SDO HMI 2014-04-15 04:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.77 | 391.09 | 33.26 | 213.93 | 11.86 | 275.01 | 18.05 | 314.30 | 0.4257 | -1005.0 | -374.0 | |
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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 |
| 60.77 | 375.07 | 33.26 | 205.28 | 11.76 | 275.24 | 18.28 | 313.74 | 0.4268 | -1398.9 | -415.1 | |
| 0.00 | 0.80 | 0.00 | 0.44 | 13.54 | 273.30 | 16.34 | 319.86 | 0.4261 | -652.0 | -580.0 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 13.92 | 272.08 | 15.11 | 322.62 | 0.4186 | -769.0 | -581.5 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 15.18 | 271.04 | 14.07 | 326.32 | 0.4250 | -683.0 | -575.2 | |
| 0.00 | 1.95 | 0.00 | 1.05 | 13.02 | 270.30 | 13.33 | 324.68 | 0.3902 | 874.0 | 769.2 | |
| 0.00 | 1.95 | 0.00 | 1.04 | 13.08 | 269.86 | 12.89 | 325.66 | 0.3869 | 1042.0 | 901.2 | |
| 0.00 | 4.51 | 0.00 | 2.43 | 14.43 | 268.98 | 12.01 | 329.39 | 0.3976 | 794.0 | 664.0 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 14.75 | 268.93 | 11.97 | 329.90 | 0.4016 | 723.0 | 573.4 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 14.86 | 268.27 | 11.31 | 331.43 | 0.3980 | 564.0 | 464.3 | |
| 0.00 | 1.68 | 0.00 | 0.91 | 14.70 | 268.17 | 11.20 | 331.45 | 0.3949 | 845.0 | 766.4 | |
| 0.00 | 0.53 | 0.00 | 0.28 | 13.92 | 267.28 | 10.31 | 332.43 | 0.3771 | 312.0 | 395.0 | |
| 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. | |