SDO HMI 2014-09-19 08:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.97 | 0.00 | 10.00 | 8.12 | 333.71 | -5.00 | 169.34 | 0.1218 | 64.3 | 41.1 | |
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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 | 1.51 | 0.00 | 0.75 | 9.30 | 343.41 | 4.70 | 295.40 | 0.0900 | -863.0 | -736.4 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 8.97 | 343.26 | 4.54 | 292.63 | 0.0852 | -1014.0 | -779.2 | |
| 0.00 | 1.95 | 0.00 | 0.97 | 10.05 | 339.48 | 0.76 | 345.60 | 0.0530 | -985.0 | -698.7 | |
| 0.00 | 1.42 | 0.00 | 0.70 | 9.87 | 339.32 | 0.61 | 347.66 | 0.0493 | -834.0 | -670.2 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 8.58 | 338.59 | -0.12 | 4.85 | 0.0256 | -1000.0 | -785.8 | |
| 0.00 | 1.69 | 0.00 | 0.84 | 8.55 | 337.37 | -1.34 | 42.98 | 0.0342 | -931.0 | -725.1 | |
| 0.00 | 1.60 | 0.00 | 0.80 | 5.94 | 331.63 | -7.08 | 99.12 | 0.1247 | 845.0 | 648.0 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 3.73 | 330.71 | -8.00 | 112.67 | 0.1512 | 811.0 | 555.9 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 8.74 | 329.53 | -9.18 | 79.31 | 0.1612 | 765.0 | 555.7 | |
| 0.00 | 1.95 | 0.00 | 0.98 | 7.68 | 329.28 | -9.44 | 85.99 | 0.1636 | 828.0 | 600.6 | |
| 0.00 | 1.69 | 0.00 | 0.85 | 7.65 | 327.89 | -10.82 | 86.49 | 0.1873 | 919.0 | 663.5 | |
| 0.00 | 1.42 | 0.00 | 0.72 | 7.38 | 327.80 | -10.91 | 87.96 | 0.1887 | 672.0 | 662.5 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 7.91 | 327.32 | -11.39 | 85.28 | 0.1971 | 915.0 | 751.4 | |
| 0.00 | 1.77 | 0.00 | 0.90 | 8.18 | 327.25 | -11.46 | 83.94 | 0.1986 | 772.0 | 569.8 | |
| 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. | |