SDO HMI 2014-03-11 14:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.51 | 0.00 | 10.44 | -10.73 | 15.08 | 21.93 | 258.75 | 0.3756 | 264.2 | 271.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.61 | 0.00 | 0.33 | -9.74 | 18.44 | 25.30 | 262.42 | 0.4267 | 697.0 | 511.0 | |
| 0.00 | 0.52 | 0.00 | 0.28 | -9.42 | 18.28 | 25.14 | 263.16 | 0.4239 | 130.0 | 209.8 | |
| 0.00 | 1.13 | 0.00 | 0.61 | -9.57 | 17.73 | 24.58 | 262.72 | 0.4153 | 731.0 | 630.2 | |
| 0.00 | 1.47 | 0.00 | 0.80 | -10.09 | 17.41 | 24.26 | 261.40 | 0.4109 | 784.0 | 621.8 | |
| 0.00 | 0.87 | 0.00 | 0.47 | -10.19 | 17.28 | 24.13 | 261.14 | 0.4090 | 819.0 | 643.2 | |
| 0.00 | 1.39 | 0.00 | 0.75 | -10.17 | 17.11 | 23.97 | 261.15 | 0.4064 | 881.0 | 632.1 | |
| 0.00 | 1.91 | 0.00 | 1.03 | -10.46 | 16.57 | 23.43 | 260.29 | 0.3984 | 710.0 | 619.3 | |
| 0.00 | 2.51 | 0.00 | 1.36 | -10.32 | 16.50 | 23.35 | 260.64 | 0.3969 | 827.0 | 762.8 | |
| 0.00 | 2.77 | 0.00 | 1.49 | -10.51 | 15.59 | 22.44 | 259.90 | 0.3829 | 586.0 | 561.1 | |
| 0.00 | 1.13 | 0.00 | 0.60 | -11.67 | 14.93 | 21.78 | 256.59 | 0.3752 | 688.0 | 537.0 | |
| 0.00 | 0.61 | 0.00 | 0.32 | -11.50 | 11.26 | 18.11 | 255.14 | 0.3166 | -764.0 | -610.0 | |
| 0.00 | 2.43 | 0.00 | 1.27 | -11.63 | 10.92 | 17.77 | 254.50 | 0.3116 | -981.0 | -813.5 | |
| 0.00 | 1.47 | 0.00 | 0.77 | -12.62 | 10.70 | 17.55 | 251.23 | 0.3122 | -727.0 | -618.1 | |
| 0.00 | 0.69 | 0.00 | 0.36 | -11.64 | 8.73 | 15.58 | 252.73 | 0.2767 | -682.0 | -529.9 | |
| 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. | |