SDO HMI 2014-05-13 14:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.91 | 287.50 | 24.62 | 150.77 | 15.07 | 248.52 | 7.04 | 338.98 | 0.3311 | -686.4 | -416.3 | |
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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 |
| 0.00 | 1.17 | 0.00 | 0.62 | 15.91 | 249.11 | 7.63 | 338.31 | 0.3472 | -571.0 | -378.2 | |
| 15.43 | 265.86 | 8.11 | 139.44 | 15.27 | 248.90 | 7.42 | 338.15 | 0.3361 | -1090.9 | -476.7 | |
| 20.27 | -2.00 | 10.63 | -2.00 | 14.86 | 248.79 | 7.31 | 337.96 | 0.3291 | -1324.8 | 999999 | |
| 11.21 | -2.00 | 5.88 | -2.00 | 15.11 | 248.29 | 6.81 | 339.60 | 0.3300 | -1257.0 | 999999 | |
| 0.00 | 6.19 | 0.00 | 3.25 | 15.62 | 247.86 | 6.39 | 341.30 | 0.3356 | -737.0 | -601.3 | |
| 0.00 | 1.35 | 0.00 | 0.71 | 15.49 | 246.82 | 5.34 | 344.08 | 0.3283 | -733.0 | -569.9 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 14.50 | 246.54 | 5.06 | 344.00 | 0.3113 | 823.0 | 670.8 | |
| 0.00 | 3.59 | 0.00 | 1.89 | 16.25 | 246.52 | 5.04 | 345.53 | 0.3392 | 711.0 | 735.5 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 15.71 | 246.29 | 4.81 | 345.76 | 0.3296 | 971.0 | 808.1 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 16.00 | 246.20 | 4.72 | 346.23 | 0.3338 | 752.0 | 615.7 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 11.69 | 245.98 | 4.50 | 342.96 | 0.2636 | 813.0 | 668.5 | |
| 0.00 | 1.52 | 0.00 | 0.80 | 14.88 | 245.70 | 4.22 | 346.84 | 0.3139 | 813.0 | 742.0 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 13.01 | 244.14 | 2.66 | 350.60 | 0.2781 | 721.0 | 547.7 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 15.13 | 241.65 | 0.18 | 359.44 | 0.3100 | 640.0 | 515.4 | |
| 0.00 | 1.97 | 0.00 | 1.03 | 15.07 | 241.25 | -0.23 | 0.72 | 0.3090 | 981.0 | 851.5 | |
| 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. | |