SDO HMI 2014-09-19 13:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.59 | 29.34 | 3.54 | 18.38 | -21.01 | 310.49 | -25.48 | 138.94 | 0.6127 | -315.0 | -195.6 | |
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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 | 1.06 | 0.00 | 0.64 | -19.20 | 313.48 | -22.49 | 140.25 | 0.5671 | 743.0 | 595.4 | |
| 0.00 | 4.52 | 0.00 | 2.71 | -18.93 | 313.38 | -22.59 | 139.81 | 0.5652 | 843.0 | 719.9 | |
| 0.00 | 1.86 | 0.00 | 1.13 | -20.11 | 312.65 | -23.33 | 140.31 | 0.5844 | 823.0 | 629.5 | |
| 0.89 | 3.90 | 0.56 | 2.46 | -21.70 | 310.27 | -25.70 | 139.43 | 0.6218 | -857.3 | -715.2 | |
| 0.71 | 3.19 | 0.45 | 2.01 | -21.07 | 310.03 | -25.94 | 138.46 | 0.6177 | -867.6 | -625.0 | |
| 0.00 | 3.10 | 0.00 | 1.98 | -22.05 | 309.55 | -26.42 | 139.06 | 0.6316 | -632.0 | -519.2 | |
| 2.57 | 4.88 | 1.63 | 3.10 | -21.65 | 309.49 | -26.48 | 138.54 | 0.6282 | -825.3 | -667.0 | |
| 0.00 | 1.77 | 0.00 | 1.12 | -21.28 | 309.38 | -26.59 | 138.00 | 0.6256 | -696.0 | -505.4 | |
| 1.42 | 2.84 | 0.90 | 1.81 | -21.56 | 309.25 | -26.72 | 138.19 | 0.6295 | -660.1 | -545.2 | |
| 0.00 | 1.42 | 0.00 | 0.91 | -21.81 | 309.09 | -26.88 | 138.30 | 0.6333 | -418.0 | -304.5 | |
| 0.00 | 0.80 | 0.00 | 0.51 | -20.87 | 308.70 | -27.27 | 136.83 | 0.6281 | -621.0 | -536.3 | |
| 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. | |