SDO HMI 2014-11-04 13:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.29 | 189.93 | 64.29 | 461.63 | 15.04 | 10.96 | -78.18 | 75.45 | 0.9755 | 88.7 | 158.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 2.15 | 17.83 | 14.82 | -74.31 | 72.59 | 0.9617 | -321.0 | -263.3 | |
| 0.00 | 0.26 | 0.00 | 0.53 | 18.71 | 12.54 | -76.59 | 71.71 | 0.9715 | -75.0 | -112.3 | |
| 15.30 | 89.61 | 26.43 | 155.31 | 14.77 | 15.35 | -73.79 | 75.78 | 0.9591 | -351.0 | -118.3 | |
| 0.00 | 1.99 | 0.00 | 4.43 | 14.68 | 11.34 | -77.79 | 75.84 | 0.9761 | 465.0 | 429.0 | |
| 2.07 | 82.18 | 4.78 | 230.54 | 14.63 | 10.96 | -78.17 | 75.89 | 0.9775 | 276.2 | 316.7 | |
| 0.00 | 1.12 | 0.00 | 6.08 | 17.75 | 3.52 | -85.62 | 72.52 | 0.9960 | -226.0 | -182.0 | |
| 6.48 | -5.00 | 16.44 | -5.00 | 14.89 | 9.80 | -79.33 | 75.61 | 0.9814 | 611.0 | 999999 | |
| 0.00 | 0.86 | 0.00 | 4.37 | 17.40 | 3.77 | -85.36 | 72.89 | 0.9956 | 30.0 | 4.3 | |
| 0.00 | 1.12 | 0.00 | 4.15 | 16.58 | 6.01 | -83.12 | 73.79 | 0.9915 | 395.0 | 365.7 | |
| 1.21 | 6.74 | 6.00 | 32.56 | 17.16 | 3.92 | -85.22 | 73.14 | 0.9954 | 216.1 | 246.5 | |
| 4.23 | -5.00 | 10.64 | -5.00 | 14.30 | 9.78 | -79.36 | 76.20 | 0.9815 | 189.9 | 999999 | |
| 0.00 | 1.04 | 0.00 | 4.39 | 16.66 | 4.90 | -84.23 | 73.67 | 0.9938 | 360.0 | 353.8 | |
| 0.00 | 3.80 | 0.00 | 17.12 | 15.95 | 4.45 | -84.68 | 74.37 | 0.9946 | 381.0 | 320.2 | |
| 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. | |