SDO HMI 2014-08-24 13:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.83 | 0.00 | 13.25 | -9.62 | 332.14 | 12.79 | 215.20 | 0.3703 | 166.3 | 272.5 | |
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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 | 1.44 | 0.00 | 0.82 | -11.11 | 342.34 | 22.99 | 231.82 | 0.4895 | 672.0 | 459.3 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -11.13 | 342.11 | 22.76 | 231.50 | 0.4869 | 694.0 | 567.1 | |
| 0.00 | 6.38 | 0.00 | 3.43 | -8.80 | 335.75 | 16.40 | 226.22 | 0.3881 | 840.0 | 736.4 | |
| 0.00 | 1.71 | 0.00 | 0.91 | -8.51 | 335.67 | 16.32 | 226.63 | 0.3840 | 1023.0 | 851.5 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -5.90 | 333.43 | 14.08 | 227.77 | 0.3283 | 945.0 | 836.8 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -13.61 | 332.80 | 13.45 | 212.95 | 0.4173 | -633.0 | -555.1 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -13.72 | 332.26 | 12.91 | 211.74 | 0.4143 | -857.0 | -633.6 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -13.90 | 331.82 | 12.47 | 210.63 | 0.4132 | -656.0 | -641.4 | |
| 0.00 | 1.71 | 0.00 | 0.89 | -7.67 | 330.81 | 11.47 | 218.15 | 0.3203 | 780.0 | 598.4 | |
| 0.00 | 2.07 | 0.00 | 1.08 | -8.81 | 330.25 | 10.90 | 214.66 | 0.3301 | 830.0 | 613.0 | |
| 0.00 | 0.72 | 0.00 | 0.38 | -9.47 | 330.15 | 10.80 | 213.29 | 0.3382 | 799.0 | 538.8 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -9.63 | 330.00 | 10.65 | 212.67 | 0.3390 | 808.0 | 667.9 | |
| 0.00 | 1.35 | 0.00 | 0.69 | -8.86 | 319.73 | 0.38 | 181.38 | 0.2746 | -970.0 | -727.7 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -9.33 | 319.24 | -0.11 | 179.62 | 0.2825 | -870.0 | -636.5 | |
| 0.00 | 1.80 | 0.00 | 0.93 | -8.98 | 319.15 | -0.20 | 179.28 | 0.2766 | -911.0 | -760.5 | |
| 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. | |