |
| 0.00 | 2.73 | 0.00 | 1.71 | -12.37 | 136.70 | -32.63 | 120.35 | 0.6126 | -743.0 | -621.9 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -12.54 | 136.53 | -32.80 | 120.46 | 0.6158 | -688.0 | -555.5 | |
| 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. | |