SDO HMI 2014-06-09 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.33 | 0.00 | 10.15 | 5.22 | 259.82 | 15.58 | 266.49 | 0.2897 | 364.4 | 266.8 | |
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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 | 1.36 | 0.00 | 0.78 | 5.56 | 274.33 | 30.09 | 280.43 | 0.5093 | -698.0 | -586.7 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 6.06 | 272.91 | 28.67 | 281.87 | 0.4895 | -578.0 | -473.8 | |
| 0.00 | 2.35 | 0.00 | 1.32 | 3.13 | 271.92 | 27.68 | 276.07 | 0.4683 | -87.0 | -208.4 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 4.32 | 271.48 | 27.24 | 278.73 | 0.4636 | -879.0 | -648.2 | |
| 0.00 | 1.18 | 0.00 | 0.66 | 6.77 | 270.71 | 26.47 | 284.27 | 0.4586 | -856.0 | -643.4 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 1.95 | 262.03 | 17.79 | 275.29 | 0.3080 | 853.0 | 644.2 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 6.43 | 260.57 | 16.33 | 290.84 | 0.3003 | 922.0 | 772.8 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 11.03 | 257.99 | 13.75 | 308.49 | 0.2994 | 893.0 | 732.8 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 7.89 | 252.39 | 8.14 | 313.14 | 0.1932 | 723.0 | 511.0 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 7.83 | 251.24 | 7.00 | 317.23 | 0.1785 | 683.0 | 519.7 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 4.99 | 250.83 | 6.59 | 305.36 | 0.1407 | 763.0 | 501.6 | |
| 0.00 | 3.08 | 0.00 | 1.54 | 5.23 | 250.52 | 6.28 | 308.07 | 0.1390 | 1129.0 | 946.9 | |
| 0.00 | 0.91 | 0.00 | 0.45 | 7.75 | 249.75 | 5.51 | 323.55 | 0.1610 | 912.0 | 768.4 | |
| 0.00 | 1.00 | 0.00 | 0.49 | 1.47 | 243.33 | -0.91 | 38.97 | 0.0254 | 823.0 | 642.1 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 1.35 | 243.12 | -1.12 | 48.21 | 0.0264 | 863.0 | 750.5 | |
| 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. | |