SDO HMI 2014-04-11 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.70 | 114.16 | 28.16 | 171.84 | 4.32 | 241.31 | -70.12 | 83.30 | 0.9448 | -36.1 | -10.5 | |
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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 |
| 2.47 | 57.52 | 3.30 | 77.41 | 4.92 | 243.96 | -67.46 | 82.27 | 0.9302 | -856.2 | -334.2 | |
| 3.35 | -1.00 | 4.45 | -1.00 | 4.34 | 244.00 | -67.43 | 82.89 | 0.9295 | -650.8 | 999999 | |
| 2.38 | -1.00 | 3.19 | -1.00 | 4.69 | 243.85 | -67.57 | 82.54 | 0.9307 | -753.8 | 999999 | |
| 1.59 | -1.00 | 2.16 | -1.00 | 4.97 | 243.47 | -67.96 | 82.30 | 0.9334 | -255.4 | 999999 | |
| 0.00 | 0.79 | 0.00 | 1.23 | 5.59 | 240.90 | -70.53 | 82.04 | 0.9488 | -238.0 | -129.7 | |
| 0.00 | 1.76 | 0.00 | 2.68 | 3.72 | 241.06 | -70.37 | 83.98 | 0.9465 | 78.0 | 91.8 | |
| 0.00 | 2.12 | 0.00 | 3.29 | 4.49 | 240.62 | -70.80 | 83.23 | 0.9495 | 379.0 | 383.6 | |
| 0.00 | 1.24 | 0.00 | 1.98 | 4.15 | 240.04 | -71.39 | 83.66 | 0.9524 | 446.0 | 435.4 | |
| 0.62 | 46.14 | 0.98 | 76.56 | 3.21 | 240.02 | -71.40 | 84.65 | 0.9518 | 358.6 | 260.6 | |
| 7.41 | -9.00 | 12.41 | -9.00 | 3.93 | 239.20 | -72.22 | 84.01 | 0.9565 | 464.6 | 999999 | |
| 0.88 | 2.56 | 1.67 | 4.84 | 5.16 | 237.28 | -74.14 | 83.00 | 0.9664 | 341.1 | 226.9 | |
| 0.00 | 2.03 | 0.00 | 3.85 | 4.78 | 237.18 | -74.25 | 83.41 | 0.9666 | 128.0 | 154.3 | |
| 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. | |