SDO HMI 2014-08-13 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.05 | 383.20 | 36.42 | 217.31 | 15.07 | 133.58 | 28.30 | 289.38 | 0.4871 | -871.7 | -326.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.33 | 360.66 | 36.04 | 205.26 | 15.24 | 133.99 | 28.71 | 289.56 | 0.4938 | -1367.6 | -379.2 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 13.69 | 132.95 | 27.67 | 286.91 | 0.4735 | -612.0 | -475.3 | |
| 0.00 | 1.26 | 0.00 | 0.70 | 18.45 | 129.22 | 23.94 | 299.26 | 0.4431 | -800.0 | -693.1 | |
| 0.00 | 1.89 | 0.00 | 1.02 | 12.62 | 127.22 | 21.94 | 287.34 | 0.3836 | 656.0 | 593.5 | |
| 0.00 | 1.26 | 0.00 | 0.68 | 11.68 | 127.07 | 21.79 | 285.00 | 0.3780 | -713.0 | -609.4 | |
| 0.00 | 2.17 | 0.00 | 1.16 | 12.11 | 127.04 | 21.76 | 286.13 | 0.3790 | 691.0 | 611.8 | |
| 0.00 | 1.89 | 0.00 | 1.01 | 12.41 | 127.04 | 21.76 | 286.93 | 0.3800 | 894.0 | 726.3 | |
| 0.00 | 3.61 | 0.00 | 1.93 | 12.66 | 126.99 | 21.71 | 287.59 | 0.3802 | 801.0 | 653.5 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 11.90 | 126.06 | 20.78 | 286.17 | 0.3630 | 833.0 | 679.2 | |
| 0.00 | 2.80 | 0.00 | 1.48 | 11.63 | 126.00 | 20.72 | 285.46 | 0.3611 | 680.0 | 457.1 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 10.85 | 125.75 | 20.46 | 283.44 | 0.3546 | 847.0 | 675.4 | |
| 0.00 | 0.54 | 0.00 | 0.28 | 6.79 | 125.15 | 19.87 | 271.88 | 0.3391 | 715.0 | 638.0 | |
| 0.72 | 3.16 | 0.38 | 1.66 | 10.29 | 124.36 | 19.08 | 282.54 | 0.3309 | 1042.8 | 756.0 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 12.64 | 123.67 | 18.39 | 289.96 | 0.3290 | 778.0 | 605.0 | |
| 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. | |