SDO HMI 2014-11-14 01:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.92 | 0.00 | 8.38 | -9.63 | 338.69 | 14.84 | 228.28 | 0.3395 | -13.7 | -47.6 | |
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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 | 1.12 | 0.00 | 0.60 | -5.39 | 345.81 | 21.96 | 249.12 | 0.4002 | 778.0 | 564.2 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -8.13 | 343.09 | 19.24 | 239.77 | 0.3792 | 809.0 | 628.2 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -7.44 | 342.99 | 19.14 | 241.28 | 0.3724 | 875.0 | 710.6 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -9.10 | 343.01 | 19.16 | 237.48 | 0.3861 | 714.0 | 536.2 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -10.03 | 342.14 | 18.29 | 234.23 | 0.3826 | 847.0 | 687.2 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -10.64 | 340.53 | 16.68 | 230.39 | 0.3679 | 897.0 | 714.2 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -10.82 | 340.48 | 16.63 | 229.91 | 0.3691 | 765.0 | 588.2 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -12.57 | 336.10 | 12.25 | 217.78 | 0.3394 | -866.0 | -752.2 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -12.84 | 336.08 | 12.23 | 217.24 | 0.3428 | -772.0 | -606.9 | |
| 0.00 | 2.67 | 0.00 | 1.38 | -8.92 | 334.97 | 11.12 | 222.85 | 0.2815 | -923.0 | -751.7 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -10.99 | 334.89 | 11.04 | 217.99 | 0.3067 | -802.0 | -684.6 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -10.83 | 334.45 | 10.60 | 217.20 | 0.3002 | -821.0 | -668.1 | |
| 0.00 | 0.69 | 0.00 | 0.35 | -8.33 | 334.13 | 10.28 | 222.08 | 0.2647 | -858.0 | -706.8 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -10.64 | 333.62 | 9.76 | 215.36 | 0.2893 | -835.0 | -626.5 | |
| 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. | |