SDO HMI 2014-09-19 06:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.03 | 0.00 | 10.05 | 8.84 | 335.01 | -4.79 | 162.92 | 0.1315 | -107.9 | -89.4 | |
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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 | 3.37 | 0.00 | 1.67 | 8.66 | 343.49 | 3.69 | 292.89 | 0.0693 | -743.0 | -834.5 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 9.29 | 343.29 | 3.48 | 302.31 | 0.0712 | -953.0 | -733.3 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 11.29 | 342.30 | 2.49 | 329.59 | 0.0846 | -900.0 | -719.9 | |
| 0.00 | 1.95 | 0.00 | 0.97 | 10.51 | 341.34 | 1.53 | 335.96 | 0.0648 | -926.0 | -685.3 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 8.50 | 339.41 | -0.40 | 16.11 | 0.0249 | -947.0 | -716.8 | |
| 0.00 | 0.98 | 0.00 | 0.48 | 8.62 | 338.50 | -1.31 | 41.15 | 0.0345 | -1001.0 | -818.4 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 8.73 | 337.18 | -2.62 | 58.22 | 0.0535 | -817.0 | -610.1 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 6.36 | 331.59 | -8.21 | 94.96 | 0.1432 | 911.0 | 783.4 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 7.46 | 328.12 | -11.69 | 87.65 | 0.2019 | 830.0 | 617.6 | |
| 0.00 | 2.66 | 0.00 | 1.35 | 8.07 | 327.33 | -12.48 | 84.85 | 0.2158 | 847.0 | 693.5 | |
| 0.00 | 1.77 | 0.00 | 0.90 | 7.70 | 326.96 | -12.84 | 86.62 | 0.2217 | 801.0 | 650.8 | |
| 0.00 | 1.42 | 0.00 | 0.72 | 7.94 | 326.86 | -12.94 | 85.57 | 0.2235 | 784.0 | 747.9 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 14.36 | 323.10 | -16.71 | 64.84 | 0.3091 | 711.0 | 629.1 | |
| 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. | |