SDO HMI 2014-04-11 11:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.38 | 0.00 | 7.71 | -8.40 | 283.77 | -22.18 | 97.28 | 0.3809 | -7.6 | 72.7 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.32 | 0.00 | 0.69 | -8.46 | 288.41 | -17.53 | 99.47 | 0.3034 | 803.0 | 600.3 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -7.79 | 288.22 | -17.72 | 97.21 | 0.3054 | 854.0 | 702.3 | |
| 0.00 | 1.41 | 0.00 | 0.74 | -5.44 | 286.27 | -19.67 | 89.71 | 0.3366 | 895.0 | 706.1 | |
| 0.00 | 3.00 | 0.00 | 1.58 | -5.80 | 286.10 | -19.85 | 90.78 | 0.3393 | 723.0 | 601.2 | |
| 0.00 | 1.24 | 0.00 | 0.65 | -4.88 | 285.74 | -20.20 | 88.14 | 0.3457 | 743.0 | 584.3 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -14.60 | 283.23 | -22.71 | 113.08 | 0.4079 | -692.0 | -642.5 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -13.10 | 282.31 | -23.63 | 108.95 | 0.4145 | -643.0 | -549.2 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -10.04 | 280.68 | -25.26 | 101.05 | 0.4300 | -667.0 | -557.7 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -16.16 | 279.74 | -26.20 | 113.97 | 0.4660 | -765.0 | -611.9 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -6.45 | 280.09 | -25.85 | 92.67 | 0.4356 | -601.0 | -489.7 | |
| 0.00 | 1.94 | 0.00 | 1.08 | -8.42 | 278.40 | -27.55 | 96.96 | 0.4628 | -734.0 | -610.8 | |
| 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. | |