| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.64 | 39.74 | 5.00 | 26.01 | -21.21 | 310.59 | -29.76 | 134.84 | 0.6543 | -182.5 | -299.1 | |
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back to the solar disc SDO HMI 2014-09-19 05:00:34 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.67 | -21.03 | 314.77 | -25.59 | 138.82 | 0.6144 | 492.0 | 425.2 | |
| 0.00 | 2.04 | 0.00 | 1.28 | -19.94 | 313.72 | -26.64 | 136.41 | 0.6136 | 898.0 | 730.3 | |
| 0.00 | 1.24 | 0.00 | 0.77 | -18.93 | 313.15 | -27.21 | 134.60 | 0.6097 | 746.0 | 565.9 | |
| 0.00 | 1.60 | 0.00 | 1.01 | -19.79 | 312.77 | -27.58 | 135.26 | 0.6212 | 900.0 | 739.8 | |
| 0.00 | 0.80 | 0.00 | 0.50 | -19.22 | 312.81 | -27.55 | 134.60 | 0.6156 | 660.0 | 507.6 | |
| 1.60 | 2.84 | 1.01 | 1.80 | -20.21 | 312.58 | -27.77 | 135.56 | 0.6269 | 788.1 | 584.3 | |
| 0.00 | 0.35 | 0.00 | 0.23 | -20.27 | 312.24 | -28.11 | 135.29 | 0.6306 | 330.0 | 441.5 | |
| 0.00 | 0.98 | 0.00 | 0.64 | -21.73 | 311.12 | -29.23 | 135.90 | 0.6542 | -786.0 | -549.7 | |
| 0.00 | 3.28 | 0.00 | 2.17 | -21.76 | 310.18 | -30.18 | 135.04 | 0.6630 | -824.0 | -767.9 | |
| 0.00 | 0.71 | 0.00 | 0.47 | -21.29 | 310.06 | -30.29 | 134.40 | 0.6601 | -835.0 | -688.1 | |
| 0.80 | 5.41 | 0.52 | 3.55 | -21.02 | 310.05 | -30.30 | 134.07 | 0.6579 | -949.0 | -696.0 | |
| 0.00 | 5.41 | 0.00 | 3.61 | -22.10 | 309.68 | -30.67 | 134.98 | 0.6705 | -700.0 | -443.7 | |
| 0.00 | 0.80 | 0.00 | 0.53 | -21.23 | 309.89 | -30.47 | 134.17 | 0.6612 | -729.0 | -649.6 | |
| 3.82 | 6.39 | 2.53 | 4.23 | -21.62 | 309.72 | -30.63 | 134.47 | 0.6660 | -912.3 | -734.2 | |
| 1.42 | 4.70 | 0.94 | 3.13 | -21.61 | 309.31 | -31.05 | 134.09 | 0.6698 | -674.2 | -550.2 | |
| 0.00 | 2.13 | 0.00 | 1.42 | -21.89 | 309.24 | -31.11 | 134.34 | 0.6728 | -616.0 | -460.7 | |
| 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. | |