SDO HMI 2014-04-03 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.92 | 0.00 | 16.58 | 4.92 | 25.67 | -31.33 | 70.84 | 0.5498 | -213.7 | -360.4 | |
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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 | 1.84 | 0.00 | 1.06 | 2.32 | 28.18 | -28.82 | 73.95 | 0.5032 | -793.0 | -675.6 | |
| 0.00 | 1.32 | 0.00 | 0.76 | 4.42 | 28.11 | -28.89 | 70.07 | 0.5144 | -759.0 | -610.4 | |
| 0.00 | 1.49 | 0.00 | 0.86 | 3.84 | 28.03 | -28.97 | 71.18 | 0.5126 | -1031.0 | -882.8 | |
| 0.00 | 1.23 | 0.00 | 0.71 | 4.06 | 28.03 | -28.98 | 70.79 | 0.5138 | -812.0 | -621.9 | |
| 0.00 | 2.11 | 0.00 | 1.22 | 3.69 | 27.59 | -29.41 | 71.75 | 0.5180 | -820.0 | -689.5 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 3.94 | 27.41 | -29.59 | 71.40 | 0.5219 | -806.0 | -663.7 | |
| 0.00 | 0.97 | 0.00 | 0.56 | 4.31 | 27.26 | -29.75 | 70.82 | 0.5259 | -688.0 | -558.6 | |
| 0.00 | 11.77 | 0.00 | 6.86 | 4.00 | 26.92 | -30.08 | 71.60 | 0.5290 | -490.0 | -571.2 | |
| 0.00 | 0.70 | 0.00 | 0.43 | 8.49 | 23.67 | -33.33 | 66.20 | 0.5962 | 457.0 | 464.6 | |
| 0.00 | 0.88 | 0.00 | 0.56 | 8.28 | 21.37 | -35.63 | 67.95 | 0.6242 | 477.0 | 456.8 | |
| 0.00 | 1.23 | 0.00 | 0.78 | 8.72 | 21.17 | -35.83 | 67.41 | 0.6289 | 664.0 | 489.8 | |
| 0.00 | 1.14 | 0.00 | 0.75 | 9.99 | 19.50 | -37.50 | 66.54 | 0.6559 | 625.0 | 469.7 | |
| 0.00 | 1.05 | 0.00 | 0.68 | 7.30 | 18.97 | -38.03 | 70.69 | 0.6498 | 532.0 | 460.8 | |
| 0.00 | 1.14 | 0.00 | 0.74 | 7.22 | 18.78 | -38.22 | 70.90 | 0.6518 | 452.0 | 503.5 | |
| 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. | |