SDO HMI 2014-11-07 11:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.76 | 17.52 | 1.78 | 10.91 | -15.89 | 18.96 | -31.71 | 123.13 | 0.6029 | -20.6 | -84.6 | |
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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 | 0.69 | 0.00 | 0.39 | -12.43 | 27.40 | -23.27 | 125.27 | 0.4746 | 547.0 | 487.6 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -14.66 | 25.48 | -25.20 | 126.90 | 0.5171 | 675.0 | 556.5 | |
| 0.00 | 1.81 | 0.00 | 1.05 | -14.47 | 25.47 | -25.21 | 126.59 | 0.5156 | 735.0 | 702.9 | |
| 0.00 | 1.55 | 0.00 | 0.90 | -13.85 | 24.32 | -26.36 | 124.41 | 0.5245 | 798.0 | 499.6 | |
| 0.00 | 0.69 | 0.00 | 0.41 | -16.70 | 23.54 | -27.13 | 128.05 | 0.5569 | 537.0 | 475.0 | |
| 0.00 | 1.12 | 0.00 | 0.71 | -18.25 | 18.70 | -31.97 | 125.95 | 0.6235 | 563.0 | 498.5 | |
| 0.00 | 1.99 | 0.00 | 1.26 | -17.29 | 17.97 | -32.70 | 124.05 | 0.6249 | -627.0 | -517.3 | |
| 0.00 | 2.68 | 0.00 | 1.72 | -16.53 | 16.26 | -34.41 | 121.74 | 0.6394 | -680.0 | -719.2 | |
| 2.76 | 4.23 | 1.78 | 2.72 | -16.19 | 15.99 | -34.68 | 121.08 | 0.6404 | -876.1 | -695.2 | |
| 0.00 | 0.43 | 0.00 | 0.28 | -16.77 | 15.60 | -35.07 | 121.63 | 0.6484 | -594.0 | -516.2 | |
| 0.00 | 1.21 | 0.00 | 0.82 | -15.29 | 11.70 | -38.97 | 117.20 | 0.6845 | -637.0 | -452.1 | |
| 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. | |