SDO HMI 2014-08-15 08:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.24 | 44.25 | 9.13 | 26.47 | -17.53 | 105.26 | 24.22 | 224.35 | 0.5615 | 376.8 | 401.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.69 | 12.08 | 2.81 | 7.25 | -17.15 | 106.12 | 25.08 | 225.86 | 0.5665 | 945.0 | 796.5 | |
| 1.26 | 4.51 | 0.76 | 2.71 | -17.48 | 106.06 | 25.02 | 225.36 | 0.5691 | 873.2 | 605.9 | |
| 0.00 | 1.08 | 0.00 | 0.65 | -17.77 | 105.85 | 24.82 | 224.76 | 0.5698 | 739.0 | 631.1 | |
| 3.16 | 6.76 | 1.91 | 4.09 | -18.36 | 105.73 | 24.69 | 223.86 | 0.5744 | 804.1 | 472.9 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -17.65 | 105.59 | 24.55 | 224.60 | 0.5661 | 751.0 | 633.5 | |
| 0.45 | 1.53 | 0.27 | 0.92 | -17.54 | 105.33 | 24.29 | 224.45 | 0.5623 | 1063.2 | 843.1 | |
| 0.00 | 1.26 | 0.00 | 0.75 | -17.00 | 105.26 | 24.22 | 225.06 | 0.5563 | 798.0 | 691.3 | |
| 4.06 | 7.39 | 2.43 | 4.42 | -17.69 | 105.11 | 24.07 | 223.98 | 0.5616 | 947.2 | 738.6 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -16.44 | 103.97 | 22.93 | 224.26 | 0.5375 | -580.0 | -410.7 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -18.47 | 103.96 | 22.92 | 221.62 | 0.5583 | -531.0 | -325.8 | |
| 1.62 | 3.16 | 0.95 | 1.84 | -16.61 | 103.27 | 22.23 | 223.16 | 0.5321 | -836.4 | -603.9 | |
| 0.00 | 1.71 | 0.00 | 1.02 | -18.34 | 103.46 | 22.42 | 221.15 | 0.5522 | -834.0 | -653.7 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -17.00 | 102.43 | 21.39 | 221.55 | 0.5278 | -638.0 | -513.5 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -17.92 | 102.13 | 21.09 | 219.98 | 0.5349 | -585.0 | -510.2 | |
| 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. | |