SDO HMI 2014-04-11 19:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.03 | 0.00 | 9.61 | -13.37 | 304.29 | 2.76 | 203.49 | 0.1817 | 143.6 | 115.2 | |
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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 | 0.54 | -14.17 | 311.19 | 9.66 | 228.15 | 0.2193 | 898.0 | 704.6 | |
| 0.00 | 1.85 | 0.00 | 0.94 | -14.93 | 311.16 | 9.63 | 225.50 | 0.2276 | 997.0 | 768.9 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -14.02 | 310.94 | 9.40 | 227.92 | 0.2144 | 824.0 | 662.5 | |
| 0.00 | 1.94 | 0.00 | 0.98 | -12.21 | 310.71 | 9.18 | 234.40 | 0.1926 | 998.0 | 811.2 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -12.06 | 310.46 | 8.92 | 234.30 | 0.1876 | 885.0 | 665.1 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -11.54 | 308.99 | 7.45 | 231.93 | 0.1621 | 608.0 | 478.8 | |
| 0.00 | 1.15 | 0.00 | 0.57 | -6.21 | 306.43 | 4.89 | 265.83 | 0.0853 | 858.0 | 661.5 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -4.71 | 305.87 | 4.33 | 284.89 | 0.0783 | 885.0 | 666.1 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -12.87 | 299.33 | -2.21 | 162.88 | 0.1281 | -875.0 | -616.1 | |
| 0.00 | 2.29 | 0.00 | 1.15 | -13.35 | 298.31 | -3.23 | 157.16 | 0.1419 | -1048.0 | -894.8 | |
| 0.00 | 1.85 | 0.00 | 0.94 | -17.03 | 297.62 | -3.92 | 161.34 | 0.2053 | -835.0 | -513.9 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -17.20 | 296.82 | -4.71 | 158.25 | 0.2128 | -730.0 | -577.3 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -17.18 | 294.74 | -6.80 | 150.10 | 0.2279 | -724.0 | -525.8 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -16.96 | 294.62 | -6.92 | 149.18 | 0.2258 | -730.0 | -547.2 | |
| 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. | |