SDO HMI 2014-11-14 05:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.97 | 0.00 | 10.58 | -9.36 | 338.10 | 16.44 | 232.20 | 0.3532 | -52.1 | -196.1 | |
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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 |
| 0.00 | 1.38 | 0.00 | 0.75 | -7.58 | 343.11 | 21.45 | 243.67 | 0.4062 | 960.0 | 856.1 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -8.18 | 343.11 | 21.45 | 242.34 | 0.4105 | 703.0 | 578.8 | |
| 0.00 | 1.20 | 0.00 | 0.66 | -9.91 | 343.05 | 21.40 | 238.61 | 0.4228 | 724.0 | 590.9 | |
| 0.00 | 0.77 | 0.00 | 0.42 | -8.99 | 342.61 | 20.95 | 240.02 | 0.4095 | 721.0 | 588.3 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -10.02 | 342.16 | 20.50 | 237.31 | 0.4115 | 848.0 | 711.9 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -10.94 | 341.00 | 19.34 | 233.87 | 0.4043 | 710.0 | 606.5 | |
| 0.00 | 1.89 | 0.00 | 1.00 | -10.06 | 337.68 | 16.03 | 230.60 | 0.3533 | -780.0 | -628.0 | |
| 0.00 | 3.79 | 0.00 | 2.00 | -9.60 | 337.41 | 15.75 | 231.16 | 0.3452 | -613.0 | -619.1 | |
| 0.00 | 1.38 | 0.00 | 0.72 | -9.72 | 335.49 | 13.83 | 227.21 | 0.3224 | -833.0 | -645.7 | |
| 0.00 | 2.41 | 0.00 | 1.25 | -9.05 | 335.06 | 13.40 | 227.92 | 0.3097 | -803.0 | -662.4 | |
| 0.00 | 1.55 | 0.00 | 0.81 | -9.20 | 334.85 | 13.19 | 227.11 | 0.3088 | -735.0 | -583.6 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -8.25 | 334.41 | 12.76 | 228.52 | 0.2930 | -780.0 | -571.0 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -10.64 | 333.64 | 11.98 | 221.07 | 0.3119 | -799.0 | -532.1 | |
| 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. | |