SDO HMI 2014-05-25 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.47 | 0.00 | 10.22 | -18.67 | 50.66 | -33.19 | 119.97 | 0.6010 | 493.5 | 450.1 | |
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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 | 1.62 | 0.00 | 0.96 | -15.70 | 53.10 | -30.74 | 116.87 | 0.5538 | 778.0 | 641.2 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -15.35 | 52.83 | -31.01 | 116.11 | 0.5554 | 645.0 | 497.6 | |
| 0.00 | 1.44 | 0.00 | 0.90 | -20.95 | 50.72 | -33.12 | 123.47 | 0.6140 | 654.0 | 481.5 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -20.17 | 50.79 | -33.05 | 122.38 | 0.6084 | 698.0 | 632.7 | |
| 0.00 | 1.44 | 0.00 | 0.90 | -20.40 | 50.74 | -33.10 | 122.68 | 0.6104 | 540.0 | 479.4 | |
| 0.00 | 2.88 | 0.00 | 1.81 | -20.65 | 50.52 | -33.32 | 122.91 | 0.6145 | 545.0 | 457.7 | |
| 0.00 | 2.61 | 0.00 | 1.61 | -18.07 | 50.85 | -32.99 | 119.23 | 0.5954 | 733.0 | 529.0 | |
| 0.00 | 1.98 | 0.00 | 1.20 | -15.39 | 51.23 | -32.62 | 115.20 | 0.5765 | 598.0 | 500.6 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -19.17 | 50.37 | -33.47 | 120.61 | 0.6075 | 284.0 | 310.6 | |
| 0.00 | 0.72 | 0.00 | 0.44 | -17.87 | 50.63 | -33.22 | 118.79 | 0.5971 | 556.0 | 416.9 | |
| 0.00 | 0.72 | 0.00 | 0.51 | -21.14 | 42.20 | -41.65 | 118.94 | 0.7105 | -603.0 | -534.9 | |
| 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. | |