SDO HMI 2014-09-12 23:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.69 | 18.32 | 1.39 | 14.13 | -19.77 | 105.59 | 42.72 | 236.43 | 0.7673 | 231.5 | 125.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.25 | 3.02 | 1.05 | 2.55 | -19.95 | 110.23 | 47.37 | 238.81 | 0.8106 | 467.0 | 345.6 | |
| 0.00 | 1.25 | 0.00 | 1.00 | -20.64 | 107.29 | 44.43 | 236.48 | 0.7880 | 547.0 | 469.4 | |
| 0.00 | 0.71 | 0.00 | 0.57 | -20.38 | 107.06 | 44.20 | 236.64 | 0.7846 | 295.0 | 447.8 | |
| 0.00 | 1.25 | 0.00 | 1.00 | -21.24 | 107.20 | 44.33 | 235.76 | 0.7902 | 563.0 | 451.6 | |
| 0.44 | 1.33 | 0.34 | 1.03 | -19.73 | 105.90 | 43.04 | 236.72 | 0.7707 | 690.4 | 646.6 | |
| 0.00 | 0.80 | 0.00 | 0.61 | -19.14 | 105.62 | 42.75 | 237.24 | 0.7649 | 479.0 | 455.1 | |
| 0.00 | 1.07 | 0.00 | 0.83 | -20.17 | 105.92 | 43.05 | 236.23 | 0.7732 | 532.0 | 379.4 | |
| 0.00 | 1.25 | 0.00 | 0.96 | -20.47 | 105.49 | 42.63 | 235.64 | 0.7709 | 635.0 | 489.4 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -20.90 | 105.42 | 42.56 | 235.11 | 0.7726 | 453.0 | 461.0 | |
| 0.00 | 0.62 | 0.00 | 0.48 | -20.35 | 104.88 | 42.02 | 235.41 | 0.7646 | 470.0 | 540.4 | |
| 0.00 | 2.67 | 0.00 | 1.94 | -18.85 | 102.72 | 39.85 | 235.80 | 0.7355 | -184.0 | -194.7 | |
| 0.00 | 2.22 | 0.00 | 1.61 | -18.93 | 102.16 | 39.29 | 235.34 | 0.7306 | -621.0 | -530.9 | |
| 0.00 | 1.33 | 0.00 | 0.96 | -18.84 | 101.80 | 38.94 | 235.22 | 0.7265 | -707.0 | -568.3 | |
| 0.00 | 0.53 | 0.00 | 0.38 | -19.14 | 101.85 | 38.98 | 234.89 | 0.7288 | -546.0 | -483.8 | |
| 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. | |