SDO HMI 2014-08-29 07:03:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.14 | 40.27 | 14.79 | 34.99 | -17.51 | 206.53 | -50.03 | 117.15 | 0.8231 | 293.7 | 188.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.13 | 19.10 | 3.47 | 16.16 | -17.62 | 207.99 | -48.57 | 117.92 | 0.8109 | 796.5 | 335.0 | |
| 7.80 | -1.00 | 6.61 | -1.00 | -17.49 | 207.65 | -48.91 | 117.62 | 0.8134 | 708.9 | 999999 | |
| 0.00 | 1.52 | 0.00 | 1.31 | -17.85 | 207.27 | -49.29 | 117.86 | 0.8183 | -244.0 | -211.2 | |
| 0.00 | 2.69 | 0.00 | 2.21 | -14.81 | 208.02 | -48.54 | 114.69 | 0.7997 | 408.0 | 462.4 | |
| 0.00 | 0.90 | 0.00 | 0.78 | -17.10 | 206.51 | -50.04 | 116.68 | 0.8221 | 437.0 | 343.3 | |
| 0.99 | 2.87 | 0.88 | 2.57 | -18.83 | 205.72 | -50.83 | 118.27 | 0.8353 | 661.0 | 374.3 | |
| 0.00 | 2.51 | 0.00 | 2.17 | -16.79 | 206.38 | -50.17 | 116.26 | 0.8221 | 667.0 | 539.9 | |
| 1.17 | 2.51 | 1.01 | 2.18 | -16.58 | 206.16 | -50.40 | 115.93 | 0.8233 | 545.0 | 331.2 | |
| 0.00 | 1.08 | 0.00 | 0.94 | -16.00 | 205.47 | -51.09 | 114.98 | 0.8273 | 165.0 | 214.4 | |
| 3.05 | 4.93 | 2.82 | 4.56 | -18.52 | 204.26 | -52.30 | 117.30 | 0.8464 | -714.0 | -484.1 | |
| 0.00 | 0.90 | 0.00 | 0.88 | -19.59 | 202.30 | -54.25 | 117.67 | 0.8654 | -431.0 | -351.0 | |
| 0.00 | 0.81 | 0.00 | 0.78 | -17.71 | 202.14 | -54.41 | 115.58 | 0.8609 | -488.0 | -439.0 | |
| 0.00 | 0.45 | 0.00 | 0.45 | -18.26 | 200.77 | -55.79 | 115.65 | 0.8732 | -389.0 | -317.8 | |
| 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. | |