SDO HMI 2014-06-05 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.83 | 0.00 | 10.56 | 4.20 | 269.86 | -27.32 | 80.54 | 0.4639 | -690.9 | -574.6 | |
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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 | 1.72 | 0.00 | 0.93 | 3.91 | 273.10 | -24.08 | 80.18 | 0.4148 | -873.0 | -758.4 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 6.21 | 273.01 | -24.17 | 74.84 | 0.4234 | -893.0 | -762.4 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 3.70 | 272.98 | -24.21 | 80.73 | 0.4163 | -923.0 | -733.3 | |
| 0.00 | 2.26 | 0.00 | 1.23 | 3.40 | 272.82 | -24.37 | 81.51 | 0.4181 | -906.0 | -792.7 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 5.90 | 272.73 | -24.46 | 75.69 | 0.4267 | -679.0 | -614.5 | |
| 0.00 | 0.54 | 0.00 | 0.30 | 6.67 | 272.59 | -24.59 | 74.03 | 0.4317 | -681.0 | -513.8 | |
| 0.00 | 2.26 | 0.00 | 1.25 | 3.68 | 270.99 | -26.20 | 81.44 | 0.4473 | -812.0 | -652.6 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 3.83 | 270.61 | -26.57 | 81.22 | 0.4535 | -651.0 | -474.1 | |
| 0.00 | 4.25 | 0.00 | 2.37 | 3.19 | 270.32 | -26.86 | 82.70 | 0.4567 | -911.0 | -711.1 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 3.59 | 270.24 | -26.94 | 81.86 | 0.4587 | -616.0 | -469.5 | |
| 0.00 | 1.72 | 0.00 | 1.15 | 6.01 | 255.22 | -41.96 | 80.90 | 0.6757 | 345.0 | 270.3 | |
| 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. | |