| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.15 | 250.41 | 35.48 | 174.20 | 8.13 | 290.02 | -44.85 | 85.63 | 0.7030 | -538.3 | -226.0 | |
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back to the solar disc SDO HMI 2014-09-19 15:00:34 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.24 | 0.00 | 0.81 | 7.34 | 294.01 | -40.86 | 87.01 | 0.6520 | -620.0 | -528.1 | |
| 0.00 | 0.89 | 0.00 | 0.59 | 12.57 | 292.63 | -42.24 | 79.09 | 0.6705 | -497.0 | -388.9 | |
| 0.00 | 1.33 | 0.00 | 0.88 | 4.49 | 293.46 | -41.41 | 91.30 | 0.6619 | 701.0 | 572.7 | |
| 0.00 | 1.24 | 0.00 | 0.85 | 3.83 | 291.36 | -43.51 | 91.95 | 0.6896 | 538.0 | 355.8 | |
| 22.60 | 97.51 | 15.49 | 66.91 | 5.28 | 290.92 | -43.95 | 89.80 | 0.6934 | -805.3 | -233.8 | |
| 9.40 | 137.13 | 6.51 | 95.54 | 10.42 | 290.11 | -44.76 | 82.36 | 0.7011 | -1067.5 | -290.5 | |
| 3.90 | -6.00 | 2.71 | -6.00 | 10.58 | 289.95 | -44.92 | 82.12 | 0.7031 | -963.5 | 999999 | |
| 10.90 | -6.00 | 7.61 | -6.00 | 10.38 | 289.64 | -45.23 | 82.42 | 0.7068 | -760.3 | 999999 | |
| 2.93 | -6.00 | 2.05 | -6.00 | 10.60 | 289.38 | -45.49 | 82.11 | 0.7100 | -627.6 | 999999 | |
| 0.00 | 0.53 | 0.00 | 0.37 | 6.61 | 289.24 | -45.63 | 87.72 | 0.7129 | 480.0 | 487.7 | |
| 0.00 | 1.06 | 0.00 | 0.76 | 5.89 | 288.27 | -46.60 | 88.64 | 0.7252 | 558.0 | 473.8 | |
| 0.00 | 1.77 | 0.00 | 1.34 | 6.06 | 285.48 | -49.39 | 88.13 | 0.7576 | 607.0 | 499.0 | |
| 0.00 | 1.51 | 0.00 | 1.16 | 6.11 | 284.72 | -50.15 | 87.99 | 0.7661 | 636.0 | 475.8 | |
| 0.00 | 0.89 | 0.00 | 0.68 | 6.22 | 284.56 | -50.31 | 87.84 | 0.7678 | 517.0 | 429.3 | |
| 0.00 | 0.35 | 0.00 | 0.27 | 6.47 | 284.39 | -50.48 | 87.49 | 0.7695 | 517.0 | 481.2 | |
| 1.42 | 2.66 | 1.11 | 2.08 | 5.16 | 283.92 | -50.95 | 89.15 | 0.7758 | 506.4 | 385.7 | |
| 0.00 | 2.30 | 0.00 | 1.96 | 3.00 | 280.41 | -54.46 | 91.41 | 0.8150 | 87.0 | 117.3 | |
| 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. | |