| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.80 | 242.76 | 29.63 | 169.21 | -23.81 | 194.02 | -40.82 | 121.72 | 0.7049 | 638.2 | 287.3 | |
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back to the solar disc SDO HMI 2014-05-14 02:00:37 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.06 | 231.54 | 1.41 | 160.36 | -23.74 | 195.17 | -39.66 | 122.18 | 0.6926 | 1168.9 | 328.2 | |
| 2.06 | -1.00 | 1.42 | -1.00 | -23.93 | 194.97 | -39.86 | 122.33 | 0.6957 | 985.8 | 999999 | |
| 36.35 | -1.00 | 25.17 | -1.00 | -23.71 | 194.36 | -40.48 | 121.74 | 0.7012 | 979.9 | 999999 | |
| 2.33 | -1.00 | 1.63 | -1.00 | -23.40 | 193.73 | -41.10 | 121.02 | 0.7064 | 450.6 | 999999 | |
| 0.00 | 2.06 | 0.00 | 1.47 | -23.09 | 192.30 | -42.54 | 119.97 | 0.7202 | 523.0 | 375.1 | |
| 0.00 | 1.08 | 0.00 | 0.81 | -23.38 | 189.23 | -45.61 | 119.09 | 0.7529 | -510.0 | -376.3 | |
| 0.00 | 0.54 | 0.00 | 0.42 | -25.72 | 187.51 | -47.33 | 121.36 | 0.7780 | -444.0 | -360.8 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -25.85 | 187.34 | -47.50 | 121.45 | 0.7800 | -625.0 | -590.7 | |
| 0.00 | 2.15 | 0.00 | 1.72 | -26.39 | 186.69 | -48.15 | 121.87 | 0.7879 | -666.0 | -541.6 | |
| 0.00 | 0.90 | 0.00 | 0.72 | -25.99 | 186.46 | -48.38 | 121.29 | 0.7886 | -581.0 | -496.9 | |
| 0.00 | 1.35 | 0.00 | 1.14 | -27.87 | 184.60 | -50.23 | 122.88 | 0.8113 | -621.0 | -525.1 | |
| 0.00 | 0.90 | 0.00 | 0.73 | -25.86 | 185.76 | -49.08 | 120.90 | 0.7946 | -429.0 | -426.5 | |
| 0.00 | 1.97 | 0.00 | 1.63 | -26.34 | 185.12 | -49.72 | 121.25 | 0.8019 | -441.0 | -355.3 | |
| 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. | |