| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.35 | 69.31 | 11.98 | 62.55 | 9.98 | 147.83 | 54.54 | 286.53 | 0.8385 | -298.5 | -365.2 | |
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back to the solar disc SDO HMI 2014-03-31 07:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.53 | 0.00 | 0.53 | 10.22 | 151.60 | 58.32 | 285.71 | 0.8719 | -185.0 | -153.8 | |
| 0.00 | 2.98 | 0.00 | 2.89 | 10.43 | 150.29 | 57.00 | 286.30 | 0.8614 | -422.0 | -252.0 | |
| 0.53 | 2.63 | 0.50 | 2.51 | 10.41 | 149.78 | 56.49 | 286.43 | 0.8571 | -416.5 | -322.0 | |
| 0.00 | 5.53 | 0.00 | 5.20 | 9.87 | 149.36 | 56.07 | 285.94 | 0.8522 | -594.0 | -433.3 | |
| 0.00 | 0.97 | 0.00 | 0.91 | 10.41 | 149.50 | 56.22 | 286.51 | 0.8547 | -447.0 | -362.2 | |
| 3.60 | 40.27 | 3.32 | 36.68 | 9.68 | 148.71 | 55.42 | 285.91 | 0.8460 | -535.8 | -515.2 | |
| 1.32 | -6.00 | 1.21 | -6.00 | 9.79 | 148.47 | 55.18 | 286.09 | 0.8441 | -655.2 | 999999 | |
| 3.60 | -6.00 | 3.26 | -6.00 | 9.74 | 147.98 | 54.69 | 286.18 | 0.8396 | -947.5 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.85 | 10.42 | 146.63 | 53.35 | 287.38 | 0.8290 | -592.0 | -528.5 | |
| 2.37 | 3.77 | 2.05 | 3.27 | 10.38 | 145.91 | 52.62 | 287.57 | 0.8221 | 477.3 | 298.9 | |
| 1.93 | 5.35 | 1.64 | 4.54 | 9.86 | 145.29 | 52.00 | 287.16 | 0.8147 | 522.5 | 387.9 | |
| 0.00 | 2.37 | 0.00 | 2.03 | 10.64 | 145.37 | 52.09 | 288.06 | 0.8177 | -493.0 | -391.0 | |
| 0.00 | 0.70 | 0.00 | 0.60 | 10.91 | 145.24 | 51.95 | 288.42 | 0.8172 | -384.0 | -332.5 | |
| 0.00 | 1.05 | 0.00 | 0.88 | 9.80 | 144.63 | 51.35 | 287.30 | 0.8082 | -411.0 | -356.1 | |
| 0.00 | 0.61 | 0.00 | 0.47 | 13.30 | 139.22 | 45.94 | 293.64 | 0.7657 | 425.0 | 398.9 | |
| 0.00 | 1.58 | 0.00 | 1.19 | 11.99 | 138.70 | 45.41 | 292.27 | 0.7550 | 576.0 | 450.3 | |
| 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. | |