SDO HMI 2014-04-18 01:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.85 | 0.00 | 8.84 | -17.13 | 194.82 | -24.18 | 119.83 | 0.4451 | -568.0 | -521.0 | |
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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 | 1.06 | 0.00 | 0.54 | -13.07 | 207.77 | -11.23 | 125.51 | 0.2341 | 717.0 | 614.5 | |
| 0.00 | 2.21 | 0.00 | 1.17 | -18.07 | 202.75 | -16.25 | 129.98 | 0.3486 | -1001.0 | -806.2 | |
| 0.00 | 1.51 | 0.00 | 0.79 | -16.09 | 202.41 | -16.59 | 124.62 | 0.3348 | -823.0 | -653.6 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -17.05 | 201.63 | -17.37 | 125.85 | 0.3536 | -726.0 | -637.1 | |
| 0.00 | 1.86 | 0.00 | 0.98 | -15.43 | 200.63 | -18.37 | 120.49 | 0.3540 | -677.0 | -556.1 | |
| 0.00 | 2.13 | 0.00 | 1.19 | -15.66 | 192.69 | -26.31 | 113.74 | 0.4681 | -765.0 | -615.4 | |
| 0.00 | 1.24 | 0.00 | 0.73 | -18.84 | 189.04 | -29.96 | 117.34 | 0.5342 | -571.0 | -529.4 | |
| 0.00 | 0.89 | 0.00 | 0.51 | -15.59 | 189.01 | -29.99 | 111.45 | 0.5194 | -757.0 | -667.8 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -20.14 | 187.54 | -31.46 | 118.63 | 0.5605 | -680.0 | -499.7 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -19.95 | 187.58 | -31.42 | 118.35 | 0.5589 | -523.0 | -612.7 | |
| 0.00 | 1.59 | 0.00 | 0.97 | -18.80 | 184.99 | -34.01 | 115.01 | 0.5864 | -381.0 | -407.6 | |
| 0.00 | 1.06 | 0.00 | 0.65 | -18.51 | 184.83 | -34.17 | 114.46 | 0.5873 | -629.0 | -516.5 | |
| 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. | |