SDO HMI 2014-09-05 00:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.84 | 199.46 | 53.30 | 238.01 | -19.44 | 107.18 | -60.78 | 115.26 | 0.9116 | 567.7 | 248.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.27 | 0.00 | 0.32 | -22.32 | 108.39 | -59.57 | 118.65 | 0.9107 | 399.0 | 401.3 | |
| 0.00 | 0.27 | 0.00 | 0.32 | -22.18 | 108.43 | -59.53 | 118.52 | 0.9101 | 354.0 | 441.3 | |
| 0.80 | 2.05 | 0.97 | 2.49 | -21.89 | 107.72 | -60.24 | 117.98 | 0.9139 | 374.7 | 290.0 | |
| 22.24 | 99.96 | 26.79 | 120.39 | -20.07 | 107.17 | -60.79 | 115.91 | 0.9132 | 599.0 | 186.6 | |
| 16.26 | 69.77 | 18.79 | 80.23 | -18.63 | 107.88 | -60.08 | 114.63 | 0.9053 | 797.4 | 471.4 | |
| 0.00 | 0.89 | 0.00 | 1.12 | -20.51 | 106.27 | -61.69 | 116.08 | 0.9198 | -307.0 | -237.5 | |
| 4.38 | 14.47 | 5.22 | 17.32 | -19.05 | 107.10 | -60.86 | 114.82 | 0.9114 | 504.9 | 50.7 | |
| 0.00 | 0.71 | 0.00 | 0.91 | -20.65 | 105.89 | -62.07 | 116.11 | 0.9224 | 224.0 | 199.1 | |
| 0.00 | 0.80 | 0.00 | 1.00 | -19.27 | 106.09 | -61.87 | 114.73 | 0.9183 | 217.0 | 166.6 | |
| 1.16 | 3.93 | 1.53 | 5.17 | -19.23 | 104.42 | -63.54 | 114.20 | 0.9283 | 264.7 | 4.6 | |
| 0.00 | 0.89 | 0.00 | 1.22 | -18.63 | 103.37 | -64.59 | 113.28 | 0.9333 | 287.0 | 260.1 | |
| 0.00 | 3.84 | 0.00 | 5.28 | -17.95 | 103.03 | -64.93 | 112.48 | 0.9341 | -424.0 | -330.0 | |
| 0.00 | 1.61 | 0.00 | 2.24 | -17.29 | 102.49 | -65.47 | 111.66 | 0.9361 | -384.0 | -280.1 | |
| 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. | |