SDO HMI 2014-05-30 03:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.10 | 39.72 | 6.80 | 23.79 | -19.80 | 51.22 | 28.60 | 233.41 | 0.5606 | 374.9 | 274.1 | |
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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 | 0.73 | -19.64 | 56.01 | 33.39 | 238.03 | 0.6132 | 608.0 | 483.8 | |
| 10.20 | 16.44 | 6.27 | 10.09 | -19.59 | 54.31 | 31.69 | 236.92 | 0.5929 | 818.1 | 632.4 | |
| 0.00 | 4.79 | 0.00 | 2.91 | -19.01 | 53.66 | 31.04 | 237.31 | 0.5814 | 716.0 | 667.7 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -14.81 | 52.54 | 29.92 | 243.33 | 0.5417 | 767.0 | 616.1 | |
| 0.00 | 1.08 | 0.00 | 0.65 | -17.04 | 52.83 | 30.21 | 239.81 | 0.5587 | 723.0 | 569.3 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -19.12 | 52.56 | 29.94 | 236.31 | 0.5689 | 192.0 | 191.2 | |
| 0.00 | 1.44 | 0.00 | 0.87 | -19.15 | 52.27 | 29.65 | 236.03 | 0.5656 | 737.0 | 599.4 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -23.04 | 52.98 | 30.36 | 230.86 | 0.6020 | 688.0 | 561.1 | |
| 0.00 | 1.81 | 0.00 | 1.08 | -20.48 | 51.01 | 28.40 | 232.93 | 0.5605 | 669.0 | 547.5 | |
| 0.90 | 2.53 | 0.53 | 1.47 | -19.59 | 48.63 | 26.01 | 232.09 | 0.5256 | -976.5 | -809.3 | |
| 0.00 | 1.35 | 0.00 | 0.79 | -22.55 | 47.11 | 24.49 | 225.98 | 0.5344 | 556.0 | 358.1 | |
| 0.00 | 2.08 | 0.00 | 1.17 | -22.01 | 42.54 | 19.92 | 221.21 | 0.4815 | -728.0 | -581.5 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -22.34 | 40.68 | 18.06 | 218.07 | 0.4669 | -696.0 | -557.6 | |
| 0.00 | 1.54 | 0.00 | 0.84 | -21.60 | 38.43 | 15.81 | 215.61 | 0.4369 | -740.0 | -520.2 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -20.76 | 34.62 | 12.00 | 209.77 | 0.3932 | -682.0 | -677.8 | |
| 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. | |