SDO HMI 2014-11-29 03:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.17 | 37.30 | 5.97 | 21.59 | 16.98 | 152.30 | 27.26 | 302.15 | 0.5194 | 175.3 | -56.2 | |
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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 |
| 7.78 | 10.09 | 4.60 | 5.97 | 17.52 | 154.30 | 29.26 | 301.38 | 0.5481 | 890.9 | 571.2 | |
| 0.00 | 1.97 | 0.00 | 1.17 | 17.83 | 154.35 | 29.32 | 301.84 | 0.5508 | 619.0 | 473.7 | |
| 1.88 | 4.96 | 1.08 | 2.85 | 15.45 | 152.49 | 27.45 | 299.28 | 0.5115 | 818.4 | 662.6 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 15.20 | 152.35 | 27.31 | 298.96 | 0.5081 | 781.0 | 652.5 | |
| 0.00 | 1.97 | 0.00 | 1.14 | 16.52 | 152.44 | 27.40 | 301.20 | 0.5180 | 687.0 | 472.9 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 17.04 | 152.21 | 27.17 | 302.30 | 0.5187 | 606.0 | 496.2 | |
| 0.00 | 1.37 | 0.00 | 0.79 | 16.62 | 151.90 | 26.86 | 301.83 | 0.5117 | 863.0 | 694.1 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 17.36 | 151.25 | 26.22 | 303.70 | 0.5089 | -757.0 | -645.4 | |
| 0.00 | 1.63 | 0.00 | 0.93 | 17.36 | 151.15 | 26.11 | 303.80 | 0.5076 | -643.0 | -394.8 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 15.22 | 150.60 | 25.57 | 300.48 | 0.4852 | -674.0 | -474.0 | |
| 0.00 | 3.68 | 0.00 | 2.10 | 17.49 | 150.55 | 25.51 | 304.59 | 0.5011 | -783.0 | -664.9 | |
| 0.00 | 3.68 | 0.00 | 2.09 | 16.94 | 150.40 | 25.36 | 303.77 | 0.4949 | -760.0 | -671.3 | |
| 0.51 | 2.31 | 0.29 | 1.32 | 18.02 | 150.46 | 25.42 | 305.58 | 0.5040 | -822.0 | -742.5 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 17.03 | 150.21 | 25.17 | 304.12 | 0.4932 | -710.0 | -567.9 | |
| 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. | |