SDO HMI 2014-08-22 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.39 | 48.84 | 11.34 | 25.99 | -9.43 | 332.82 | -13.51 | 140.74 | 0.3655 | 676.6 | 337.5 | |
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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 | 1.26 | 0.00 | 0.67 | -14.09 | 339.27 | -7.06 | 161.58 | 0.3789 | 692.0 | 503.7 | |
| 0.00 | 1.71 | 0.00 | 0.88 | -6.35 | 338.40 | -7.92 | 149.08 | 0.2678 | 903.0 | 772.8 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -10.16 | 338.26 | -8.07 | 154.74 | 0.3252 | 893.0 | 749.5 | |
| 0.00 | 1.53 | 0.00 | 0.80 | -8.72 | 335.68 | -10.64 | 145.72 | 0.3256 | 764.0 | 549.1 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -8.65 | 334.72 | -11.61 | 143.23 | 0.3338 | 849.0 | 668.6 | |
| 16.09 | 30.48 | 8.53 | 16.16 | -9.53 | 333.46 | -12.87 | 141.94 | 0.3578 | 1006.2 | 602.6 | |
| 5.30 | -6.00 | 2.81 | -6.00 | -9.31 | 333.47 | -12.86 | 141.57 | 0.3549 | 1108.2 | 999999 | |
| 0.00 | 2.61 | 0.00 | 1.43 | -14.05 | 331.37 | -14.96 | 144.73 | 0.4355 | -578.0 | -536.3 | |
| 0.00 | 2.52 | 0.00 | 1.32 | -5.68 | 331.23 | -15.10 | 129.58 | 0.3378 | 689.0 | 576.8 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -5.31 | 330.16 | -16.17 | 126.81 | 0.3477 | 809.0 | 616.9 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -11.30 | 329.64 | -16.69 | 137.56 | 0.4191 | 524.0 | 461.4 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -7.93 | 329.49 | -16.83 | 131.23 | 0.3830 | 661.0 | 448.2 | |
| 0.00 | 1.71 | 0.00 | 0.94 | -11.70 | 328.38 | -17.95 | 136.12 | 0.4372 | -803.0 | -717.4 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -7.08 | 322.68 | -23.64 | 120.26 | 0.4627 | -564.0 | -486.5 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -9.29 | 321.22 | -25.11 | 122.64 | 0.4992 | -68.0 | -83.3 | |
| 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. | |