| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.12 | 237.66 | 30.98 | 128.71 | -13.26 | 121.47 | -13.23 | 146.58 | 0.4053 | 590.2 | 280.9 | |
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back to the solar disc SDO HMI 2014-10-04 19:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.32 | 204.55 | 23.37 | 110.40 | -13.22 | 122.13 | -12.57 | 147.73 | 0.3985 | 1300.8 | 362.5 | |
| 1.85 | -1.00 | 1.00 | -1.00 | -13.52 | 121.67 | -13.03 | 147.20 | 0.4065 | 814.3 | 999999 | |
| 1.32 | 4.22 | 0.72 | 2.29 | -13.60 | 121.10 | -13.61 | 146.18 | 0.4125 | 831.4 | 625.9 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -13.23 | 119.63 | -15.08 | 142.87 | 0.4213 | 857.0 | 734.7 | |
| 0.00 | 1.49 | 0.00 | 0.82 | -13.48 | 119.58 | -15.13 | 143.15 | 0.4250 | 727.0 | 519.6 | |
| 0.00 | 1.67 | 0.00 | 0.91 | -13.17 | 119.47 | -15.23 | 142.50 | 0.4220 | 881.0 | 684.7 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -13.04 | 117.59 | -17.12 | 139.03 | 0.4392 | -749.0 | -681.1 | |
| 2.55 | 4.04 | 1.41 | 2.23 | -13.36 | 117.34 | -17.37 | 139.12 | 0.4456 | -1015.0 | -828.8 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -13.12 | 117.16 | -17.54 | 138.46 | 0.4445 | -1114.0 | -911.8 | |
| 8.08 | 13.71 | 4.48 | 7.60 | -13.29 | 116.63 | -18.07 | 137.88 | 0.4520 | -961.9 | -866.1 | |
| 0.00 | 1.67 | 0.00 | 0.93 | -13.73 | 116.11 | -18.60 | 137.72 | 0.4624 | -792.0 | -633.4 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -15.12 | 115.72 | -18.98 | 139.16 | 0.4821 | -822.0 | -686.9 | |
| 0.00 | 0.44 | 0.00 | 0.25 | -15.29 | 115.64 | -19.06 | 139.26 | 0.4848 | -659.0 | -728.8 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -14.02 | 115.14 | -19.57 | 136.70 | 0.4758 | -806.0 | -695.8 | |
| 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. | |