SDO HMI 2014-05-25 19:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.59 | 0.00 | 8.16 | -18.87 | 50.19 | -29.78 | 122.81 | 0.5605 | 545.3 | 407.6 | |
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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 | 0.99 | 0.00 | 0.57 | -15.70 | 53.20 | -26.77 | 119.85 | 0.5019 | 725.0 | 609.8 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -19.42 | 51.94 | -28.04 | 125.09 | 0.5438 | 768.0 | 613.5 | |
| 0.00 | 2.07 | 0.00 | 1.24 | -20.11 | 50.92 | -29.06 | 125.31 | 0.5610 | 756.0 | 639.7 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -20.27 | 50.81 | -29.16 | 125.47 | 0.5634 | 756.0 | 591.2 | |
| 0.00 | 2.25 | 0.00 | 1.33 | -18.07 | 51.20 | -28.77 | 122.29 | 0.5433 | 242.0 | 259.4 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -19.12 | 50.93 | -29.04 | 123.76 | 0.5538 | 643.0 | 456.8 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -14.74 | 51.67 | -28.30 | 116.93 | 0.5163 | 756.0 | 600.6 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -20.66 | 50.58 | -29.39 | 125.87 | 0.5689 | 560.0 | 505.7 | |
| 0.00 | 1.26 | 0.00 | 0.75 | -18.83 | 50.80 | -29.17 | 123.20 | 0.5534 | 683.0 | 582.1 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -15.27 | 51.13 | -28.85 | 117.46 | 0.5266 | 687.0 | 552.6 | |
| 0.00 | 1.44 | 0.00 | 0.96 | -21.25 | 42.29 | -37.68 | 121.10 | 0.6676 | -578.0 | -439.4 | |
| 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. | |