SDO HMI 2014-03-11 09:01:14 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.17 | 0.00 | 14.89 | -10.46 | 15.77 | 19.89 | 258.68 | 0.3423 | 433.1 | 387.6 | |
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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 | 2.26 | 0.00 | 1.24 | -9.99 | 21.88 | 26.00 | 261.98 | 0.4378 | 751.0 | 514.0 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -9.93 | 20.10 | 24.22 | 261.81 | 0.4100 | 669.0 | 495.4 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -9.39 | 18.91 | 23.03 | 262.95 | 0.3905 | 749.0 | 642.9 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -8.66 | 18.56 | 22.68 | 264.79 | 0.3845 | 777.0 | 626.4 | |
| 0.00 | 0.52 | 0.00 | 0.28 | -9.65 | 17.84 | 21.96 | 262.07 | 0.3739 | 714.0 | 611.7 | |
| 0.00 | 2.34 | 0.00 | 1.25 | -9.88 | 17.37 | 21.49 | 261.34 | 0.3667 | 995.0 | 893.7 | |
| 0.00 | 2.43 | 0.00 | 1.29 | -10.29 | 16.81 | 20.94 | 260.04 | 0.3585 | 994.0 | 805.7 | |
| 0.00 | 7.37 | 0.00 | 3.90 | -10.49 | 16.34 | 20.46 | 259.32 | 0.3514 | 643.0 | 705.4 | |
| 0.00 | 2.52 | 0.00 | 1.32 | -10.68 | 14.49 | 18.61 | 257.96 | 0.3221 | 834.0 | 643.0 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -10.22 | 12.49 | 16.61 | 258.46 | 0.2885 | 792.0 | 650.9 | |
| 0.00 | 0.69 | 0.00 | 0.36 | -9.42 | 11.38 | 15.50 | 260.76 | 0.2684 | 755.0 | 518.8 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -11.51 | 11.24 | 15.36 | 253.01 | 0.2726 | -784.0 | -596.4 | |
| 0.00 | 1.30 | 0.00 | 0.67 | -11.52 | 11.05 | 15.17 | 252.82 | 0.2696 | -836.0 | -668.2 | |
| 0.00 | 3.64 | 0.00 | 1.87 | -11.73 | 10.87 | 14.99 | 251.87 | 0.2677 | -989.0 | -803.4 | |
| 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. | |