| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.76 | 317.45 | 34.07 | 178.14 | -1.40 | 155.00 | 26.90 | 254.49 | 0.4712 | 954.6 | 388.5 | |
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back to the solar disc SDO HMI 2014-10-05 07:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.67 | 279.09 | 0.94 | 157.01 | -1.52 | 155.86 | 27.76 | 254.79 | 0.4845 | 744.4 | 395.8 | |
| 42.12 | -1.00 | 23.70 | -1.00 | -1.40 | 155.32 | 27.22 | 254.71 | 0.4760 | 1336.7 | 999999 | |
| 3.96 | -1.00 | 2.21 | -1.00 | -1.51 | 154.55 | 26.44 | 254.00 | 0.4650 | 1270.4 | 999999 | |
| 8.09 | 18.03 | 4.50 | 10.02 | -1.75 | 153.92 | 25.81 | 253.09 | 0.4568 | 1054.2 | 600.0 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 0.19 | 153.77 | 25.67 | 257.15 | 0.4461 | 771.0 | 634.3 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -1.16 | 153.64 | 25.54 | 254.15 | 0.4499 | 814.0 | 723.4 | |
| 4.92 | 7.30 | 2.72 | 4.03 | -0.21 | 153.37 | 25.27 | 256.04 | 0.4417 | 1034.1 | 805.5 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -0.22 | 152.87 | 24.77 | 255.72 | 0.4342 | 833.0 | 614.6 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 0.74 | 152.42 | 24.31 | 257.61 | 0.4233 | 806.0 | 635.1 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -3.67 | 152.23 | 24.13 | 247.76 | 0.4426 | 153.0 | 172.3 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 0.00 | 152.12 | 24.01 | 255.73 | 0.4217 | 721.0 | 663.5 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -1.73 | 150.23 | 22.13 | 250.30 | 0.4017 | -723.0 | -572.9 | |
| 0.00 | 2.02 | 0.00 | 1.09 | -2.23 | 149.98 | 21.88 | 248.89 | 0.4008 | -829.0 | -672.4 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -1.77 | 149.94 | 21.84 | 249.92 | 0.3976 | -737.0 | -548.0 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -2.10 | 148.98 | 20.88 | 248.24 | 0.3851 | -757.0 | -568.1 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -1.63 | 147.98 | 19.88 | 248.37 | 0.3672 | -772.0 | -646.4 | |
| 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. | |