| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.99 | 138.81 | 29.88 | 175.54 | 14.85 | 249.79 | -64.94 | 72.22 | 0.9208 | -556.8 | -105.2 | |
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back to the solar disc SDO HMI 2014-05-08 01:00:37 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.37 | 135.50 | 14.17 | 169.35 | 15.13 | 250.14 | -64.58 | 71.86 | 0.9192 | -506.8 | -110.3 | |
| 12.62 | -1.00 | 15.71 | -1.00 | 14.66 | 250.04 | -64.69 | 72.38 | 0.9193 | -659.8 | 999999 | |
| 0.00 | 0.89 | 0.00 | 1.47 | 13.55 | 243.78 | -70.94 | 74.61 | 0.9544 | -373.0 | -375.0 | |
| 0.00 | 2.42 | 0.00 | 4.72 | 14.07 | 240.86 | -73.87 | 74.47 | 0.9682 | 171.0 | 131.0 | |
| 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. | |