SDO HMI 2014-04-09 11:05:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.34 | 289.62 | 35.22 | 202.44 | 12.79 | 13.27 | 40.97 | 294.95 | 0.7075 | -883.7 | -297.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.56 | 14.13 | 13.33 | 41.03 | 296.66 | 0.7146 | -307.0 | -241.8 | |
| 3.97 | 274.97 | 2.77 | 192.56 | 13.40 | 12.86 | 40.55 | 295.97 | 0.7058 | -807.3 | -310.4 | |
| 45.75 | -2.00 | 32.03 | -2.00 | 12.77 | 13.42 | 41.12 | 294.84 | 0.7091 | -1194.1 | 999999 | |
| 0.00 | 0.62 | 0.00 | 0.42 | 13.14 | 11.97 | 39.67 | 296.11 | 0.6946 | -522.0 | -512.7 | |
| 0.00 | 1.23 | 0.00 | 0.85 | 12.97 | 12.05 | 39.75 | 295.84 | 0.6947 | -326.0 | -331.0 | |
| 0.00 | 1.23 | 0.00 | 0.83 | 13.12 | 10.95 | 38.65 | 296.67 | 0.6830 | -824.0 | -694.4 | |
| 0.62 | 2.12 | 0.42 | 1.43 | 12.06 | 11.46 | 39.16 | 294.95 | 0.6834 | -629.9 | -519.9 | |
| 0.00 | 1.15 | 0.00 | 0.77 | 12.73 | 10.24 | 37.94 | 296.57 | 0.6728 | 115.0 | 136.4 | |
| 0.00 | 1.94 | 0.00 | 1.30 | 12.30 | 10.50 | 38.20 | 295.83 | 0.6735 | -507.0 | -306.5 | |
| 0.00 | 0.71 | 0.00 | 0.47 | 11.56 | 11.01 | 38.71 | 294.52 | 0.6757 | 391.0 | 358.5 | |
| 0.00 | 1.15 | 0.00 | 0.77 | 11.66 | 10.78 | 38.47 | 294.78 | 0.6735 | 473.0 | 387.4 | |
| 0.00 | 1.15 | 0.00 | 0.76 | 11.77 | 10.52 | 38.22 | 295.09 | 0.6710 | 500.0 | 453.9 | |
| 0.00 | 1.85 | 0.00 | 1.25 | 10.58 | 11.89 | 39.58 | 292.70 | 0.6813 | 249.0 | 252.4 | |
| 0.00 | 0.71 | 0.00 | 0.47 | 11.53 | 10.26 | 37.96 | 294.91 | 0.6668 | 407.0 | 390.6 | |
| 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. | |