SDO HMI 2014-10-11 19:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.79 | 32.85 | 0.51 | 21.01 | -22.64 | 68.94 | 26.59 | 221.01 | 0.6336 | -199.0 | -335.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.65 | -22.49 | 81.46 | 39.11 | 231.92 | 0.7428 | 396.0 | 282.3 | |
| 0.00 | 0.79 | 0.00 | 0.56 | -21.65 | 79.67 | 37.32 | 231.66 | 0.7207 | 621.0 | 542.3 | |
| 0.00 | 3.59 | 0.00 | 2.36 | -16.77 | 77.02 | 34.67 | 235.75 | 0.6612 | 693.0 | 498.6 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -18.80 | 74.13 | 31.78 | 230.82 | 0.6454 | 732.0 | 552.0 | |
| 0.00 | 1.84 | 0.00 | 1.09 | -14.94 | 68.81 | 26.46 | 231.00 | 0.5561 | 675.0 | 560.9 | |
| 0.00 | 1.40 | 0.00 | 0.90 | -23.86 | 68.45 | 26.10 | 219.40 | 0.6361 | -233.0 | -273.2 | |
| 0.79 | 3.68 | 0.51 | 2.37 | -24.55 | 68.45 | 26.10 | 218.66 | 0.6429 | -608.7 | -487.9 | |
| 0.00 | 6.74 | 0.00 | 4.28 | -23.36 | 68.05 | 25.70 | 219.53 | 0.6277 | -716.0 | -727.2 | |
| 0.00 | 2.54 | 0.00 | 1.62 | -23.69 | 67.98 | 25.62 | 219.08 | 0.6305 | -815.0 | -724.4 | |
| 0.00 | 5.78 | 0.00 | 3.69 | -23.97 | 68.00 | 25.65 | 218.81 | 0.6334 | -739.0 | -623.7 | |
| 0.00 | 0.96 | 0.00 | 0.61 | -24.08 | 67.37 | 25.02 | 218.02 | 0.6292 | -776.0 | -691.3 | |
| 0.00 | 1.75 | 0.00 | 1.07 | -26.25 | 58.34 | 15.99 | 204.92 | 0.5886 | -849.0 | -601.8 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -26.64 | 58.19 | 15.83 | 204.41 | 0.5925 | -677.0 | -578.1 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -26.85 | 58.18 | 15.83 | 204.23 | 0.5951 | -690.0 | -491.9 | |
| 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. | |