SDO HMI 2014-05-27 08:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.17 | 0.00 | 10.78 | -19.97 | 49.06 | -10.52 | 153.26 | 0.3690 | 338.7 | 259.2 | |
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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 | 1.17 | 0.00 | 0.61 | -19.82 | 56.01 | -3.57 | 169.59 | 0.3255 | 710.0 | 595.5 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -16.14 | 53.45 | -6.12 | 158.28 | 0.2781 | 876.0 | 649.0 | |
| 0.00 | 0.81 | 0.00 | 0.42 | -18.70 | 52.75 | -6.83 | 159.44 | 0.3219 | 730.0 | 592.3 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -19.05 | 52.51 | -7.07 | 159.19 | 0.3287 | 792.0 | 633.7 | |
| 0.00 | 3.25 | 0.00 | 1.70 | -18.73 | 52.26 | -7.31 | 158.15 | 0.3253 | 931.0 | 704.7 | |
| 0.00 | 1.71 | 0.00 | 0.90 | -19.23 | 51.26 | -8.31 | 156.18 | 0.3394 | 1009.0 | 754.2 | |
| 0.00 | 1.62 | 0.00 | 0.86 | -19.81 | 51.00 | -8.57 | 156.25 | 0.3496 | 829.0 | 716.9 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -20.03 | 50.63 | -8.94 | 155.63 | 0.3554 | 974.0 | 731.7 | |
| 0.00 | 1.62 | 0.00 | 0.86 | -20.13 | 50.43 | -9.14 | 155.27 | 0.3582 | 823.0 | 739.7 | |
| 0.00 | 1.89 | 0.00 | 1.05 | -21.70 | 42.60 | -16.97 | 142.26 | 0.4449 | -801.0 | -704.2 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -21.92 | 42.54 | -17.03 | 142.49 | 0.4482 | -841.0 | -718.8 | |
| 0.00 | 1.89 | 0.00 | 1.05 | -22.15 | 42.10 | -17.47 | 142.14 | 0.4550 | -766.0 | -694.0 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -22.41 | 41.79 | -17.78 | 142.05 | 0.4610 | -863.0 | -680.7 | |
| 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. | |