| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.28 | 20.67 | 1.49 | 13.59 | 17.97 | 89.63 | -33.33 | 52.59 | 0.6601 | -335.4 | -337.6 | |
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back to the solar disc SDO HMI 2014-03-29 01:00:31 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.26 | 0.00 | 0.18 | 22.98 | 90.98 | -31.98 | 45.51 | 0.6859 | 243.0 | 342.3 | |
| 0.00 | 0.88 | 0.00 | 0.56 | 18.31 | 91.57 | -31.39 | 50.55 | 0.6426 | -697.0 | -590.6 | |
| 0.00 | 2.98 | 0.00 | 1.94 | 18.15 | 90.53 | -32.43 | 51.65 | 0.6521 | -567.0 | -473.5 | |
| 0.00 | 0.96 | 0.00 | 0.62 | 17.19 | 90.72 | -32.24 | 52.71 | 0.6428 | -663.0 | -569.9 | |
| 0.00 | 0.79 | 0.00 | 0.50 | 16.47 | 90.86 | -32.10 | 53.54 | 0.6359 | -629.0 | -531.7 | |
| 0.00 | 1.49 | 0.00 | 0.97 | 17.80 | 90.37 | -32.58 | 52.22 | 0.6511 | -804.0 | -649.5 | |
| 0.00 | 2.10 | 0.00 | 1.38 | 18.21 | 90.18 | -32.78 | 51.87 | 0.6562 | -560.0 | -510.4 | |
| 0.00 | 1.31 | 0.00 | 0.86 | 17.95 | 90.16 | -32.80 | 52.21 | 0.6544 | -630.0 | -559.9 | |
| 2.28 | 3.77 | 1.49 | 2.46 | 17.82 | 90.15 | -32.81 | 52.39 | 0.6536 | -850.7 | -711.9 | |
| 0.00 | 0.96 | 0.00 | 0.63 | 18.36 | 89.84 | -33.12 | 51.95 | 0.6608 | -561.0 | -423.4 | |
| 0.00 | 2.10 | 0.00 | 1.38 | 18.14 | 89.82 | -33.14 | 52.26 | 0.6594 | -520.0 | -428.0 | |
| 0.00 | 0.35 | 0.00 | 0.24 | 17.88 | 86.06 | -36.90 | 55.41 | 0.6964 | 677.0 | 494.8 | |
| 0.00 | 1.49 | 0.00 | 1.03 | 17.93 | 85.89 | -37.07 | 55.48 | 0.6984 | 487.0 | 473.0 | |
| 0.00 | 1.23 | 0.00 | 0.84 | 17.42 | 85.74 | -37.22 | 56.22 | 0.6968 | 632.0 | 572.7 | |
| 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. | |