SDO HMI 2014-10-21 09:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.34 | 367.56 | 49.90 | 271.27 | -8.95 | 321.69 | 45.75 | 252.76 | 0.7429 | 740.6 | 253.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.96 | 347.36 | 2.22 | 257.48 | -8.86 | 322.52 | 46.58 | 253.18 | 0.7520 | 453.4 | 285.6 | |
| 0.26 | -1.00 | 0.19 | -1.00 | -8.21 | 322.02 | 46.08 | 253.85 | 0.7446 | 1011.3 | 999999 | |
| 63.77 | -1.00 | 47.23 | -1.00 | -8.94 | 321.92 | 45.98 | 252.87 | 0.7456 | 1018.9 | 999999 | |
| 0.00 | 2.09 | 0.00 | 1.50 | -8.61 | 320.32 | 44.38 | 252.71 | 0.7266 | 564.0 | 474.8 | |
| 0.00 | 1.13 | 0.00 | 0.81 | -9.12 | 320.10 | 44.16 | 251.95 | 0.7258 | 700.0 | 627.1 | |
| 0.00 | 0.52 | 0.00 | 0.37 | -8.91 | 319.81 | 43.87 | 252.11 | 0.7218 | 654.0 | 611.3 | |
| 0.00 | 0.70 | 0.00 | 0.50 | -8.73 | 319.74 | 43.80 | 252.34 | 0.7204 | 759.0 | 699.5 | |
| 0.35 | 1.48 | 0.26 | 1.09 | -12.57 | 320.36 | 44.42 | 247.57 | 0.7414 | 452.0 | 368.6 | |
| 0.00 | 0.78 | 0.00 | 0.55 | -8.40 | 319.07 | 43.13 | 252.51 | 0.7115 | -502.0 | -372.0 | |
| 0.00 | 0.78 | 0.00 | 0.56 | -10.72 | 318.77 | 42.83 | 249.27 | 0.7165 | -484.0 | -392.4 | |
| 0.00 | 2.70 | 0.00 | 1.90 | -10.67 | 318.47 | 42.53 | 249.21 | 0.7129 | -800.0 | -608.9 | |
| 0.00 | 1.13 | 0.00 | 0.78 | -8.91 | 317.42 | 41.48 | 251.14 | 0.6938 | -610.0 | -504.4 | |
| 0.00 | 0.78 | 0.00 | 0.52 | -9.45 | 315.26 | 39.32 | 249.40 | 0.6701 | -547.0 | -497.1 | |
| 0.00 | 2.18 | 0.00 | 1.43 | -9.51 | 314.18 | 38.24 | 248.78 | 0.6571 | -835.0 | -697.7 | |
| 0.00 | 0.96 | 0.00 | 0.62 | -8.91 | 314.03 | 38.09 | 249.56 | 0.6526 | -621.0 | -471.4 | |
| 0.00 | 3.92 | 0.00 | 2.49 | -7.34 | 312.75 | 36.81 | 251.27 | 0.6298 | -556.0 | -653.8 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -11.66 | 311.29 | 35.34 | 244.03 | 0.6325 | -560.0 | -339.9 | |
| 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. | |