SDO HMI 2014-04-11 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.35 | 118.23 | 42.87 | 172.61 | 4.31 | 241.30 | -69.57 | 83.23 | 0.9417 | -143.4 | 24.7 | |
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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 |
| 3.62 | 56.21 | 4.71 | 73.69 | 4.92 | 244.03 | -66.85 | 82.18 | 0.9263 | -858.5 | -341.6 | |
| 3.26 | -1.00 | 4.26 | -1.00 | 4.71 | 243.99 | -66.88 | 82.41 | 0.9263 | -818.6 | 999999 | |
| 5.91 | -1.00 | 7.65 | -1.00 | 4.37 | 244.05 | -66.82 | 82.76 | 0.9256 | -618.9 | 999999 | |
| 0.97 | -1.00 | 1.29 | -1.00 | 5.00 | 243.54 | -67.33 | 82.17 | 0.9295 | -300.1 | 999999 | |
| 2.47 | -1.00 | 3.30 | -1.00 | 4.83 | 243.42 | -67.46 | 82.37 | 0.9301 | -116.6 | 999999 | |
| 2.82 | -1.00 | 3.76 | -1.00 | 4.43 | 243.42 | -67.46 | 82.80 | 0.9298 | -291.7 | 999999 | |
| 2.21 | 6.35 | 2.95 | 8.50 | 4.14 | 243.31 | -67.57 | 83.13 | 0.9302 | -247.6 | -74.5 | |
| 0.00 | 0.71 | 0.00 | 0.96 | 4.37 | 242.86 | -68.01 | 82.95 | 0.9332 | 254.0 | 239.1 | |
| 0.00 | 0.97 | 0.00 | 1.42 | 3.71 | 241.21 | -69.67 | 83.89 | 0.9425 | -20.0 | -53.6 | |
| 0.00 | 0.35 | 0.00 | 0.53 | 5.58 | 240.79 | -70.08 | 81.99 | 0.9464 | -40.0 | -115.5 | |
| 0.00 | 1.24 | 0.00 | 1.86 | 4.49 | 240.70 | -70.18 | 83.14 | 0.9460 | 370.0 | 395.9 | |
| 0.00 | 0.26 | 0.00 | 0.43 | 5.13 | 239.13 | -71.74 | 82.70 | 0.9549 | 454.0 | 447.3 | |
| 8.38 | 46.85 | 13.66 | 75.51 | 3.91 | 239.13 | -71.74 | 83.97 | 0.9541 | 447.9 | 285.0 | |
| 0.71 | 3.53 | 1.29 | 6.48 | 5.17 | 237.27 | -73.61 | 82.92 | 0.9640 | 359.5 | 200.0 | |
| 0.00 | 1.76 | 0.00 | 3.23 | 4.74 | 237.28 | -73.59 | 83.36 | 0.9636 | 257.0 | 177.6 | |
| 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. | |