SDO HMI 2014-04-11 20:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.57 | 0.00 | 9.76 | -20.33 | 323.20 | 22.21 | 231.93 | 0.4530 | 5.7 | -30.6 | |
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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 | 1.06 | 0.00 | 0.62 | -15.07 | 332.67 | 31.69 | 251.02 | 0.5385 | 691.0 | 568.2 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -17.24 | 332.65 | 31.67 | 247.11 | 0.5464 | 666.0 | 599.0 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -17.17 | 331.03 | 30.04 | 246.39 | 0.5240 | 702.0 | 630.6 | |
| 0.00 | 1.76 | 0.00 | 1.02 | -16.97 | 330.74 | 29.75 | 246.60 | 0.5192 | 655.0 | 499.0 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -18.88 | 330.83 | 29.85 | 243.20 | 0.5297 | 581.0 | 481.7 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -16.86 | 329.07 | 28.08 | 245.83 | 0.4958 | 704.0 | 645.4 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -16.81 | 328.91 | 27.93 | 245.84 | 0.4934 | 875.0 | 815.6 | |
| 0.00 | 1.15 | 0.00 | 0.64 | -18.75 | 325.24 | 24.26 | 239.26 | 0.4546 | 671.0 | 572.5 | |
| 0.00 | 1.24 | 0.00 | 0.67 | -21.28 | 319.42 | 18.43 | 227.43 | 0.4017 | -645.0 | -484.5 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -23.61 | 317.02 | 16.04 | 219.39 | 0.4006 | -833.0 | -750.5 | |
| 0.00 | 1.68 | 0.00 | 0.89 | -22.00 | 315.96 | 14.97 | 220.45 | 0.3708 | -890.0 | -721.9 | |
| 0.00 | 1.68 | 0.00 | 0.90 | -24.30 | 315.98 | 15.00 | 216.45 | 0.3986 | -884.0 | -780.6 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -25.23 | 314.52 | 13.53 | 212.37 | 0.3971 | -589.0 | -470.6 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -25.01 | 314.43 | 13.44 | 212.53 | 0.3934 | -821.0 | -663.6 | |
| 0.00 | 1.68 | 0.00 | 0.90 | -24.50 | 314.17 | 13.18 | 212.81 | 0.3846 | -797.0 | -619.6 | |
| 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. | |