SDO HMI 2014-08-12 20:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.83 | 419.60 | 34.48 | 222.36 | 14.80 | 133.36 | 19.29 | 295.21 | 0.3542 | -906.0 | -331.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.63 | 16.01 | 135.05 | 20.97 | 296.58 | 0.3864 | -440.0 | -273.6 | |
| 64.83 | 387.26 | 34.48 | 205.91 | 15.06 | 133.97 | 19.90 | 295.28 | 0.3650 | -1510.0 | -430.3 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 17.34 | 129.74 | 15.66 | 306.67 | 0.3227 | -727.0 | -572.9 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 12.47 | 127.16 | 13.08 | 295.74 | 0.2464 | 837.0 | 651.6 | |
| 0.00 | 7.12 | 0.00 | 3.63 | 12.45 | 126.71 | 12.63 | 296.40 | 0.2395 | 652.0 | 652.1 | |
| 0.00 | 1.89 | 0.00 | 0.96 | 11.85 | 126.20 | 12.13 | 294.90 | 0.2277 | 960.0 | 815.2 | |
| 0.00 | 1.80 | 0.00 | 0.91 | 10.71 | 125.46 | 11.38 | 291.23 | 0.2090 | 976.0 | 818.8 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 10.63 | 125.11 | 11.03 | 291.41 | 0.2029 | 996.0 | 745.7 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 10.63 | 124.79 | 10.72 | 291.97 | 0.1980 | 991.0 | 832.8 | |
| 0.00 | 6.58 | 0.00 | 3.33 | 10.88 | 124.68 | 10.60 | 293.35 | 0.1977 | 900.0 | 824.2 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 11.13 | 124.44 | 10.36 | 294.99 | 0.1955 | 867.0 | 614.1 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 10.40 | 124.38 | 10.30 | 291.57 | 0.1900 | 893.0 | 733.9 | |
| 0.00 | 4.78 | 0.00 | 2.41 | 10.22 | 124.15 | 10.08 | 291.07 | 0.1854 | 1262.0 | 950.5 | |
| 0.00 | 1.80 | 0.00 | 0.91 | 11.33 | 123.41 | 9.33 | 298.26 | 0.1813 | 879.0 | 690.8 | |
| 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. | |