SDO HMI 2014-05-10 20:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.92 | 294.13 | 28.44 | 174.81 | 14.77 | 249.26 | -28.57 | 56.88 | 0.5542 | -647.4 | -288.3 | |
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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 |
| 0.90 | 279.90 | 0.53 | 166.13 | 15.40 | 249.84 | -27.99 | 55.39 | 0.5519 | -710.6 | -344.1 | |
| 11.91 | -1.00 | 7.05 | -1.00 | 14.52 | 249.54 | -28.29 | 57.04 | 0.5489 | -1299.2 | 999999 | |
| 26.96 | -1.00 | 16.02 | -1.00 | 14.97 | 249.40 | -28.43 | 56.46 | 0.5539 | -1082.6 | 999999 | |
| 8.15 | -1.00 | 4.84 | -1.00 | 14.63 | 249.16 | -28.66 | 57.20 | 0.5543 | -1008.5 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.75 | 12.25 | 247.41 | -30.42 | 62.42 | 0.5604 | 618.0 | 549.8 | |
| 0.00 | 3.67 | 0.00 | 2.21 | 13.39 | 247.26 | -30.57 | 60.72 | 0.5695 | 657.0 | 571.7 | |
| 0.00 | 0.90 | 0.00 | 0.55 | 15.60 | 246.59 | -31.24 | 57.85 | 0.5922 | 719.0 | 667.4 | |
| 0.00 | 1.52 | 0.00 | 0.93 | 14.16 | 246.71 | -31.12 | 59.93 | 0.5813 | 834.0 | 665.5 | |
| 0.00 | 1.25 | 0.00 | 0.76 | 13.88 | 246.64 | -31.19 | 60.42 | 0.5803 | 784.0 | 655.9 | |
| 0.00 | 1.34 | 0.00 | 0.83 | 15.44 | 246.39 | -31.44 | 58.23 | 0.5935 | 700.0 | 599.3 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 14.02 | 246.33 | -31.50 | 60.44 | 0.5850 | 615.0 | 536.9 | |
| 0.00 | 1.61 | 0.00 | 0.99 | 14.40 | 246.16 | -31.67 | 59.98 | 0.5896 | 769.0 | 654.2 | |
| 0.00 | 1.43 | 0.00 | 0.88 | 14.82 | 245.98 | -31.85 | 59.48 | 0.5944 | 728.0 | 534.2 | |
| 0.00 | 0.27 | 0.00 | 0.18 | 16.77 | 241.10 | -36.73 | 60.01 | 0.6635 | 449.0 | 489.0 | |
| 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. | |