SDO HMI 2014-10-01 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.06 | 0.00 | 7.63 | -17.93 | 196.24 | 15.90 | 216.34 | 0.5013 | -513.7 | -381.0 | |
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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 | 1.15 | 0.00 | 0.79 | -26.26 | 210.43 | 30.10 | 220.32 | 0.6974 | 495.0 | 467.8 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -20.47 | 204.15 | 23.82 | 220.22 | 0.5881 | -730.0 | -646.9 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -15.44 | 202.60 | 22.27 | 224.74 | 0.5210 | -678.0 | -479.8 | |
| 0.00 | 1.50 | 0.00 | 0.84 | -11.95 | 200.42 | 20.08 | 227.02 | 0.4610 | -771.0 | -657.4 | |
| 0.00 | 1.94 | 0.00 | 1.02 | -6.99 | 195.49 | 15.15 | 228.11 | 0.3500 | -27.0 | -10.5 | |
| 0.00 | 0.71 | 0.00 | 0.42 | -22.92 | 196.48 | 16.14 | 207.59 | 0.5552 | -619.0 | -515.9 | |
| 0.00 | 1.59 | 0.00 | 0.82 | -2.32 | 194.06 | 13.72 | 237.07 | 0.2836 | -959.0 | -711.0 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -3.44 | 191.67 | 11.33 | 228.44 | 0.2633 | -776.0 | -619.1 | |
| 0.00 | 1.15 | 0.00 | 0.71 | -28.34 | 192.63 | 12.29 | 198.14 | 0.6041 | -630.0 | -569.6 | |
| 0.00 | 1.32 | 0.00 | 0.93 | -37.86 | 187.13 | 6.79 | 187.59 | 0.7096 | -482.0 | -344.7 | |
| 0.00 | 0.62 | 0.00 | 0.38 | -30.02 | 182.74 | 2.41 | 183.48 | 0.6013 | -474.0 | -462.4 | |
| 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. | |