SDO HMI 2014-04-14 08:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.24 | 398.51 | 36.20 | 208.44 | 11.70 | 274.87 | 6.89 | 338.46 | 0.3222 | -979.6 | -407.9 | |
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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 |
| 67.38 | 376.68 | 35.23 | 196.98 | 11.60 | 275.11 | 7.13 | 337.67 | 0.3215 | -1508.5 | -447.8 | |
| 1.86 | -1.00 | 0.97 | -1.00 | 12.26 | 274.94 | 6.96 | 338.90 | 0.3307 | -838.2 | 999999 | |
| 0.00 | 5.39 | 0.00 | 2.84 | 13.67 | 273.27 | 5.29 | 344.83 | 0.3442 | -654.0 | -592.0 | |
| 0.00 | 2.12 | 0.00 | 1.12 | 13.57 | 272.71 | 4.73 | 346.31 | 0.3404 | -914.0 | -695.5 | |
| 0.00 | 1.24 | 0.00 | 0.64 | 9.51 | 272.06 | 4.08 | 344.98 | 0.2720 | -837.0 | -620.0 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 12.90 | 271.15 | 3.17 | 350.38 | 0.3242 | 835.0 | 586.9 | |
| 0.00 | 1.86 | 0.00 | 0.98 | 13.78 | 270.05 | 2.07 | 353.98 | 0.3363 | 692.0 | 616.5 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 12.86 | 269.95 | 1.97 | 353.98 | 0.3209 | 832.0 | 630.4 | |
| 0.00 | 2.30 | 0.00 | 1.20 | 12.95 | 269.70 | 1.72 | 354.76 | 0.3221 | 958.0 | 879.9 | |
| 0.00 | 1.77 | 0.00 | 0.93 | 13.72 | 269.68 | 1.70 | 355.04 | 0.3346 | 856.0 | 641.0 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 12.95 | 269.24 | 1.26 | 356.16 | 0.3215 | 945.0 | 777.2 | |
| 0.00 | 0.71 | 0.00 | 0.38 | 15.45 | 268.98 | 1.00 | 357.34 | 0.3623 | 617.0 | 366.4 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 13.02 | 268.19 | 0.21 | 359.36 | 0.3218 | 856.0 | 637.6 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 13.27 | 268.10 | 0.12 | 359.64 | 0.3260 | 896.0 | 741.7 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 11.75 | 267.67 | -0.31 | 1.02 | 0.3008 | 678.0 | 570.9 | |
| 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. | |