SDO HMI 2011-07-25 00:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 32.01 | 0.00 | 17.08 | 24.64 | 78.28 | 9.80 | 334.99 | 0.3732 | -279.1 | -355.9 | |
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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 | 6.44 | 0.00 | 3.44 | 23.53 | 81.25 | 12.77 | 327.35 | 0.3774 | -948.0 | -754.9 | |
| 0.00 | 5.08 | 0.00 | 2.71 | 23.50 | 80.74 | 12.26 | 328.35 | 0.3727 | -1102.0 | -838.9 | |
| 0.00 | 1.90 | 0.00 | 1.01 | 23.55 | 80.26 | 11.79 | 329.38 | 0.3693 | -1016.0 | -852.0 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 22.53 | 79.84 | 11.36 | 328.71 | 0.3519 | -862.0 | -684.8 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 22.02 | 79.76 | 11.29 | 328.05 | 0.3444 | -701.0 | -578.9 | |
| 0.00 | 1.81 | 0.00 | 0.96 | 23.05 | 79.01 | 10.53 | 331.36 | 0.3524 | -955.0 | -732.5 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 23.99 | 78.61 | 10.13 | 333.57 | 0.3626 | -754.0 | -559.9 | |
| 0.00 | 4.53 | 0.00 | 2.41 | 25.08 | 77.13 | 8.66 | 338.21 | 0.3687 | -879.0 | -732.8 | |
| 0.00 | 2.45 | 0.00 | 1.32 | 27.22 | 74.84 | 6.36 | 345.29 | 0.3898 | 865.0 | 707.4 | |
| 0.00 | 1.81 | 0.00 | 0.98 | 27.42 | 74.78 | 6.31 | 345.56 | 0.3926 | 728.0 | 551.7 | |
| 0.00 | 3.08 | 0.00 | 1.65 | 26.74 | 74.37 | 5.89 | 345.99 | 0.3803 | 712.0 | 660.9 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 27.33 | 74.09 | 5.61 | 347.02 | 0.3886 | 676.0 | 561.1 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 26.09 | 73.92 | 5.45 | 346.56 | 0.3684 | 608.0 | 467.1 | |
| 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. | |