SDO HMI 2014-08-04 23:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.81 | 0.00 | 12.83 | -18.79 | 239.68 | 21.49 | 219.90 | 0.5425 | 112.0 | 264.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.81 | -16.85 | 243.99 | 25.80 | 227.69 | 0.5653 | 757.0 | 553.0 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -17.56 | 242.83 | 24.63 | 225.44 | 0.5598 | 514.0 | 414.5 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -17.71 | 242.53 | 24.34 | 224.90 | 0.5583 | 708.0 | 653.9 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -17.40 | 242.35 | 24.15 | 225.10 | 0.5534 | 610.0 | 523.8 | |
| 0.00 | 0.63 | 0.00 | 0.38 | -17.95 | 242.15 | 23.95 | 224.13 | 0.5568 | 600.0 | 626.4 | |
| 0.00 | 4.52 | 0.00 | 2.68 | -19.17 | 240.26 | 22.07 | 220.28 | 0.5510 | 996.0 | 813.5 | |
| 0.00 | 3.89 | 0.00 | 2.31 | -19.83 | 239.80 | 21.60 | 218.89 | 0.5538 | 775.0 | 603.5 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -19.21 | 237.78 | 19.59 | 216.95 | 0.5287 | -136.0 | -163.8 | |
| 0.00 | 1.63 | 0.00 | 0.95 | -19.32 | 237.28 | 19.09 | 216.12 | 0.5257 | -463.0 | -324.9 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -20.06 | 237.10 | 18.91 | 215.00 | 0.5327 | -805.0 | -622.2 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -18.43 | 236.84 | 18.65 | 216.55 | 0.5114 | -767.0 | -603.6 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -17.99 | 236.56 | 18.36 | 216.68 | 0.5036 | -659.0 | -495.4 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -19.78 | 236.15 | 17.95 | 213.95 | 0.5215 | -674.0 | -559.5 | |
| 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. | |