SDO HMI 2014-09-22 22:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.94 | 24.60 | 6.30 | 18.00 | -15.00 | 249.13 | -42.28 | 118.03 | 0.7375 | 93.7 | -198.9 | |
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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 |
| 4.34 | 12.56 | 3.06 | 8.85 | -15.46 | 251.66 | -39.74 | 119.99 | 0.7137 | 725.3 | 530.0 | |
| 4.60 | -1.00 | 3.24 | -1.00 | -15.24 | 251.68 | -39.73 | 119.71 | 0.7123 | 924.7 | 999999 | |
| 0.00 | 1.42 | 0.00 | 0.99 | -13.74 | 251.56 | -39.85 | 117.73 | 0.7055 | 757.0 | 543.2 | |
| 0.00 | 0.97 | 0.00 | 0.73 | -14.03 | 246.91 | -44.49 | 115.59 | 0.7561 | -649.0 | -598.4 | |
| 0.00 | 1.24 | 0.00 | 0.95 | -15.27 | 246.37 | -45.04 | 116.82 | 0.7671 | -384.0 | -399.8 | |
| 0.00 | 1.15 | 0.00 | 0.87 | -13.96 | 246.67 | -44.73 | 115.38 | 0.7583 | -670.0 | -600.8 | |
| 0.00 | 1.33 | 0.00 | 1.02 | -15.23 | 246.16 | -45.25 | 116.66 | 0.7690 | -607.0 | -557.5 | |
| 0.00 | 1.24 | 0.00 | 0.96 | -15.52 | 245.76 | -45.64 | 116.82 | 0.7742 | -436.0 | -366.9 | |
| 0.00 | 1.42 | 0.00 | 1.10 | -15.33 | 245.68 | -45.72 | 116.55 | 0.7742 | -507.0 | -393.0 | |
| 0.00 | 1.50 | 0.00 | 1.16 | -14.06 | 245.89 | -45.51 | 115.13 | 0.7666 | -571.0 | -532.5 | |
| 0.00 | 1.77 | 0.00 | 1.37 | -14.72 | 245.67 | -45.73 | 115.82 | 0.7716 | -715.0 | -659.4 | |
| 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. | |