SDO HMI 2014-09-25 07:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.82 | 0.00 | 8.01 | -15.43 | 289.07 | 29.01 | 231.35 | 0.6071 | 588.9 | 496.3 | |
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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 | 1.59 | 0.00 | 1.08 | -8.84 | 300.14 | 40.07 | 249.01 | 0.6836 | 354.0 | 358.7 | |
| 0.00 | 0.53 | 0.00 | 0.36 | -11.12 | 298.92 | 38.85 | 245.23 | 0.6802 | 623.0 | 535.3 | |
| 0.00 | 1.06 | 0.00 | 0.66 | -10.97 | 293.16 | 33.10 | 241.71 | 0.6110 | 659.0 | 594.4 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -10.66 | 292.68 | 32.62 | 241.82 | 0.6032 | 672.0 | 585.0 | |
| 0.00 | 0.62 | 0.00 | 0.39 | -11.81 | 292.50 | 32.44 | 239.99 | 0.6085 | 631.0 | 499.3 | |
| 0.00 | 1.06 | 0.00 | 0.66 | -11.93 | 292.41 | 32.34 | 239.74 | 0.6082 | 648.0 | 602.4 | |
| 0.00 | 0.62 | 0.00 | 0.38 | -12.94 | 291.35 | 31.28 | 237.44 | 0.6027 | 673.0 | 600.0 | |
| 0.00 | 1.24 | 0.00 | 0.80 | -22.53 | 287.58 | 27.51 | 221.65 | 0.6442 | 497.0 | 395.4 | |
| 0.00 | 1.33 | 0.00 | 0.77 | -15.37 | 283.00 | 22.93 | 225.38 | 0.5299 | 609.0 | 423.5 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -14.24 | 281.06 | 21.00 | 224.47 | 0.4978 | 498.0 | 448.3 | |
| 0.00 | 1.33 | 0.00 | 0.84 | -24.47 | 282.39 | 22.32 | 213.97 | 0.6209 | 614.0 | 516.6 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -21.59 | 280.26 | 20.19 | 214.28 | 0.5721 | 716.0 | 615.5 | |
| 0.00 | 0.71 | 0.00 | 0.43 | -21.58 | 280.05 | 19.99 | 214.01 | 0.5704 | 462.0 | 458.9 | |
| 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. | |