SDO HMI 2014-08-10 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.28 | 46.92 | 6.76 | 26.02 | -18.57 | 160.62 | 9.09 | 199.64 | 0.4484 | 607.3 | 597.2 | |
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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 | 2.89 | 0.00 | 1.61 | -19.09 | 161.48 | 9.95 | 200.87 | 0.4603 | 683.0 | 623.2 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -18.79 | 161.43 | 9.90 | 201.02 | 0.4556 | 865.0 | 765.6 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -17.58 | 161.33 | 9.80 | 201.86 | 0.4376 | 214.0 | 287.1 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -18.45 | 161.38 | 9.85 | 201.20 | 0.4504 | 747.0 | 565.6 | |
| 8.76 | 12.91 | 4.80 | 7.08 | -17.18 | 161.02 | 9.49 | 201.59 | 0.4299 | 968.0 | 671.8 | |
| 1.17 | 16.16 | 0.65 | 9.01 | -19.05 | 161.09 | 9.56 | 200.15 | 0.4575 | 974.2 | 732.0 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -19.09 | 159.92 | 8.39 | 197.82 | 0.4523 | 660.0 | 557.0 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -20.89 | 159.95 | 8.42 | 196.66 | 0.4789 | -540.0 | -515.8 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -19.19 | 159.66 | 8.13 | 197.25 | 0.4525 | 749.0 | 689.1 | |
| 2.35 | 6.05 | 1.31 | 3.37 | -19.69 | 159.20 | 7.67 | 195.99 | 0.4579 | 856.7 | 623.0 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -15.65 | 158.84 | 7.31 | 198.13 | 0.3953 | 525.0 | 531.1 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -21.24 | 155.50 | 3.98 | 187.94 | 0.4696 | -734.0 | -641.6 | |
| 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. | |