SDO HMI 2014-11-08 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.97 | 0.00 | 10.40 | -14.79 | 18.02 | -24.93 | 128.09 | 0.5133 | -157.5 | -206.2 | |
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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 |
| 0.00 | 1.73 | 0.00 | 0.91 | -11.21 | 28.92 | -14.03 | 136.98 | 0.3502 | 6.0 | -0.6 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -10.51 | 28.24 | -14.72 | 134.21 | 0.3500 | 22.0 | 26.0 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -14.50 | 23.08 | -19.88 | 133.11 | 0.4529 | 803.0 | 593.5 | |
| 0.00 | 1.04 | 0.00 | 0.57 | -11.99 | 21.57 | -21.38 | 126.68 | 0.4466 | 687.0 | 565.2 | |
| 0.00 | 4.06 | 0.00 | 2.28 | -13.78 | 20.78 | -22.17 | 128.85 | 0.4726 | 909.0 | 502.3 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -14.01 | 20.13 | -22.83 | 128.45 | 0.4826 | -899.0 | -783.8 | |
| 0.00 | 0.35 | 0.00 | 0.20 | -17.37 | 18.08 | -24.87 | 131.35 | 0.5369 | -678.0 | -734.5 | |
| 0.00 | 4.23 | 0.00 | 2.50 | -16.19 | 15.94 | -27.01 | 127.37 | 0.5509 | -769.0 | -811.3 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -16.49 | 15.51 | -27.44 | 127.39 | 0.5583 | -632.0 | -598.4 | |
| 0.00 | 1.64 | 0.00 | 1.05 | -16.65 | 8.76 | -34.20 | 122.01 | 0.6374 | -505.0 | -385.5 | |
| 0.00 | 1.29 | 0.00 | 0.83 | -16.50 | 8.64 | -34.32 | 121.72 | 0.6378 | -676.0 | -597.3 | |
| 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. | |