SDO HMI 2014-10-09 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.71 | 0.00 | 10.78 | 13.24 | 90.58 | 14.70 | 301.68 | 0.2900 | 124.6 | 207.2 | |
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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 | 1.32 | 0.00 | 0.74 | 9.39 | 104.24 | 28.37 | 278.18 | 0.4755 | -855.0 | -703.7 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 10.63 | 102.33 | 26.46 | 281.27 | 0.4484 | -734.0 | -507.2 | |
| 0.00 | 1.40 | 0.00 | 0.77 | 8.27 | 100.92 | 25.05 | 276.12 | 0.4232 | -696.0 | -555.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 8.35 | 98.35 | 22.47 | 276.70 | 0.3824 | -703.0 | -624.3 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 7.17 | 96.33 | 20.46 | 273.72 | 0.3490 | -751.0 | -617.9 | |
| 0.00 | 1.75 | 0.00 | 0.91 | 15.56 | 89.55 | 13.68 | 305.81 | 0.2821 | 795.0 | 576.8 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 15.68 | 88.19 | 12.31 | 308.94 | 0.2651 | 793.0 | 528.6 | |
| 0.00 | 1.67 | 0.00 | 0.86 | 15.94 | 87.85 | 11.98 | 310.44 | 0.2634 | 946.0 | 733.3 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 13.97 | 87.45 | 11.58 | 304.95 | 0.2387 | 824.0 | 663.4 | |
| 0.00 | 2.90 | 0.00 | 1.48 | 14.77 | 86.99 | 11.12 | 308.76 | 0.2402 | 925.0 | 871.7 | |
| 0.00 | 2.46 | 0.00 | 1.25 | 14.60 | 86.48 | 10.60 | 309.46 | 0.2317 | 530.0 | 468.5 | |
| 0.00 | 0.44 | 0.00 | 0.22 | 16.79 | 84.95 | 9.07 | 320.59 | 0.2389 | 690.0 | 584.6 | |
| 0.00 | 2.19 | 0.00 | 1.12 | 16.73 | 84.69 | 8.81 | 321.22 | 0.2354 | 931.0 | 791.2 | |
| 0.00 | 1.49 | 0.00 | 0.75 | 11.97 | 81.01 | 5.14 | 318.68 | 0.1333 | -950.0 | -755.6 | |
| 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. | |