SDO HMI 2014-08-29 11:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.86 | 41.44 | 14.69 | 34.80 | -17.58 | 205.96 | -48.43 | 117.96 | 0.8090 | 208.1 | 71.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.68 | 16.59 | 2.96 | 13.40 | -17.69 | 208.09 | -46.30 | 119.09 | 0.7905 | 654.7 | 449.1 | |
| 8.34 | -1.00 | 6.75 | -1.00 | -17.52 | 207.77 | -46.62 | 118.74 | 0.7927 | 596.1 | 999999 | |
| 0.36 | 2.51 | 0.28 | 1.97 | -14.94 | 208.16 | -46.23 | 115.90 | 0.7779 | 661.0 | 574.5 | |
| 0.00 | 2.06 | 0.00 | 1.70 | -17.32 | 206.81 | -47.58 | 118.04 | 0.8007 | 460.0 | 372.0 | |
| 0.99 | 2.24 | 0.84 | 1.91 | -18.81 | 205.78 | -48.60 | 119.24 | 0.8160 | 462.5 | 395.1 | |
| 0.63 | 2.60 | 0.52 | 2.14 | -16.76 | 206.48 | -47.91 | 117.24 | 0.8014 | 613.0 | 462.7 | |
| 0.00 | 1.26 | 0.00 | 1.03 | -16.35 | 206.34 | -48.05 | 116.70 | 0.8011 | 500.0 | 424.6 | |
| 0.90 | 1.79 | 0.74 | 1.48 | -16.55 | 206.22 | -48.17 | 116.88 | 0.8030 | 438.9 | 379.9 | |
| 2.96 | 6.28 | 2.60 | 5.51 | -18.52 | 204.32 | -50.07 | 118.25 | 0.8276 | -631.6 | -416.2 | |
| 0.00 | 1.26 | 0.00 | 1.16 | -19.60 | 202.47 | -51.92 | 118.64 | 0.8470 | -408.0 | -467.1 | |
| 0.00 | 0.81 | 0.00 | 0.74 | -17.79 | 202.38 | -52.01 | 116.61 | 0.8414 | -606.0 | -601.2 | |
| 0.00 | 1.26 | 0.00 | 1.15 | -17.68 | 202.16 | -52.22 | 116.40 | 0.8428 | -526.0 | -445.4 | |
| 0.00 | 0.99 | 0.00 | 0.90 | -17.55 | 202.11 | -52.28 | 116.23 | 0.8429 | -340.0 | -281.5 | |
| 0.00 | 1.79 | 0.00 | 1.71 | -17.66 | 200.41 | -53.98 | 115.68 | 0.8572 | -556.0 | -443.9 | |
| 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. | |