SDO HMI 2014-04-10 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.08 | 0.00 | 8.19 | -15.07 | 302.41 | -21.67 | 117.00 | 0.3953 | -254.5 | -162.8 | |
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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 | 0.79 | 0.00 | 0.40 | -11.48 | 320.30 | -3.78 | 145.98 | 0.1159 | 713.0 | 507.8 | |
| 0.00 | 2.47 | 0.00 | 1.25 | -11.50 | 313.37 | -10.70 | 118.21 | 0.2074 | 882.0 | 741.3 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -18.29 | 309.45 | -14.63 | 132.01 | 0.3241 | 640.0 | 484.8 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -20.65 | 302.29 | -21.79 | 126.81 | 0.4356 | 723.0 | 575.7 | |
| 0.00 | 1.50 | 0.00 | 0.82 | -16.44 | 300.41 | -23.66 | 116.22 | 0.4309 | -758.0 | -629.2 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -15.92 | 300.41 | -23.67 | 115.09 | 0.4280 | -769.0 | -612.1 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -15.54 | 299.26 | -24.81 | 113.40 | 0.4424 | -664.0 | -471.5 | |
| 0.00 | 1.68 | 0.00 | 0.93 | -14.71 | 298.44 | -25.64 | 111.08 | 0.4504 | -730.0 | -531.8 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -16.81 | 295.78 | -28.29 | 113.74 | 0.4977 | -766.0 | -665.8 | |
| 0.00 | 0.53 | 0.00 | 0.30 | -16.62 | 295.67 | -28.40 | 113.31 | 0.4983 | -504.0 | -514.2 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -14.32 | 295.98 | -28.09 | 108.94 | 0.4843 | -697.0 | -595.0 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -11.86 | 296.12 | -27.96 | 103.96 | 0.4747 | -734.0 | -735.3 | |
| 0.00 | 0.53 | 0.00 | 0.30 | -14.35 | 294.20 | -29.87 | 108.20 | 0.5099 | -644.0 | -547.0 | |
| 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. | |