SDO HMI 2014-04-09 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.05 | 0.00 | 7.59 | -14.59 | 303.47 | -29.97 | 109.22 | 0.5124 | -48.4 | 15.6 | |
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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 | 0.88 | 0.00 | 0.56 | -12.40 | 295.14 | -38.30 | 102.39 | 0.6220 | -516.0 | -441.0 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -13.95 | 295.75 | -37.69 | 105.00 | 0.6166 | -675.0 | -587.4 | |
| 0.00 | 1.15 | 0.00 | 0.72 | -16.46 | 295.80 | -37.64 | 109.02 | 0.6218 | -474.0 | -383.9 | |
| 0.00 | 1.76 | 0.00 | 1.04 | -10.32 | 300.37 | -33.07 | 99.68 | 0.5467 | -598.0 | -471.6 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -16.34 | 296.11 | -37.33 | 108.93 | 0.6174 | -670.0 | -537.0 | |
| 0.00 | 1.06 | 0.00 | 0.65 | -15.11 | 297.96 | -35.48 | 107.50 | 0.5898 | -561.0 | -421.6 | |
| 0.00 | 2.29 | 0.00 | 1.25 | -11.15 | 309.43 | -24.01 | 103.81 | 0.4129 | 740.0 | 636.7 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -20.64 | 305.61 | -27.83 | 121.11 | 0.5123 | 588.0 | 485.8 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -15.47 | 310.96 | -22.48 | 114.98 | 0.4082 | 809.0 | 576.8 | |
| 0.00 | 1.15 | 0.00 | 0.64 | -20.01 | 308.80 | -24.64 | 122.61 | 0.4669 | 820.0 | 654.6 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -14.47 | 314.52 | -18.92 | 115.89 | 0.3504 | 5.0 | -4.6 | |
| 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. | |