SDO HMI 2014-11-04 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.15 | 29.11 | 5.11 | 16.12 | -16.57 | 101.67 | 16.39 | 217.37 | 0.4466 | 223.6 | 71.1 | |
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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 |
| 1.90 | 5.70 | 1.05 | 3.16 | -15.05 | 104.09 | 18.81 | 223.96 | 0.4506 | -927.5 | -748.3 | |
| 4.92 | 7.43 | 2.76 | 4.16 | -16.78 | 104.09 | 18.82 | 221.30 | 0.4699 | 902.3 | 678.5 | |
| 2.33 | 4.15 | 1.30 | 2.32 | -16.50 | 104.00 | 18.72 | 221.58 | 0.4657 | 997.9 | 789.2 | |
| 0.00 | 1.55 | 0.00 | 0.86 | -16.41 | 101.74 | 16.47 | 218.15 | 0.4422 | 745.0 | 464.0 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -16.77 | 100.87 | 15.60 | 216.14 | 0.4384 | 898.0 | 744.4 | |
| 0.00 | 2.16 | 0.00 | 1.19 | -16.71 | 100.67 | 15.40 | 215.89 | 0.4357 | 802.0 | 717.8 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -17.59 | 100.36 | 15.09 | 214.13 | 0.4440 | 728.0 | 589.6 | |
| 0.00 | 1.47 | 0.00 | 0.79 | -17.21 | 95.13 | 9.86 | 204.36 | 0.3982 | -815.0 | -752.4 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -17.75 | 94.50 | 9.22 | 202.42 | 0.4020 | -816.0 | -735.9 | |
| 0.00 | 1.38 | 0.00 | 0.75 | -17.77 | 93.61 | 8.34 | 200.44 | 0.3971 | -868.0 | -667.1 | |
| 0.00 | 1.38 | 0.00 | 0.75 | -18.19 | 93.51 | 8.23 | 199.83 | 0.4027 | -556.0 | -556.6 | |
| 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. | |