SDO HMI 2014-09-05 21:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.85 | 0.00 | 9.74 | 10.66 | 178.83 | 22.43 | 285.30 | 0.3832 | -440.2 | -66.4 | |
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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 | 1.07 | 0.00 | 0.63 | 3.33 | 188.72 | 32.31 | 264.77 | 0.5379 | -655.0 | -467.8 | |
| 0.00 | 1.52 | 0.00 | 0.88 | 11.02 | 188.36 | 31.95 | 279.25 | 0.5284 | -723.0 | -596.4 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 10.78 | 188.33 | 31.92 | 278.79 | 0.5277 | -734.0 | -618.7 | |
| 0.00 | 1.43 | 0.00 | 0.82 | 10.94 | 187.27 | 30.86 | 279.24 | 0.5123 | -729.0 | -570.4 | |
| 0.00 | 1.25 | 0.00 | 0.72 | 10.90 | 186.91 | 30.50 | 279.22 | 0.5069 | -792.0 | -527.1 | |
| 0.00 | 1.07 | 0.00 | 0.61 | 11.39 | 186.43 | 30.02 | 280.27 | 0.5004 | -739.0 | -614.3 | |
| 0.00 | 1.16 | 0.00 | 0.66 | 11.00 | 185.88 | 29.48 | 279.57 | 0.4918 | -757.0 | -567.4 | |
| 0.00 | 0.80 | 0.00 | 0.45 | 7.24 | 183.84 | 27.44 | 271.75 | 0.4592 | -688.0 | -524.1 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 14.89 | 182.95 | 26.55 | 288.66 | 0.4578 | -753.0 | -595.2 | |
| 0.00 | 1.25 | 0.00 | 0.66 | 7.42 | 176.91 | 20.50 | 271.80 | 0.3490 | 759.0 | 551.0 | |
| 0.00 | 6.25 | 0.00 | 3.14 | 11.96 | 164.42 | 8.02 | 301.44 | 0.1607 | 969.0 | 749.1 | |
| 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. | |