SDO HMI 2014-08-09 03:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.66 | 0.00 | 14.64 | -18.92 | 160.04 | -3.06 | 173.37 | 0.4318 | 731.1 | 634.5 | |
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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 | 2.17 | 0.00 | 1.18 | -17.60 | 165.04 | 1.94 | 184.54 | 0.4084 | 720.0 | 595.1 | |
| 0.00 | 1.81 | 0.00 | 1.00 | -20.05 | 160.73 | -2.37 | 174.99 | 0.4476 | 861.0 | 665.8 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -20.25 | 160.69 | -2.41 | 174.96 | 0.4508 | 646.0 | 461.9 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -19.85 | 160.70 | -2.40 | 174.89 | 0.4445 | 730.0 | 548.8 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -20.09 | 160.53 | -2.57 | 174.59 | 0.4484 | 888.0 | 753.3 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -19.58 | 160.48 | -2.62 | 174.36 | 0.4406 | 842.0 | 605.1 | |
| 0.00 | 2.08 | 0.00 | 1.15 | -20.29 | 160.37 | -2.73 | 174.29 | 0.4519 | 721.0 | 661.1 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -19.99 | 159.98 | -3.12 | 173.42 | 0.4478 | 653.0 | 579.2 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -17.30 | 160.00 | -3.10 | 172.66 | 0.4055 | 961.0 | 778.1 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -20.26 | 159.75 | -3.35 | 173.01 | 0.4524 | 721.0 | 528.5 | |
| 0.00 | 5.51 | 0.00 | 2.98 | -17.20 | 159.72 | -3.38 | 171.96 | 0.4046 | 211.0 | 669.8 | |
| 0.00 | 1.45 | 0.00 | 0.78 | -16.90 | 159.72 | -3.38 | 171.86 | 0.3998 | 911.0 | 792.4 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -21.18 | 159.56 | -3.54 | 172.90 | 0.4670 | 745.0 | 558.5 | |
| 0.00 | 2.53 | 0.00 | 1.37 | -16.65 | 158.52 | -4.58 | 168.90 | 0.3990 | 718.0 | 628.9 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -24.31 | 153.90 | -9.20 | 164.01 | 0.5308 | 638.0 | 552.7 | |
| 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. | |