SDO HMI 2014-05-20 20:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.53 | 82.49 | 22.04 | 66.90 | -17.82 | 196.40 | 50.83 | 248.93 | 0.7927 | 76.3 | 49.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.63 | 0.00 | 0.54 | -19.31 | 198.79 | 53.22 | 247.68 | 0.8193 | -246.0 | -241.6 | |
| 0.00 | 1.08 | 0.00 | 0.89 | -16.67 | 197.62 | 52.05 | 250.62 | 0.8030 | -127.0 | -101.0 | |
| 0.00 | 1.62 | 0.00 | 1.38 | -19.44 | 198.43 | 52.86 | 247.43 | 0.8162 | -178.0 | -146.8 | |
| 0.00 | 1.08 | 0.00 | 0.91 | -18.47 | 197.98 | 52.42 | 248.51 | 0.8101 | -281.0 | -272.5 | |
| 0.00 | 1.98 | 0.00 | 1.66 | -18.63 | 197.90 | 52.33 | 248.29 | 0.8095 | -331.0 | -302.1 | |
| 14.12 | 51.54 | 11.73 | 42.82 | -18.45 | 197.45 | 51.89 | 248.40 | 0.8049 | 737.4 | 253.1 | |
| 3.15 | -6.00 | 2.59 | -6.00 | -17.98 | 197.15 | 51.59 | 248.91 | 0.8010 | 734.7 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.75 | -19.57 | 197.11 | 51.55 | 246.95 | 0.8041 | -514.0 | -398.1 | |
| 0.00 | 1.80 | 0.00 | 1.46 | -18.76 | 196.40 | 50.83 | 247.76 | 0.7953 | 571.0 | 393.1 | |
| 0.00 | 0.45 | 0.00 | 0.34 | -16.04 | 194.11 | 48.54 | 250.61 | 0.7658 | -67.0 | -175.6 | |
| 0.00 | 1.17 | 0.00 | 0.89 | -16.07 | 193.93 | 48.36 | 250.52 | 0.7640 | -450.0 | -351.2 | |
| 0.00 | 1.62 | 0.00 | 1.23 | -16.17 | 193.72 | 48.16 | 250.34 | 0.7620 | -335.0 | -284.1 | |
| 2.34 | 18.62 | 1.77 | 14.03 | -16.24 | 193.37 | 47.80 | 250.16 | 0.7584 | -740.8 | -536.7 | |
| 7.92 | -13.00 | 5.95 | -13.00 | -15.91 | 193.02 | 47.46 | 250.51 | 0.7539 | -813.6 | 999999 | |
| 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. | |