SDO HMI 2014-10-04 18:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.25 | 245.05 | 28.97 | 133.04 | -13.25 | 121.47 | -13.79 | 145.47 | 0.4101 | 583.4 | 304.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.59 | 211.40 | 21.95 | 114.37 | -13.20 | 122.12 | -13.14 | 146.55 | 0.4032 | 1298.0 | 377.1 | |
| 1.41 | 4.04 | 0.77 | 2.20 | -13.58 | 121.05 | -14.21 | 145.00 | 0.4177 | 878.6 | 703.4 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -13.27 | 119.96 | -15.30 | 142.52 | 0.4239 | 879.0 | 588.9 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -13.28 | 119.57 | -15.69 | 141.84 | 0.4278 | 848.0 | 748.0 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -13.15 | 119.42 | -15.84 | 141.39 | 0.4277 | 825.0 | 658.8 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -11.61 | 118.11 | -17.14 | 136.72 | 0.4230 | 428.0 | 364.4 | |
| 2.90 | 4.83 | 1.61 | 2.68 | -13.38 | 117.37 | -17.88 | 138.31 | 0.4511 | -984.6 | -745.1 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -15.25 | 117.22 | -18.04 | 140.76 | 0.4743 | -627.0 | -524.1 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -13.10 | 117.17 | -18.09 | 137.56 | 0.4500 | -1007.0 | -956.8 | |
| 8.35 | 14.23 | 4.64 | 7.92 | -13.31 | 116.67 | -18.59 | 137.10 | 0.4577 | -1000.2 | -790.3 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -15.24 | 115.71 | -19.55 | 138.48 | 0.4891 | -839.0 | -732.9 | |
| 0.00 | 1.58 | 0.00 | 0.89 | -14.07 | 115.13 | -20.13 | 135.97 | 0.4823 | -672.0 | -591.0 | |
| 0.00 | 1.41 | 0.00 | 0.80 | -15.43 | 114.86 | -20.40 | 137.56 | 0.4998 | -626.0 | -358.5 | |
| 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. | |