SDO HMI 2011-06-05 20:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.05 | 107.19 | 14.14 | 60.39 | -21.12 | 18.76 | 19.56 | 221.01 | 0.4785 | 504.8 | 359.8 | |
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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 | 1.09 | 0.00 | 0.61 | -20.04 | 20.71 | 21.51 | 225.33 | 0.4862 | 754.0 | 678.3 | |
| 23.42 | 84.19 | 13.22 | 47.52 | -20.66 | 19.62 | 20.41 | 222.96 | 0.4809 | 1139.5 | 462.0 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -22.42 | 18.97 | 19.76 | 219.50 | 0.4934 | 605.0 | 516.3 | |
| 0.00 | 3.53 | 0.00 | 2.00 | -22.32 | 18.53 | 19.33 | 219.04 | 0.4881 | 710.0 | 550.8 | |
| 1.63 | 3.17 | 0.92 | 1.79 | -21.99 | 18.31 | 19.11 | 219.19 | 0.4823 | 860.9 | 813.9 | |
| 0.00 | 2.80 | 0.00 | 1.59 | -23.54 | 16.58 | 17.38 | 214.58 | 0.4844 | 808.0 | 678.5 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -23.74 | 16.43 | 17.23 | 214.10 | 0.4856 | 579.0 | 501.2 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -20.62 | 14.52 | 15.32 | 215.24 | 0.4303 | -616.0 | -402.3 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -22.59 | 14.19 | 14.99 | 212.02 | 0.4522 | -627.0 | -483.4 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -23.05 | 13.69 | 14.49 | 210.61 | 0.4541 | -596.0 | -459.1 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -22.72 | 12.64 | 13.44 | 209.17 | 0.4415 | -773.0 | -560.2 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -23.68 | 12.36 | 13.16 | 207.57 | 0.4524 | -809.0 | -643.1 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -24.01 | 11.44 | 12.24 | 205.57 | 0.4504 | -738.0 | -656.3 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -25.45 | 10.76 | 11.56 | 202.94 | 0.4661 | -597.0 | -421.1 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -23.91 | 10.62 | 11.41 | 204.17 | 0.4436 | -857.0 | -648.9 | |
| 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. | |