| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.50 | 22.10 | 0.96 | 13.79 | 6.74 | 208.04 | -37.74 | 87.95 | 0.6101 | -112.2 | -109.2 | |
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back to the solar disc SDO HMI 2014-09-26 09:00:33 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.33 | 0.00 | 0.80 | 6.71 | 210.49 | -35.28 | 88.16 | 0.5761 | -747.0 | -562.7 | |
| 0.00 | 3.27 | 0.00 | 1.98 | 6.72 | 210.23 | -35.54 | 88.12 | 0.5798 | -724.0 | -596.0 | |
| 0.00 | 1.59 | 0.00 | 0.97 | 5.91 | 209.81 | -35.96 | 89.48 | 0.5864 | -642.0 | -516.8 | |
| 0.00 | 1.33 | 0.00 | 0.81 | 6.95 | 209.58 | -36.20 | 87.68 | 0.5889 | -355.0 | -443.2 | |
| 0.35 | 1.33 | 0.22 | 0.81 | 6.35 | 209.59 | -36.18 | 88.71 | 0.5891 | -673.8 | -584.4 | |
| 0.00 | 1.94 | 0.00 | 1.19 | 5.66 | 209.60 | -36.17 | 89.89 | 0.5895 | -589.0 | -483.2 | |
| 0.00 | 1.59 | 0.00 | 0.98 | 6.41 | 208.83 | -36.94 | 88.53 | 0.5997 | -559.0 | -392.7 | |
| 0.00 | 1.06 | 0.00 | 0.66 | 6.89 | 207.91 | -37.86 | 87.67 | 0.6121 | -632.0 | -510.1 | |
| 0.00 | 0.44 | 0.00 | 0.28 | 5.69 | 206.73 | -39.04 | 89.51 | 0.6290 | 535.0 | 486.4 | |
| 0.00 | 1.06 | 0.00 | 0.68 | 6.42 | 206.44 | -39.34 | 88.32 | 0.6324 | 468.0 | 467.8 | |
| 0.00 | 1.50 | 0.00 | 0.97 | 7.61 | 205.84 | -39.93 | 86.40 | 0.6397 | 739.0 | 643.3 | |
| 0.00 | 1.24 | 0.00 | 0.80 | 7.82 | 205.74 | -40.03 | 86.07 | 0.6410 | 624.0 | 516.4 | |
| 1.15 | 3.71 | 0.74 | 2.40 | 7.04 | 205.51 | -40.27 | 87.27 | 0.6445 | 737.9 | 621.6 | |
| 0.00 | 0.71 | 0.00 | 0.46 | 8.12 | 204.58 | -41.19 | 85.56 | 0.6562 | 591.0 | 485.0 | |
| 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. | |