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 |
| 9.35 | 49.99 | 8.38 | 44.98 | 2.71 | 28.02 | 55.71 | 277.55 | 0.8321 | 187.7 | 120.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.71 | 0.00 | 0.74 | 1.90 | 33.53 | 61.23 | 275.44 | 0.8820 | -247.0 | -193.5 | |
| 1.50 | 4.14 | 1.55 | 4.30 | 1.69 | 33.39 | 61.08 | 275.23 | 0.8806 | -530.5 | -404.6 | |
| 0.00 | 0.97 | 0.00 | 1.00 | 1.48 | 33.15 | 60.85 | 275.03 | 0.8784 | -433.0 | -431.1 | |
| 0.00 | 1.59 | 0.00 | 1.65 | 1.32 | 33.46 | 61.15 | 274.79 | 0.8807 | -308.0 | -229.4 | |
| 0.44 | 3.70 | 0.44 | 3.68 | 1.81 | 31.84 | 59.53 | 275.61 | 0.8676 | -498.6 | -304.8 | |
| 0.00 | 1.59 | 0.00 | 1.42 | 3.45 | 28.04 | 55.74 | 278.19 | 0.8356 | -565.0 | -431.6 | |
| 0.00 | 0.88 | 0.00 | 0.86 | 1.89 | 31.34 | 59.03 | 275.78 | 0.8634 | -525.0 | -506.9 | |
| 0.00 | 0.97 | 0.00 | 0.99 | 0.98 | 32.87 | 60.57 | 274.51 | 0.8755 | -340.0 | -342.1 | |
| 0.00 | 1.23 | 0.00 | 1.21 | 1.18 | 31.55 | 59.25 | 274.93 | 0.8645 | -527.0 | -442.1 | |
| 0.00 | 0.26 | 0.00 | 0.27 | 0.40 | 33.25 | 60.95 | 273.79 | 0.8780 | -406.0 | -324.0 | |
| 0.00 | 1.06 | 0.00 | 0.94 | 2.54 | 27.78 | 55.47 | 277.17 | 0.8317 | 496.0 | 381.3 | |
| 0.00 | 1.15 | 0.00 | 1.02 | 2.27 | 28.14 | 55.84 | 276.78 | 0.8347 | 451.0 | 373.2 | |
| 6.79 | 26.27 | 5.98 | 23.22 | 2.56 | 27.48 | 55.17 | 277.25 | 0.8288 | 846.9 | 402.7 | |
| 0.00 | 0.88 | 0.00 | 0.63 | 8.54 | 16.51 | 44.21 | 287.84 | 0.7267 | 449.0 | 439.0 | |
| 0.62 | 2.03 | 0.41 | 1.35 | 8.26 | 12.07 | 39.76 | 289.38 | 0.6733 | 712.0 | 597.4 | |
| 0.00 | 0.97 | 0.00 | 0.65 | 7.97 | 12.25 | 39.95 | 288.88 | 0.6744 | 592.0 | 473.1 | |
| 0.00 | 0.88 | 0.00 | 0.59 | 7.77 | 12.15 | 39.84 | 288.64 | 0.6723 | 676.0 | 603.6 | |
| 0.00 | 0.71 | 0.00 | 0.46 | 7.49 | 11.28 | 38.98 | 288.65 | 0.6605 | 734.0 | 571.9 | |
| 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. | |