SDO HMI 2014-09-30 16:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.11 | 15.32 | 1.12 | 8.48 | -16.75 | 196.23 | 7.09 | 197.36 | 0.4245 | -216.6 | -127.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.59 | -21.16 | 210.70 | 21.56 | 216.66 | 0.5760 | 630.0 | 502.4 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -25.34 | 208.08 | 18.94 | 209.18 | 0.6039 | 504.0 | 462.7 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -14.61 | 201.24 | 12.09 | 209.29 | 0.4162 | -774.0 | -520.0 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -14.44 | 200.97 | 11.83 | 208.96 | 0.4119 | -549.0 | -471.2 | |
| 0.00 | 1.59 | 0.00 | 0.84 | -10.93 | 199.38 | 10.24 | 210.05 | 0.3500 | -6.0 | -0.9 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -20.06 | 198.32 | 9.17 | 198.43 | 0.4757 | -767.0 | -605.7 | |
| 0.00 | 1.85 | 0.00 | 0.98 | -12.05 | 197.09 | 7.95 | 202.84 | 0.3498 | -10.0 | -21.1 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -12.66 | 195.31 | 6.17 | 197.55 | 0.3491 | -2.0 | 8.2 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -1.44 | 194.24 | 5.10 | 212.05 | 0.1681 | -811.0 | -472.4 | |
| 2.11 | 2.20 | 1.12 | 1.16 | -13.42 | 192.11 | 2.97 | 188.31 | 0.3497 | -46.9 | -20.0 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -13.51 | 191.49 | 2.35 | 186.57 | 0.3498 | 23.0 | 3.9 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -13.73 | 190.41 | 1.27 | 183.52 | 0.3519 | 0.0 | 1.8 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -32.49 | 190.47 | 1.33 | 181.78 | 0.6351 | -648.0 | -548.2 | |
| 0.00 | 1.15 | 0.00 | 0.71 | -30.11 | 183.74 | -5.41 | 172.25 | 0.6070 | -596.0 | -494.9 | |
| 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. | |