SDO HMI 2014-10-11 16:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.81 | 470.80 | 39.52 | 292.47 | -20.59 | 17.88 | -26.13 | 136.84 | 0.6046 | 961.3 | 313.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.66 | 0.00 | 1.02 | -21.43 | 20.46 | -23.55 | 140.69 | 0.5893 | -526.0 | -425.9 | |
| 0.00 | 0.61 | 0.00 | 0.37 | -20.32 | 20.61 | -23.40 | 139.56 | 0.5763 | 681.0 | 539.4 | |
| 1.58 | 4.29 | 0.94 | 2.56 | -18.29 | 20.13 | -23.88 | 136.47 | 0.5602 | 918.0 | 704.0 | |
| 0.00 | 1.14 | 0.00 | 0.68 | -18.66 | 19.97 | -24.04 | 136.75 | 0.5655 | 769.0 | 581.5 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -18.44 | 19.62 | -24.39 | 136.07 | 0.5668 | 782.0 | 628.2 | |
| 1.14 | 453.47 | 0.70 | 281.36 | -20.42 | 19.05 | -24.96 | 137.89 | 0.5919 | 1050.5 | 326.6 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -22.13 | 17.77 | -26.24 | 138.51 | 0.6205 | -45.0 | 51.6 | |
| 61.09 | -6.00 | 37.88 | -6.00 | -20.57 | 17.96 | -26.05 | 136.88 | 0.6037 | 1240.1 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -21.87 | 16.84 | -27.17 | 137.25 | 0.6265 | -260.0 | -222.2 | |
| 0.00 | 0.70 | 0.00 | 0.48 | -26.02 | 14.03 | -29.97 | 139.14 | 0.6887 | 450.0 | 388.8 | |
| 0.00 | 0.79 | 0.00 | 0.53 | -22.35 | 11.85 | -32.16 | 133.16 | 0.6771 | -477.0 | -418.0 | |
| 0.00 | 2.01 | 0.00 | 1.44 | -26.30 | 9.84 | -34.16 | 135.91 | 0.7258 | -644.0 | -539.8 | |
| 0.00 | 2.36 | 0.00 | 1.58 | -19.66 | 9.85 | -34.16 | 128.30 | 0.6761 | -632.0 | -359.2 | |
| 0.00 | 1.14 | 0.00 | 0.82 | -23.11 | 6.89 | -37.12 | 130.16 | 0.7286 | -107.0 | -141.3 | |
| 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. | |