SDO HMI 2014-10-10 18:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.37 | 0.00 | 13.66 | 13.45 | 94.61 | 38.51 | 284.44 | 0.6265 | 115.9 | -93.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.45 | 0.00 | 1.72 | 10.76 | 101.51 | 45.41 | 279.04 | 0.7108 | -588.0 | -547.6 | |
| 0.00 | 2.71 | 0.00 | 1.90 | 10.93 | 101.37 | 45.27 | 279.28 | 0.7092 | -804.0 | -665.0 | |
| 0.00 | 0.44 | 0.00 | 0.29 | 11.97 | 98.76 | 42.67 | 280.98 | 0.6777 | -679.0 | -578.8 | |
| 0.00 | 2.19 | 0.00 | 1.46 | 12.63 | 98.36 | 42.26 | 282.01 | 0.6732 | -661.0 | -530.5 | |
| 0.00 | 3.33 | 0.00 | 2.13 | 10.59 | 95.56 | 39.46 | 279.18 | 0.6351 | -816.0 | -634.8 | |
| 0.00 | 0.26 | 0.00 | 0.17 | 10.27 | 94.92 | 38.82 | 278.73 | 0.6263 | -637.0 | -577.3 | |
| 0.00 | 1.58 | 0.00 | 0.99 | 11.19 | 93.81 | 37.72 | 280.33 | 0.6122 | 860.0 | 715.7 | |
| 0.00 | 0.70 | 0.00 | 0.46 | 21.83 | 94.89 | 38.80 | 296.64 | 0.6530 | 608.0 | 518.4 | |
| 0.00 | 0.79 | 0.00 | 0.52 | 24.43 | 94.45 | 38.35 | 300.60 | 0.6587 | 549.0 | 366.4 | |
| 0.00 | 1.23 | 0.00 | 0.73 | 15.92 | 88.47 | 32.37 | 289.78 | 0.5493 | 584.0 | 534.8 | |
| 0.00 | 1.31 | 0.00 | 0.77 | 15.74 | 87.41 | 31.31 | 289.89 | 0.5341 | 542.0 | 448.9 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 15.45 | 87.11 | 31.01 | 289.49 | 0.5289 | 831.0 | 725.8 | |
| 0.00 | 0.96 | 0.00 | 0.56 | 15.09 | 86.90 | 30.81 | 288.92 | 0.5248 | 626.0 | 517.8 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 17.06 | 84.36 | 28.26 | 293.93 | 0.4973 | 631.0 | 504.4 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 16.73 | 84.23 | 28.14 | 293.37 | 0.4940 | 693.0 | 567.1 | |
| 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. | |