SDO HMI 2014-08-11 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.89 | 60.31 | 9.18 | 39.73 | -17.96 | 161.52 | 33.67 | 233.13 | 0.6621 | 670.9 | 442.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.53 | 38.96 | 8.94 | 25.72 | -16.97 | 162.49 | 34.64 | 235.15 | 0.6648 | 929.4 | 456.9 | |
| 0.36 | -1.00 | 0.24 | -1.00 | -16.88 | 162.01 | 34.16 | 234.91 | 0.6589 | 851.0 | 999999 | |
| 0.00 | 2.07 | 0.00 | 1.37 | -18.63 | 161.50 | 33.65 | 232.28 | 0.6661 | 783.0 | 649.4 | |
| 0.00 | 1.08 | 0.00 | 0.70 | -17.28 | 160.68 | 32.83 | 233.33 | 0.6476 | 718.0 | 535.6 | |
| 0.00 | 0.99 | 0.00 | 0.64 | -17.41 | 160.55 | 32.70 | 233.07 | 0.6472 | 473.0 | 504.2 | |
| 0.00 | 4.15 | 0.00 | 2.75 | -19.79 | 160.72 | 32.87 | 230.22 | 0.6668 | 644.0 | 567.6 | |
| 0.00 | 1.89 | 0.00 | 1.26 | -20.09 | 160.72 | 32.86 | 229.85 | 0.6691 | 633.0 | 500.0 | |
| 0.00 | 1.35 | 0.00 | 0.89 | -19.48 | 160.19 | 32.34 | 230.15 | 0.6592 | 817.0 | 646.5 | |
| 0.00 | 1.26 | 0.00 | 0.83 | -20.13 | 159.76 | 31.91 | 229.00 | 0.6600 | 396.0 | 368.2 | |
| 0.00 | 3.97 | 0.00 | 2.61 | -20.32 | 159.66 | 31.81 | 228.67 | 0.6605 | 726.0 | 596.7 | |
| 0.00 | 1.17 | 0.00 | 0.77 | -20.62 | 159.53 | 31.68 | 228.20 | 0.6617 | 355.0 | 423.8 | |
| 0.00 | 0.72 | 0.00 | 0.46 | -19.69 | 158.12 | 30.27 | 228.08 | 0.6401 | -148.0 | -266.6 | |
| 0.00 | 2.07 | 0.00 | 1.33 | -20.54 | 157.18 | 29.33 | 226.16 | 0.6382 | -502.0 | -511.8 | |
| 0.00 | 0.63 | 0.00 | 0.40 | -23.23 | 154.26 | 26.41 | 220.15 | 0.6361 | 622.0 | 528.7 | |
| 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. | |