SDO HMI 2014-10-11 08:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.38 | 0.00 | 11.91 | 14.98 | 56.75 | 8.36 | 321.01 | 0.2134 | 242.0 | 55.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.50 | 16.49 | 63.66 | 15.27 | 305.99 | 0.3134 | -780.0 | -706.9 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 18.37 | 60.84 | 12.44 | 316.34 | 0.2975 | -751.0 | -681.2 | |
| 0.00 | 3.50 | 0.00 | 1.82 | 18.46 | 60.58 | 12.19 | 317.14 | 0.2957 | -522.0 | -534.8 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 12.83 | 60.02 | 11.63 | 301.13 | 0.2306 | 805.0 | 689.4 | |
| 0.00 | 1.49 | 0.00 | 0.77 | 17.77 | 60.28 | 11.88 | 316.11 | 0.2841 | -951.0 | -735.5 | |
| 0.00 | 3.42 | 0.00 | 1.76 | 16.71 | 59.79 | 11.40 | 314.43 | 0.2662 | -863.0 | -701.5 | |
| 0.00 | 1.66 | 0.00 | 0.84 | 13.67 | 54.82 | 6.43 | 320.47 | 0.1717 | 907.0 | 701.7 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 13.74 | 54.61 | 6.21 | 321.65 | 0.1702 | 800.0 | 747.0 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 13.28 | 54.59 | 6.20 | 319.95 | 0.1641 | 888.0 | 739.4 | |
| 0.00 | 2.28 | 0.00 | 1.14 | 10.38 | 53.33 | 4.94 | 311.31 | 0.1132 | 832.0 | 550.0 | |
| 0.00 | 1.58 | 0.00 | 0.79 | 13.57 | 52.84 | 4.44 | 329.86 | 0.1507 | 839.0 | 656.3 | |
| 0.00 | 1.84 | 0.00 | 0.91 | 10.80 | 49.13 | 0.73 | 351.19 | 0.0826 | 949.0 | 659.8 | |
| 0.00 | 1.31 | 0.00 | 0.66 | 14.80 | 48.81 | 0.41 | 357.37 | 0.1516 | 993.0 | 762.5 | |
| 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. | |