SDO HMI 2014-08-13 05:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.00 | 34.45 | 11.82 | 31.06 | -18.54 | 160.65 | 51.53 | 242.67 | 0.8377 | 292.9 | 240.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.52 | 9.11 | 3.27 | 8.45 | -16.26 | 162.78 | 53.66 | 246.07 | 0.8480 | 505.6 | 451.0 | |
| 2.08 | -1.00 | 1.92 | -1.00 | -16.37 | 162.55 | 53.43 | 245.87 | 0.8465 | 662.0 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.91 | -16.96 | 161.89 | 52.77 | 244.96 | 0.8427 | 380.0 | 306.6 | |
| 0.00 | 0.72 | 0.00 | 0.68 | -18.47 | 162.47 | 53.35 | 243.51 | 0.8523 | 405.0 | 357.0 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -19.66 | 161.47 | 52.35 | 241.79 | 0.8481 | 281.0 | 305.7 | |
| 3.25 | 7.76 | 2.94 | 6.99 | -19.14 | 160.50 | 51.38 | 241.97 | 0.8383 | 590.8 | 641.8 | |
| 0.00 | 0.72 | 0.00 | 0.64 | -18.00 | 160.02 | 50.90 | 243.04 | 0.8302 | 456.0 | 445.9 | |
| 1.80 | 4.51 | 1.63 | 4.07 | -19.53 | 160.41 | 51.29 | 241.50 | 0.8390 | 542.1 | 470.6 | |
| 0.00 | 1.08 | 0.00 | 0.97 | -19.25 | 159.93 | 50.81 | 241.60 | 0.8339 | 679.0 | 641.9 | |
| 0.00 | 0.27 | 0.00 | 0.23 | -18.08 | 159.09 | 49.97 | 242.56 | 0.8224 | 594.0 | 483.7 | |
| 0.36 | 1.89 | 0.32 | 1.66 | -19.61 | 159.06 | 49.94 | 240.83 | 0.8279 | -384.8 | -298.8 | |
| 0.00 | 1.08 | 0.00 | 0.93 | -18.52 | 158.47 | 49.35 | 241.78 | 0.8186 | -296.0 | -343.0 | |
| 1.99 | 3.70 | 1.74 | 3.24 | -20.37 | 158.59 | 49.47 | 239.77 | 0.8268 | -504.4 | -365.8 | |
| 0.00 | 2.35 | 0.00 | 2.04 | -20.53 | 158.16 | 49.04 | 239.39 | 0.8238 | -560.0 | -464.9 | |
| 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. | |