| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.67 | 483.52 | 40.50 | 269.60 | -20.91 | 17.32 | 4.66 | 189.56 | 0.4604 | 937.9 | 380.9 | |
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back to the solar disc SDO HMI 2014-10-14 01:00:31 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.22 | 0.00 | 0.67 | -18.05 | 20.96 | 8.31 | 198.69 | 0.4304 | 854.0 | 712.9 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -18.53 | 20.09 | 7.44 | 196.52 | 0.4334 | 593.0 | 482.6 | |
| 0.00 | 2.54 | 0.00 | 1.43 | -21.86 | 20.02 | 7.37 | 194.33 | 0.4830 | -797.0 | -665.7 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -18.15 | 19.47 | 6.82 | 195.46 | 0.4251 | 878.0 | 643.8 | |
| 22.56 | 465.70 | 12.59 | 259.59 | -20.95 | 17.82 | 5.16 | 190.53 | 0.4620 | 1310.9 | 412.4 | |
| 50.11 | -5.00 | 27.91 | -5.00 | -20.88 | 17.21 | 4.55 | 189.33 | 0.4593 | 1382.6 | 999999 | |
| 0.00 | 1.92 | 0.00 | 1.09 | -22.30 | 17.09 | 4.43 | 188.59 | 0.4806 | -165.0 | -104.3 | |
| 0.00 | 2.54 | 0.00 | 1.38 | -18.02 | 15.90 | 3.25 | 187.55 | 0.4117 | -849.0 | -774.4 | |
| 0.00 | 1.31 | 0.00 | 0.71 | -18.02 | 15.62 | 2.96 | 186.90 | 0.4111 | -864.0 | -698.5 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -18.67 | 15.12 | 2.47 | 185.59 | 0.4206 | -772.0 | -587.4 | |
| 0.00 | 0.87 | 0.00 | 0.49 | -20.89 | 14.07 | 1.41 | 182.91 | 0.4543 | 591.0 | 511.2 | |
| 0.00 | 0.87 | 0.00 | 0.49 | -21.12 | 12.75 | 0.10 | 180.20 | 0.4573 | -827.0 | -687.5 | |
| 0.00 | 0.87 | 0.00 | 0.51 | -25.45 | 9.83 | -2.82 | 175.13 | 0.5252 | -793.0 | -635.4 | |
| 0.00 | 1.31 | 0.00 | 0.79 | -27.82 | 7.30 | -5.36 | 171.55 | 0.5640 | -559.0 | -490.3 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -27.64 | 4.28 | -8.38 | 166.85 | 0.5696 | -626.0 | -582.6 | |
| 0.00 | 0.35 | 0.00 | 0.20 | -24.18 | 2.57 | -10.09 | 162.30 | 0.5277 | -640.0 | -456.2 | |
| 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. | |