SDO HMI 2014-09-04 13:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.91 | 0.00 | 10.05 | 8.82 | 182.99 | 8.95 | 238.07 | 0.1856 | -504.2 | -478.4 | |
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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 | 1.16 | 0.00 | 0.59 | 11.46 | 188.10 | 14.07 | 288.05 | 0.2517 | -771.0 | -629.2 | |
| 0.00 | 2.32 | 0.00 | 1.18 | 10.72 | 186.33 | 12.29 | 287.00 | 0.2197 | -668.0 | -616.7 | |
| 0.00 | 2.23 | 0.00 | 1.13 | 11.18 | 186.13 | 12.09 | 289.28 | 0.2187 | -1033.0 | -832.8 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 10.95 | 185.99 | 11.96 | 288.40 | 0.2153 | -985.0 | -809.3 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 10.80 | 185.95 | 11.92 | 287.77 | 0.2140 | -868.0 | -793.1 | |
| 0.00 | 1.61 | 0.00 | 0.81 | 5.75 | 185.67 | 11.63 | 263.44 | 0.2029 | -890.0 | -688.2 | |
| 0.00 | 2.14 | 0.00 | 1.08 | 5.94 | 185.45 | 11.42 | 264.23 | 0.1988 | -1003.0 | -834.8 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 10.96 | 185.45 | 11.42 | 289.19 | 0.2068 | -929.0 | -726.8 | |
| 0.00 | 1.97 | 0.00 | 0.99 | 5.95 | 185.05 | 11.02 | 264.03 | 0.1920 | -928.0 | -764.2 | |
| 0.00 | 0.80 | 0.00 | 0.41 | 10.55 | 185.09 | 11.06 | 287.73 | 0.1989 | -874.0 | -693.0 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 10.33 | 172.88 | -1.15 | 20.02 | 0.0580 | 727.0 | 596.9 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 9.48 | 171.60 | -2.44 | 46.72 | 0.0579 | 886.0 | 682.8 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 2.65 | 168.59 | -5.45 | 129.85 | 0.1241 | 781.0 | 569.7 | |
| 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. | |