SDO HMI 2014-10-21 18:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.84 | 332.62 | 48.23 | 271.53 | -8.99 | 321.80 | 50.80 | 254.39 | 0.7969 | 673.7 | 254.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.79 | 318.88 | 44.10 | 261.39 | -8.91 | 322.02 | 51.02 | 254.56 | 0.7991 | 963.2 | 279.9 | |
| 2.96 | -1.00 | 2.43 | -1.00 | -9.64 | 321.98 | 50.98 | 253.65 | 0.8005 | 441.8 | 999999 | |
| 2.09 | -1.00 | 1.70 | -1.00 | -9.46 | 321.60 | 50.60 | 253.76 | 0.7962 | 928.9 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.76 | -8.95 | 320.51 | 49.51 | 254.05 | 0.7836 | 695.0 | 607.7 | |
| 0.00 | 0.78 | 0.00 | 0.61 | -9.56 | 319.60 | 48.60 | 253.00 | 0.7759 | 362.0 | 400.1 | |
| 0.00 | 0.52 | 0.00 | 0.42 | -12.83 | 320.30 | 49.30 | 249.22 | 0.7929 | 538.0 | 505.2 | |
| 0.00 | 1.04 | 0.00 | 0.81 | -9.05 | 319.42 | 48.42 | 253.57 | 0.7725 | -371.0 | -279.0 | |
| 0.00 | 1.31 | 0.00 | 1.01 | -10.29 | 319.11 | 48.11 | 251.91 | 0.7728 | -514.0 | -337.5 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -10.83 | 318.90 | 47.90 | 251.16 | 0.7723 | -452.0 | -507.0 | |
| 0.00 | 0.87 | 0.00 | 0.67 | -10.65 | 318.50 | 47.50 | 251.25 | 0.7675 | -536.0 | -523.5 | |
| 0.00 | 1.04 | 0.00 | 0.78 | -8.82 | 317.54 | 46.54 | 253.22 | 0.7515 | -353.0 | -395.0 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -14.27 | 318.65 | 47.65 | 246.83 | 0.7813 | 393.0 | 461.3 | |
| 0.00 | 1.04 | 0.00 | 0.74 | -9.53 | 314.35 | 43.35 | 251.10 | 0.7179 | -550.0 | -516.1 | |
| 0.00 | 0.96 | 0.00 | 0.68 | -9.42 | 314.08 | 43.08 | 251.14 | 0.7144 | -643.0 | -603.2 | |
| 0.00 | 1.39 | 0.00 | 0.97 | -9.72 | 313.51 | 42.51 | 250.49 | 0.7089 | -580.0 | -516.3 | |
| 0.00 | 2.61 | 0.00 | 1.80 | -7.49 | 313.16 | 42.16 | 253.40 | 0.6968 | -648.0 | -559.0 | |
| 0.00 | 0.70 | 0.00 | 0.48 | -9.91 | 313.13 | 42.13 | 250.07 | 0.7052 | -545.0 | -518.5 | |
| 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. | |