SDO HMI 2011-05-03 15:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.67 | 35.70 | 9.42 | 26.02 | -17.47 | 124.63 | 46.14 | 249.64 | 0.7351 | -69.9 | -11.3 | |
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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 |
| 8.21 | 14.37 | 6.30 | 11.01 | -17.01 | 127.53 | 49.05 | 250.99 | 0.7662 | 631.1 | 594.4 | |
| 0.00 | 1.34 | 0.00 | 1.00 | -17.96 | 126.10 | 47.62 | 249.44 | 0.7528 | 387.0 | 353.7 | |
| 0.00 | 1.52 | 0.00 | 1.13 | -18.11 | 125.63 | 47.15 | 249.13 | 0.7481 | 486.0 | 424.2 | |
| 0.00 | 1.70 | 0.00 | 1.24 | -16.39 | 124.97 | 46.49 | 251.26 | 0.7370 | 589.0 | 477.9 | |
| 4.46 | 6.78 | 3.12 | 4.75 | -17.07 | 122.39 | 43.91 | 249.67 | 0.7093 | -659.2 | -388.1 | |
| 0.00 | 2.77 | 0.00 | 1.90 | -17.29 | 121.19 | 42.70 | 249.03 | 0.6958 | -799.0 | -716.0 | |
| 0.00 | 0.62 | 0.00 | 0.44 | -19.74 | 121.78 | 43.30 | 245.81 | 0.7099 | -445.0 | -363.3 | |
| 0.00 | 0.98 | 0.00 | 0.67 | -17.36 | 120.99 | 42.51 | 248.87 | 0.6937 | -621.0 | -539.2 | |
| 0.00 | 1.16 | 0.00 | 0.80 | -19.04 | 121.20 | 42.72 | 246.58 | 0.7011 | -489.0 | -402.2 | |
| 0.00 | 0.98 | 0.00 | 0.68 | -19.27 | 121.06 | 42.57 | 246.22 | 0.7002 | -526.0 | -467.4 | |
| 0.00 | 1.52 | 0.00 | 1.04 | -18.75 | 120.80 | 42.32 | 246.86 | 0.6956 | -739.0 | -540.0 | |
| 0.00 | 1.07 | 0.00 | 0.74 | -19.56 | 121.02 | 42.53 | 245.81 | 0.7007 | -517.0 | -450.9 | |
| 0.00 | 0.89 | 0.00 | 0.62 | -19.41 | 120.84 | 42.35 | 245.95 | 0.6981 | -672.0 | -579.8 | |
| 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. | |