SDO HMI 2011-06-03 19:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.61 | 31.55 | 3.10 | 17.13 | 17.47 | 42.13 | 15.90 | 320.39 | 0.4066 | -13.5 | -71.1 | |
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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 | 0.99 | 0.00 | 0.55 | 15.80 | 47.09 | 20.86 | 309.09 | 0.4433 | 716.0 | 535.3 | |
| 4.07 | 12.38 | 2.25 | 6.85 | 17.99 | 45.54 | 19.31 | 315.04 | 0.4470 | -906.4 | -752.4 | |
| 1.54 | -2.00 | 0.85 | -2.00 | 18.02 | 45.31 | 19.08 | 315.43 | 0.4447 | -984.4 | 999999 | |
| 0.00 | 1.81 | 0.00 | 1.00 | 18.73 | 44.40 | 18.18 | 317.92 | 0.4427 | -617.0 | -576.8 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 16.55 | 44.18 | 17.95 | 314.58 | 0.4165 | -754.0 | -548.0 | |
| 0.00 | 1.90 | 0.00 | 1.04 | 18.37 | 43.02 | 16.79 | 319.53 | 0.4242 | -885.0 | -667.5 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 17.54 | 42.11 | 15.88 | 319.69 | 0.4050 | 895.0 | 635.0 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 17.34 | 41.79 | 15.57 | 319.92 | 0.3995 | -789.0 | -588.5 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 16.70 | 41.08 | 14.85 | 320.11 | 0.3845 | -761.0 | -593.2 | |
| 0.00 | 2.26 | 0.00 | 1.19 | 16.79 | 37.40 | 11.18 | 327.86 | 0.3503 | 936.0 | 723.6 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 16.51 | 36.84 | 10.61 | 328.72 | 0.3414 | 738.0 | 760.1 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 16.22 | 36.72 | 10.50 | 328.53 | 0.3365 | 947.0 | 752.9 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 16.31 | 35.76 | 9.54 | 331.04 | 0.3298 | 885.0 | 664.6 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 18.42 | 35.71 | 9.49 | 334.12 | 0.3598 | 695.0 | 484.1 | |
| 0.00 | 2.80 | 0.00 | 1.47 | 16.54 | 35.42 | 9.19 | 332.24 | 0.3303 | 652.0 | 637.0 | |
| 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. | |