SDO HMI 2014-10-09 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.00 | 0.00 | 11.28 | -16.17 | 106.29 | 29.87 | 231.48 | 0.6116 | 216.8 | 186.7 | |
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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 | 1.05 | 0.00 | 0.69 | -13.00 | 112.80 | 36.38 | 241.84 | 0.6578 | 562.0 | 519.4 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -13.68 | 110.72 | 34.30 | 239.47 | 0.6379 | 474.0 | 470.6 | |
| 0.00 | 2.37 | 0.00 | 1.56 | -16.58 | 110.95 | 34.53 | 235.74 | 0.6597 | 637.0 | 473.4 | |
| 0.00 | 3.42 | 0.00 | 2.18 | -13.40 | 110.30 | 33.88 | 239.55 | 0.6313 | 631.0 | 415.4 | |
| 0.00 | 0.70 | 0.00 | 0.46 | -15.82 | 110.65 | 34.23 | 236.52 | 0.6512 | 628.0 | 536.0 | |
| 0.00 | 0.53 | 0.00 | 0.34 | -15.62 | 110.58 | 34.15 | 236.72 | 0.6490 | 572.0 | 541.5 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -16.65 | 110.59 | 34.17 | 235.37 | 0.6562 | 788.0 | 653.3 | |
| 0.00 | 1.23 | 0.00 | 0.78 | -13.47 | 109.98 | 33.56 | 239.21 | 0.6280 | 692.0 | 606.0 | |
| 0.00 | 0.97 | 0.00 | 0.63 | -15.89 | 110.21 | 33.79 | 236.09 | 0.6468 | 724.0 | 612.4 | |
| 0.00 | 0.44 | 0.00 | 0.30 | -26.43 | 105.59 | 29.17 | 219.58 | 0.6873 | 371.0 | 341.6 | |
| 0.00 | 0.61 | 0.00 | 0.36 | -16.09 | 100.81 | 24.38 | 226.89 | 0.5454 | -782.0 | -596.9 | |
| 0.00 | 1.32 | 0.00 | 0.80 | -21.09 | 99.85 | 23.43 | 219.42 | 0.5864 | -777.0 | -525.4 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -13.51 | 95.13 | 18.71 | 223.13 | 0.4581 | -654.0 | -521.6 | |
| 0.00 | 2.90 | 0.00 | 1.66 | -19.42 | 92.69 | 16.27 | 211.59 | 0.5064 | -831.0 | -650.2 | |
| 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. | |