SDO HMI 2014-04-24 21:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.92 | 339.55 | 34.77 | 231.27 | 17.98 | 166.16 | 37.41 | 302.70 | 0.6889 | -681.0 | -311.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.68 | 321.71 | 25.73 | 219.59 | 17.82 | 166.37 | 37.62 | 302.34 | 0.6902 | -1089.2 | -357.7 | |
| 12.35 | -1.00 | 8.46 | -1.00 | 18.40 | 166.24 | 37.49 | 303.17 | 0.6922 | -927.1 | 999999 | |
| 0.00 | 1.33 | 0.00 | 0.89 | 17.94 | 164.81 | 36.06 | 303.53 | 0.6742 | -305.0 | -279.0 | |
| 0.89 | 4.35 | 0.58 | 2.85 | 17.95 | 163.14 | 34.39 | 304.75 | 0.6563 | 710.5 | 541.9 | |
| 0.00 | 0.36 | 0.00 | 0.23 | 18.31 | 163.19 | 34.44 | 305.19 | 0.6592 | 441.0 | 448.0 | |
| 0.00 | 3.11 | 0.00 | 2.03 | 18.14 | 162.95 | 34.20 | 305.13 | 0.6555 | 602.0 | 542.3 | |
| 0.00 | 1.33 | 0.00 | 0.87 | 17.87 | 162.86 | 34.11 | 304.85 | 0.6526 | 704.0 | 607.7 | |
| 0.00 | 1.24 | 0.00 | 0.81 | 18.22 | 162.74 | 33.99 | 305.40 | 0.6538 | 542.0 | 508.9 | |
| 0.00 | 1.24 | 0.00 | 0.82 | 18.55 | 162.82 | 34.07 | 305.78 | 0.6569 | 557.0 | 430.4 | |
| 0.00 | 1.42 | 0.00 | 0.93 | 18.02 | 162.62 | 33.87 | 305.23 | 0.6511 | 765.0 | 693.6 | |
| 0.00 | 1.24 | 0.00 | 0.81 | 18.93 | 162.48 | 33.73 | 306.53 | 0.6560 | 458.0 | 411.7 | |
| 0.00 | 1.24 | 0.00 | 0.81 | 19.36 | 161.82 | 33.07 | 307.60 | 0.6520 | 605.0 | 513.0 | |
| 0.00 | 0.98 | 0.00 | 0.63 | 20.98 | 160.22 | 31.47 | 310.98 | 0.6479 | 598.0 | 509.6 | |
| 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. | |