SDO HMI 2014-10-16 23:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.35 | 331.98 | 36.94 | 253.15 | -21.15 | 16.52 | 42.34 | 235.73 | 0.7623 | 810.8 | 290.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.43 | 318.61 | 17.24 | 243.52 | -21.22 | 16.98 | 42.80 | 235.91 | 0.7671 | 890.3 | 302.2 | |
| 21.47 | -1.00 | 16.31 | -1.00 | -21.04 | 16.35 | 42.17 | 235.75 | 0.7603 | 1227.3 | 999999 | |
| 3.84 | -1.00 | 2.93 | -1.00 | -21.45 | 16.45 | 42.27 | 235.34 | 0.7634 | 883.0 | 999999 | |
| 0.26 | -1.00 | 0.20 | -1.00 | -21.43 | 16.18 | 42.00 | 235.20 | 0.7608 | 867.3 | 999999 | |
| 0.00 | 0.35 | 0.00 | 0.26 | -22.62 | 15.10 | 40.92 | 233.18 | 0.7576 | 321.0 | 484.0 | |
| 0.00 | 2.10 | 0.00 | 1.55 | -21.35 | 14.61 | 40.43 | 234.35 | 0.7457 | 669.0 | 591.1 | |
| 0.00 | 0.52 | 0.00 | 0.39 | -21.83 | 14.78 | 40.59 | 233.89 | 0.7500 | 599.0 | 612.3 | |
| 0.00 | 1.31 | 0.00 | 0.98 | -22.03 | 14.76 | 40.58 | 233.65 | 0.7510 | 551.0 | 402.5 | |
| 0.00 | 1.83 | 0.00 | 1.35 | -21.53 | 14.34 | 40.15 | 233.96 | 0.7441 | 283.0 | 415.1 | |
| 0.00 | 1.66 | 0.00 | 1.22 | -22.10 | 13.90 | 39.71 | 233.02 | 0.7434 | -446.0 | -305.1 | |
| 0.35 | 2.36 | 0.26 | 1.74 | -22.56 | 13.80 | 39.62 | 232.42 | 0.7453 | -506.0 | -386.3 | |
| 0.00 | 0.70 | 0.00 | 0.50 | -21.15 | 12.72 | 38.53 | 233.36 | 0.7265 | -320.0 | -274.1 | |
| 0.00 | 0.44 | 0.00 | 0.30 | -20.54 | 10.44 | 36.26 | 232.51 | 0.7003 | -467.0 | -461.4 | |
| 0.00 | 2.10 | 0.00 | 1.34 | -13.33 | 8.61 | 34.43 | 240.61 | 0.6337 | -680.0 | -599.4 | |
| 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. | |