SDO HMI 2014-09-29 16:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.34 | 0.00 | 8.37 | -15.64 | 201.06 | -1.28 | 174.42 | 0.4002 | -211.9 | -164.1 | |
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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 | 0.88 | 0.00 | 0.47 | -11.22 | 211.97 | 9.63 | 208.09 | 0.3500 | 3.0 | 0.2 | |
| 0.00 | 1.67 | 0.00 | 0.99 | -24.80 | 211.26 | 8.93 | 195.09 | 0.5432 | 767.0 | 673.7 | |
| 0.00 | 1.41 | 0.00 | 0.83 | -25.22 | 211.09 | 8.75 | 194.60 | 0.5485 | 683.0 | 501.8 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -6.89 | 206.74 | 4.40 | 197.88 | 0.2492 | -878.0 | -723.5 | |
| 0.00 | 2.73 | 0.00 | 1.45 | -14.33 | 200.11 | -2.23 | 174.03 | 0.3637 | -784.0 | -607.6 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -20.50 | 198.45 | -3.89 | 172.11 | 0.4645 | -750.0 | -641.8 | |
| 0.00 | 1.50 | 0.00 | 0.79 | -13.00 | 197.41 | -4.93 | 166.08 | 0.3498 | -3.0 | 1.6 | |
| 0.00 | 0.53 | 0.00 | 0.32 | -26.41 | 195.67 | -6.67 | 169.23 | 0.5588 | -547.0 | -468.0 | |
| 0.00 | 1.59 | 0.00 | 0.82 | -6.93 | 193.91 | -8.42 | 148.33 | 0.2783 | 794.0 | 642.8 | |
| 0.00 | 2.12 | 0.00 | 1.09 | -6.92 | 192.87 | -9.47 | 145.24 | 0.2876 | -1117.0 | -867.9 | |
| 0.00 | 0.62 | 0.00 | 0.39 | -29.86 | 187.65 | -14.69 | 159.67 | 0.6352 | -499.0 | -426.0 | |
| 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. | |