SDO HMI 2014-07-06 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 33.97 | 0.00 | 17.89 | -13.84 | 256.10 | 9.25 | 207.37 | 0.3389 | 588.1 | 586.6 | |
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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 | 1.63 | 0.00 | 0.86 | -11.69 | 259.71 | 12.85 | 219.99 | 0.3404 | 801.0 | 612.6 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -12.93 | 259.71 | 12.85 | 217.70 | 0.3559 | 796.0 | 641.0 | |
| 0.00 | 2.36 | 0.00 | 1.26 | -13.75 | 259.62 | 12.76 | 216.10 | 0.3657 | 778.0 | 684.6 | |
| 0.00 | 2.18 | 0.00 | 1.16 | -13.88 | 259.43 | 12.58 | 215.50 | 0.3656 | 697.0 | 622.8 | |
| 0.00 | 4.18 | 0.00 | 2.22 | -14.22 | 258.55 | 11.69 | 213.03 | 0.3620 | 747.0 | 691.6 | |
| 0.00 | 1.82 | 0.00 | 0.96 | -13.99 | 258.38 | 11.52 | 213.00 | 0.3574 | 827.0 | 642.2 | |
| 0.00 | 0.82 | 0.00 | 0.43 | -12.31 | 256.05 | 9.19 | 209.96 | 0.3139 | 829.0 | 690.7 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -13.26 | 255.67 | 8.82 | 207.49 | 0.3246 | 840.0 | 600.5 | |
| 0.00 | 9.81 | 0.00 | 5.17 | -14.53 | 255.37 | 8.51 | 204.95 | 0.3412 | 1044.0 | 860.0 | |
| 0.00 | 2.09 | 0.00 | 1.10 | -14.65 | 254.20 | 7.34 | 201.73 | 0.3353 | 905.0 | 690.4 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -12.04 | 254.00 | 7.14 | 204.52 | 0.2941 | 783.0 | 666.1 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -14.95 | 251.76 | 4.91 | 194.69 | 0.3274 | -872.0 | -700.5 | |
| 0.00 | 2.09 | 0.00 | 1.09 | -14.82 | 251.38 | 4.52 | 193.69 | 0.3238 | -996.0 | -750.7 | |
| 0.00 | 1.91 | 0.00 | 0.98 | -11.16 | 251.04 | 4.18 | 195.85 | 0.2631 | 1054.0 | 832.6 | |
| 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. | |