SDO HMI 2014-07-02 16:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.45 | 17.81 | 0.24 | 10.06 | 6.84 | 271.06 | -27.63 | 81.33 | 0.4661 | 31.5 | 34.6 | |
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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 |
| 0.45 | 2.00 | 0.24 | 1.05 | 4.74 | 279.44 | -19.25 | 84.26 | 0.3317 | -1090.2 | -900.6 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 4.53 | 279.35 | -19.34 | 84.93 | 0.3329 | -884.0 | -677.2 | |
| 0.00 | 1.73 | 0.00 | 0.91 | 3.79 | 279.21 | -19.49 | 87.16 | 0.3347 | -788.0 | -617.8 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 6.29 | 279.07 | -19.63 | 79.79 | 0.3407 | -837.0 | -672.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 5.41 | 275.94 | -22.75 | 83.21 | 0.3893 | -755.0 | -516.5 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 4.17 | 274.55 | -24.14 | 86.55 | 0.4104 | -840.0 | -692.9 | |
| 0.00 | 1.18 | 0.00 | 0.68 | 8.98 | 268.64 | -30.05 | 77.36 | 0.5089 | 692.0 | 630.2 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 8.03 | 268.62 | -30.08 | 79.23 | 0.5071 | 832.0 | 692.8 | |
| 0.00 | 1.54 | 0.00 | 0.91 | 10.57 | 266.97 | -31.73 | 74.94 | 0.5374 | 610.0 | 578.8 | |
| 0.00 | 0.73 | 0.00 | 0.43 | 10.69 | 266.70 | -32.00 | 74.82 | 0.5416 | 573.0 | 503.9 | |
| 0.00 | 0.82 | 0.00 | 0.48 | 10.93 | 266.48 | -32.21 | 74.46 | 0.5453 | 682.0 | 544.1 | |
| 0.00 | 1.00 | 0.00 | 0.60 | 11.37 | 265.65 | -33.04 | 73.98 | 0.5583 | 640.0 | 510.7 | |
| 0.00 | 0.73 | 0.00 | 0.44 | 9.63 | 263.96 | -34.73 | 77.52 | 0.5775 | 692.0 | 604.4 | |
| 0.00 | 0.91 | 0.00 | 0.55 | 6.20 | 264.02 | -34.67 | 83.47 | 0.5714 | 598.0 | 437.5 | |
| 0.00 | 1.09 | 0.00 | 0.71 | 1.63 | 258.38 | -40.31 | 91.05 | 0.6490 | 617.0 | 534.2 | |
| 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. | |