SDO HMI 2014-08-08 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.79 | 0.00 | 10.53 | -18.70 | 159.56 | -12.38 | 154.32 | 0.4684 | 667.2 | 540.1 | |
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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 | 1.81 | 0.00 | 0.99 | -17.30 | 164.58 | -7.35 | 162.97 | 0.4190 | 792.0 | 678.3 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -17.51 | 160.60 | -11.34 | 154.94 | 0.4445 | 851.0 | 664.1 | |
| 0.00 | 1.63 | 0.00 | 0.92 | -19.84 | 159.91 | -12.03 | 155.87 | 0.4815 | 857.0 | 706.4 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -20.01 | 159.66 | -12.27 | 155.60 | 0.4854 | 769.0 | 545.3 | |
| 0.00 | 2.08 | 0.00 | 1.15 | -17.49 | 159.82 | -12.12 | 153.44 | 0.4496 | 904.0 | 730.4 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -20.87 | 159.49 | -12.45 | 156.06 | 0.4983 | 773.0 | 605.0 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -21.08 | 159.31 | -12.63 | 155.93 | 0.5023 | 679.0 | 543.6 | |
| 0.00 | 2.08 | 0.00 | 1.15 | -17.33 | 159.54 | -12.40 | 152.74 | 0.4494 | 697.0 | 585.9 | |
| 0.00 | 2.35 | 0.00 | 1.30 | -17.07 | 159.46 | -12.48 | 152.30 | 0.4463 | 862.0 | 696.4 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -18.17 | 159.25 | -12.69 | 153.08 | 0.4629 | 892.0 | 699.3 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -17.04 | 159.23 | -12.71 | 151.85 | 0.4476 | 774.0 | 558.7 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -20.75 | 157.39 | -14.54 | 152.49 | 0.5104 | 537.0 | 519.8 | |
| 0.00 | 1.45 | 0.00 | 0.85 | -21.83 | 154.59 | -17.35 | 149.31 | 0.5443 | -714.0 | -606.5 | |
| 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. | |