SDO HMI 2014-08-29 10:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.93 | 42.23 | 14.94 | 35.73 | -17.33 | 206.06 | -48.88 | 117.47 | 0.8121 | 272.3 | 128.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.21 | 17.57 | 3.43 | 14.35 | -17.65 | 208.09 | -46.85 | 118.77 | 0.7954 | 663.8 | 408.4 | |
| 8.43 | -1.00 | 6.90 | -1.00 | -17.51 | 207.76 | -47.18 | 118.46 | 0.7978 | 579.5 | 999999 | |
| 0.00 | 2.87 | 0.00 | 2.28 | -14.90 | 208.12 | -46.82 | 115.58 | 0.7835 | 752.0 | 543.7 | |
| 0.00 | 2.06 | 0.00 | 1.72 | -17.22 | 206.72 | -48.21 | 117.63 | 0.8061 | 477.0 | 400.2 | |
| 0.99 | 1.97 | 0.85 | 1.70 | -18.80 | 205.79 | -49.14 | 118.98 | 0.8207 | 536.9 | 395.8 | |
| 0.00 | 2.42 | 0.00 | 2.02 | -16.72 | 206.47 | -48.47 | 116.94 | 0.8064 | 663.0 | 526.1 | |
| 1.34 | 2.69 | 1.13 | 2.25 | -16.55 | 206.19 | -48.75 | 116.61 | 0.8083 | 505.3 | 397.0 | |
| 0.00 | 0.99 | 0.00 | 0.83 | -15.94 | 205.43 | -49.51 | 115.58 | 0.8129 | 386.0 | 263.6 | |
| 2.96 | 5.29 | 2.63 | 4.70 | -18.51 | 204.31 | -50.62 | 118.00 | 0.8323 | -605.7 | -440.8 | |
| 0.00 | 0.63 | 0.00 | 0.53 | -16.02 | 205.20 | -49.73 | 115.58 | 0.8153 | 350.0 | 254.1 | |
| 0.00 | 1.17 | 0.00 | 1.09 | -19.60 | 202.43 | -52.50 | 118.40 | 0.8517 | -548.0 | -476.5 | |
| 0.00 | 1.79 | 0.00 | 1.66 | -17.67 | 202.18 | -52.75 | 116.18 | 0.8472 | -597.0 | -471.9 | |
| 0.00 | 0.90 | 0.00 | 0.78 | -11.72 | 202.65 | -52.29 | 109.60 | 0.8245 | -141.0 | -141.2 | |
| 0.00 | 1.88 | 0.00 | 1.82 | -17.62 | 200.43 | -54.51 | 115.44 | 0.8614 | -532.0 | -422.7 | |
| 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. | |