SDO HMI 2014-09-09 15:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.11 | 65.68 | 13.75 | 42.54 | 9.67 | 147.42 | 40.52 | 276.42 | 0.6465 | -159.1 | -141.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.54 | 6.42 | 3.10 | 4.37 | 9.67 | 150.69 | 43.79 | 276.43 | 0.6888 | -647.6 | -372.5 | |
| 1.25 | 2.58 | 0.85 | 1.76 | 9.98 | 150.61 | 43.72 | 276.88 | 0.6879 | -645.6 | -499.1 | |
| 0.00 | 1.34 | 0.00 | 0.90 | 9.19 | 150.23 | 43.33 | 275.73 | 0.6832 | -649.0 | -623.4 | |
| 0.00 | 1.07 | 0.00 | 0.72 | 10.52 | 149.95 | 43.05 | 277.69 | 0.6795 | -435.0 | -345.6 | |
| 0.62 | 24.86 | 0.41 | 16.23 | 10.11 | 148.34 | 41.44 | 277.10 | 0.6589 | -593.7 | -700.4 | |
| 0.00 | 1.07 | 0.00 | 0.70 | 9.62 | 147.98 | 41.08 | 276.36 | 0.6541 | -704.0 | -598.9 | |
| 3.30 | -5.00 | 2.15 | -5.00 | 9.87 | 147.97 | 41.07 | 276.73 | 0.6541 | -923.9 | 999999 | |
| 1.96 | -5.00 | 1.28 | -5.00 | 10.12 | 147.89 | 40.99 | 277.12 | 0.6530 | -824.6 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.58 | 9.17 | 147.14 | 40.24 | 275.66 | 0.6432 | -784.0 | -675.4 | |
| 3.56 | 9.62 | 2.26 | 6.09 | 9.35 | 145.73 | 38.84 | 275.93 | 0.6244 | 785.9 | 561.8 | |
| 0.80 | 16.49 | 0.51 | 10.35 | 9.56 | 145.41 | 38.51 | 276.27 | 0.6200 | 748.9 | 700.9 | |
| 5.08 | -11.00 | 3.19 | -11.00 | 9.24 | 145.25 | 38.35 | 275.75 | 0.6178 | 947.4 | 999999 | |
| 0.00 | 1.34 | 0.00 | 0.84 | 9.85 | 145.13 | 38.24 | 276.75 | 0.6163 | 684.0 | 391.1 | |
| 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. | |