SDO HMI 2014-08-24 15:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.94 | 0.00 | 11.71 | -9.51 | 331.84 | 13.60 | 218.08 | 0.3745 | 144.2 | 299.6 | |
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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 | 0.90 | 0.00 | 0.49 | -6.06 | 338.95 | 20.70 | 238.17 | 0.4155 | 644.0 | 453.2 | |
| 0.00 | 6.64 | 0.00 | 3.59 | -8.84 | 335.80 | 17.56 | 228.11 | 0.4021 | 555.0 | 726.3 | |
| 0.00 | 1.53 | 0.00 | 0.82 | -8.52 | 335.69 | 17.44 | 228.53 | 0.3974 | 1150.0 | 926.8 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -5.91 | 333.52 | 15.28 | 230.10 | 0.3431 | 895.0 | 786.6 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -13.61 | 332.91 | 14.67 | 215.25 | 0.4282 | -759.0 | -551.2 | |
| 0.00 | 1.71 | 0.00 | 0.93 | -13.69 | 332.31 | 14.06 | 214.02 | 0.4238 | -733.0 | -545.2 | |
| 0.00 | 1.62 | 0.00 | 0.88 | -13.90 | 331.93 | 13.69 | 213.02 | 0.4233 | -170.0 | -219.3 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -7.00 | 330.60 | 12.35 | 221.60 | 0.3212 | 856.0 | 588.6 | |
| 0.00 | 1.89 | 0.00 | 0.99 | -8.81 | 330.28 | 12.03 | 217.36 | 0.3410 | 913.0 | 737.9 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -8.99 | 330.16 | 11.91 | 216.75 | 0.3422 | 855.0 | 677.8 | |
| 0.00 | 0.72 | 0.00 | 0.38 | -11.98 | 324.03 | 5.78 | 196.89 | 0.3408 | -699.0 | -562.9 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -8.86 | 319.70 | 1.46 | 185.25 | 0.2757 | -721.0 | -616.1 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -8.95 | 319.18 | 0.94 | 183.36 | 0.2766 | -911.0 | -795.5 | |
| 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. | |