SDO HMI 2014-06-11 00:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.60 | 0.00 | 10.90 | 6.39 | 256.20 | 30.74 | 282.27 | 0.5153 | 485.5 | 348.6 | |
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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 | 1.00 | 0.00 | 0.70 | 5.22 | 270.12 | 44.66 | 276.90 | 0.7074 | -687.0 | -567.0 | |
| 0.00 | 2.72 | 0.00 | 1.90 | 5.59 | 270.15 | 44.69 | 277.41 | 0.7082 | -220.0 | -227.4 | |
| 0.00 | 1.36 | 0.00 | 0.83 | 6.29 | 261.13 | 35.67 | 280.01 | 0.5907 | 648.0 | 482.5 | |
| 0.00 | 1.54 | 0.00 | 0.90 | 9.91 | 255.84 | 30.38 | 288.28 | 0.5268 | 601.0 | 550.4 | |
| 0.00 | 1.18 | 0.00 | 0.67 | 7.00 | 254.88 | 29.42 | 283.17 | 0.5027 | 608.0 | 544.3 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 6.66 | 254.36 | 28.90 | 282.71 | 0.4941 | 713.0 | 620.1 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 9.70 | 254.40 | 28.94 | 288.64 | 0.5054 | 703.0 | 629.4 | |
| 0.00 | 2.90 | 0.00 | 1.64 | 6.69 | 254.05 | 28.59 | 282.89 | 0.4895 | 590.0 | 458.5 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 6.33 | 253.54 | 28.08 | 282.35 | 0.4808 | 647.0 | 505.2 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 0.11 | 246.48 | 21.02 | 268.99 | 0.3603 | 696.0 | 535.3 | |
| 0.00 | 3.62 | 0.00 | 1.93 | 6.76 | 245.92 | 20.46 | 287.50 | 0.3656 | 758.0 | 649.7 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 3.07 | 237.66 | 12.20 | 281.99 | 0.2167 | 769.0 | 613.6 | |
| 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. | |