SDO HMI 2014-03-25 03:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.77 | 0.00 | 11.48 | -14.08 | 131.12 | -43.49 | 102.83 | 0.6867 | 533.1 | 445.1 | |
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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 | 1.57 | 0.00 | 0.94 | -10.74 | 140.05 | -34.56 | 98.97 | 0.5665 | 654.0 | 520.9 | |
| 0.00 | 0.87 | 0.00 | 0.54 | -7.11 | 138.00 | -36.61 | 92.65 | 0.5947 | 543.0 | 466.3 | |
| 0.00 | 1.22 | 0.00 | 0.77 | -6.33 | 136.32 | -38.29 | 91.48 | 0.6183 | 724.0 | 632.0 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -6.56 | 136.26 | -38.35 | 91.86 | 0.6190 | 685.0 | 627.6 | |
| 0.00 | 1.05 | 0.00 | 0.69 | -10.54 | 133.23 | -41.39 | 98.15 | 0.6589 | 574.0 | 458.4 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -19.09 | 130.78 | -43.83 | 110.37 | 0.7005 | 562.0 | 399.9 | |
| 0.00 | 1.31 | 0.00 | 0.88 | -14.80 | 131.94 | -42.67 | 104.40 | 0.6790 | 767.0 | 670.8 | |
| 0.00 | 1.14 | 0.00 | 0.77 | -15.05 | 131.36 | -43.25 | 104.70 | 0.6864 | 632.0 | 540.4 | |
| 0.00 | 1.57 | 0.00 | 1.04 | -8.73 | 132.52 | -42.09 | 95.42 | 0.6678 | 675.0 | 612.0 | |
| 0.00 | 1.49 | 0.00 | 1.02 | -15.45 | 130.57 | -44.04 | 105.15 | 0.6965 | 377.0 | 261.4 | |
| 0.00 | 1.05 | 0.00 | 0.76 | -18.74 | 128.02 | -46.59 | 109.30 | 0.7313 | 596.0 | 403.4 | |
| 0.00 | 1.92 | 0.00 | 1.42 | -18.06 | 126.96 | -47.65 | 108.20 | 0.7420 | 376.0 | 282.9 | |
| 0.00 | 0.61 | 0.00 | 0.46 | -19.18 | 125.92 | -48.69 | 109.51 | 0.7550 | 78.0 | 119.9 | |
| 0.00 | 0.61 | 0.00 | 0.48 | -21.17 | 124.46 | -50.15 | 111.84 | 0.7735 | 411.0 | 359.9 | |
| 0.00 | 0.87 | 0.00 | 0.73 | -19.30 | 120.77 | -53.84 | 108.93 | 0.8078 | 343.0 | 310.1 | |
| 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. | |