SDO HMI 2014-04-11 15:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.17 | 0.00 | 10.79 | -13.48 | 307.12 | 3.38 | 197.74 | 0.2153 | 13.7 | 84.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.56 | 0.00 | 1.36 | -8.51 | 324.54 | 20.79 | 261.48 | 0.3565 | 796.0 | 461.8 | |
| 0.00 | 1.50 | 0.00 | 0.76 | -10.63 | 313.50 | 9.75 | 243.13 | 0.1875 | 898.0 | 789.8 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -19.97 | 313.00 | 9.25 | 211.69 | 0.2889 | -804.0 | -642.8 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -14.86 | 311.40 | 7.65 | 219.31 | 0.2040 | 878.0 | 704.1 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -12.53 | 311.01 | 7.27 | 226.59 | 0.1707 | 811.0 | 562.6 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -13.87 | 310.96 | 7.21 | 221.07 | 0.1863 | 788.0 | 672.8 | |
| 0.00 | 3.44 | 0.00 | 1.73 | -12.15 | 310.63 | 6.88 | 226.82 | 0.1614 | 660.0 | 782.1 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -12.06 | 310.38 | 6.63 | 226.19 | 0.1573 | 707.0 | 564.7 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -16.63 | 300.94 | -2.81 | 165.89 | 0.1935 | -81.0 | -104.6 | |
| 0.00 | 1.76 | 0.00 | 0.89 | -13.30 | 298.42 | -5.33 | 145.11 | 0.1587 | -985.0 | -784.7 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -13.23 | 298.14 | -5.61 | 143.51 | 0.1606 | -957.0 | -743.6 | |
| 0.00 | 1.50 | 0.00 | 0.77 | -17.13 | 295.56 | -8.18 | 145.25 | 0.2398 | -964.0 | -730.3 | |
| 0.00 | 1.50 | 0.00 | 0.76 | -14.46 | 294.70 | -9.05 | 134.67 | 0.2150 | -784.0 | -512.0 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -17.74 | 293.71 | -10.03 | 141.29 | 0.2666 | -771.0 | -590.6 | |
| 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. | |