SDO HMI 2014-08-01 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.84 | 38.04 | 9.30 | 22.39 | -20.81 | 249.00 | -19.34 | 145.01 | 0.5421 | 842.6 | 520.3 | |
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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 | 0.58 | -19.95 | 250.99 | -17.36 | 146.89 | 0.5153 | 589.0 | 542.5 | |
| 0.00 | 0.91 | 0.00 | 0.54 | -23.26 | 250.25 | -18.09 | 149.33 | 0.5614 | 631.0 | 419.9 | |
| 2.08 | 28.80 | 1.22 | 16.90 | -20.69 | 249.19 | -19.16 | 145.13 | 0.5391 | 824.9 | 513.0 | |
| 9.87 | -3.00 | 5.79 | -3.00 | -20.45 | 249.11 | -19.23 | 144.76 | 0.5369 | 1114.6 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.38 | -22.73 | 248.69 | -19.66 | 146.68 | 0.5669 | 745.0 | 519.7 | |
| 0.00 | 1.54 | 0.00 | 0.93 | -22.97 | 248.61 | -19.73 | 146.84 | 0.5704 | 633.0 | 484.4 | |
| 3.89 | -3.00 | 2.29 | -3.00 | -20.49 | 248.87 | -19.48 | 144.47 | 0.5395 | 786.3 | 999999 | |
| 0.00 | 2.90 | 0.00 | 1.74 | -22.70 | 248.45 | -19.90 | 146.34 | 0.5686 | 804.0 | 611.3 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -20.47 | 248.45 | -19.89 | 143.89 | 0.5428 | 525.0 | 426.2 | |
| 0.00 | 0.45 | 0.00 | 0.26 | -18.98 | 247.83 | -20.52 | 141.25 | 0.5315 | 718.0 | 614.2 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -19.42 | 247.63 | -20.71 | 141.53 | 0.5383 | 671.0 | 506.5 | |
| 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. | |