SDO HMI 2014-05-18 20:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.12 | 70.84 | 10.83 | 36.30 | 10.17 | 180.19 | 8.17 | 327.02 | 0.2593 | -436.8 | -392.8 | |
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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 | 0.83 | 10.32 | 181.58 | 9.56 | 323.08 | 0.2731 | -723.0 | -601.1 | |
| 13.30 | 45.93 | 6.83 | 23.55 | 9.82 | 181.22 | 9.20 | 322.99 | 0.2628 | -1079.2 | -732.5 | |
| 6.11 | -2.00 | 3.13 | -2.00 | 9.42 | 181.08 | 9.06 | 322.44 | 0.2560 | -1223.0 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 10.18 | 178.96 | 6.94 | 331.09 | 0.2470 | -662.0 | -487.0 | |
| 0.36 | 5.66 | 0.18 | 2.90 | 10.74 | 178.91 | 6.89 | 332.34 | 0.2550 | -919.5 | -785.7 | |
| 0.00 | 1.80 | 0.00 | 0.94 | 15.62 | 178.96 | 6.94 | 339.23 | 0.3296 | 859.0 | 689.2 | |
| 0.00 | 3.15 | 0.00 | 1.61 | 10.96 | 178.76 | 6.74 | 333.25 | 0.2571 | -755.0 | -545.2 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 10.65 | 178.72 | 6.70 | 332.81 | 0.2521 | -656.0 | -547.3 | |
| 1.35 | 3.77 | 0.69 | 1.93 | 10.18 | 178.19 | 6.16 | 333.86 | 0.2409 | 836.3 | 725.2 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 10.55 | 178.10 | 6.08 | 334.85 | 0.2460 | 730.0 | 569.3 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 10.15 | 177.57 | 5.54 | 336.12 | 0.2360 | 880.0 | 790.8 | |
| 0.00 | 2.25 | 0.00 | 1.15 | 12.08 | 177.33 | 5.30 | 339.95 | 0.2648 | 794.0 | 691.3 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 9.77 | 176.32 | 4.30 | 340.48 | 0.2222 | 848.0 | 571.6 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 11.58 | 174.00 | 1.97 | 351.97 | 0.2427 | 857.0 | 759.2 | |
| 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. | |