| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.60 | 342.13 | 38.49 | 186.69 | -1.35 | 154.86 | 23.47 | 252.18 | 0.4199 | 986.3 | 379.7 | |
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back to the solar disc SDO HMI 2014-10-05 01:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.34 | 292.28 | 1.83 | 159.93 | -1.81 | 155.28 | 23.89 | 251.50 | 0.4286 | 883.2 | 379.9 | |
| 46.77 | -1.00 | 25.58 | -1.00 | -1.38 | 155.24 | 23.85 | 252.42 | 0.4258 | 1277.1 | 999999 | |
| 0.62 | -1.00 | 0.34 | -1.00 | -1.77 | 155.02 | 23.63 | 251.39 | 0.4245 | 755.3 | 999999 | |
| 3.96 | -1.00 | 2.15 | -1.00 | -1.53 | 154.49 | 23.10 | 251.50 | 0.4153 | 1255.3 | 999999 | |
| 9.58 | 20.66 | 5.19 | 11.19 | -1.81 | 153.91 | 22.52 | 250.38 | 0.4081 | 1026.2 | 649.7 | |
| 0.00 | 2.11 | 0.00 | 1.14 | 0.13 | 153.80 | 22.41 | 254.89 | 0.3966 | 711.0 | 555.6 | |
| 0.00 | 1.41 | 0.00 | 0.76 | -1.13 | 153.71 | 22.32 | 251.79 | 0.4014 | 985.0 | 778.7 | |
| 6.33 | 10.46 | 3.40 | 5.62 | -0.24 | 153.28 | 21.89 | 253.60 | 0.3903 | 1006.4 | 755.1 | |
| 0.00 | 3.87 | 0.00 | 2.06 | 1.65 | 152.78 | 21.39 | 258.03 | 0.3742 | 857.0 | 650.7 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 0.40 | 152.61 | 21.21 | 254.66 | 0.3768 | 822.0 | 713.8 | |
| 0.00 | 2.73 | 0.00 | 1.45 | 0.94 | 152.48 | 21.09 | 255.98 | 0.3724 | 815.0 | 625.0 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -0.03 | 151.20 | 19.80 | 252.38 | 0.3570 | -759.0 | -569.1 | |
| 0.00 | 3.16 | 0.00 | 1.67 | -2.22 | 149.91 | 18.51 | 245.25 | 0.3509 | -804.0 | -734.3 | |
| 0.00 | 0.35 | 0.00 | 0.18 | -1.70 | 148.11 | 16.71 | 244.29 | 0.3205 | -791.0 | -674.2 | |
| 0.00 | 2.64 | 0.00 | 1.38 | -1.60 | 147.89 | 16.49 | 244.26 | 0.3165 | -755.0 | -623.0 | |
| 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. | |