SDO HMI 2014-10-08 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.70 | 20.45 | 0.36 | 10.42 | 9.90 | 99.34 | 11.91 | 270.50 | 0.2254 | -468.7 | -298.9 | |
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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 |
| 0.70 | 2.28 | 0.36 | 1.18 | 8.93 | 103.57 | 16.14 | 280.27 | 0.2803 | -879.0 | -728.2 | |
| 0.00 | 2.37 | 0.00 | 1.22 | 8.70 | 103.30 | 15.88 | 279.57 | 0.2755 | -850.0 | -757.6 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 9.38 | 102.67 | 15.25 | 282.41 | 0.2669 | 831.0 | 617.8 | |
| 0.00 | 3.95 | 0.00 | 2.03 | 9.29 | 102.48 | 15.05 | 282.22 | 0.2634 | 898.0 | 715.6 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 10.08 | 100.14 | 12.71 | 287.46 | 0.2281 | -953.0 | -699.7 | |
| 0.00 | 1.40 | 0.00 | 0.71 | 10.56 | 99.91 | 12.48 | 289.80 | 0.2268 | -763.0 | -674.9 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 10.44 | 98.72 | 11.29 | 291.00 | 0.2072 | -873.0 | -768.2 | |
| 0.00 | 1.84 | 0.00 | 0.93 | 10.11 | 98.61 | 11.19 | 289.64 | 0.2037 | -1107.0 | -928.5 | |
| 0.00 | 2.02 | 0.00 | 1.02 | 9.45 | 97.26 | 9.83 | 288.43 | 0.1784 | -913.0 | -743.2 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 11.93 | 96.48 | 9.05 | 302.76 | 0.1838 | -818.0 | -576.4 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 8.30 | 92.31 | 4.89 | 292.45 | 0.0916 | -910.0 | -719.0 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 14.82 | 84.10 | -3.33 | 20.80 | 0.1589 | 860.0 | 705.7 | |
| 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. | |