SDO HMI 2014-01-06 11:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.08 | 0.00 | 11.78 | -17.10 | 79.11 | -38.51 | 112.70 | 0.6473 | 441.4 | 393.4 | |
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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 | 5.86 | 0.00 | 3.62 | -18.67 | 83.38 | -34.24 | 116.85 | 0.5997 | 807.0 | 652.2 | |
| 0.00 | 1.10 | 0.00 | 0.69 | -19.55 | 83.13 | -34.49 | 118.08 | 0.6071 | 622.0 | 508.8 | |
| 0.00 | 2.38 | 0.00 | 1.48 | -18.93 | 83.12 | -34.49 | 117.13 | 0.6041 | 725.0 | 563.9 | |
| 0.00 | 0.93 | 0.00 | 0.59 | -12.22 | 80.06 | -37.56 | 105.23 | 0.6198 | -491.0 | -397.5 | |
| 0.00 | 0.51 | 0.00 | 0.34 | -17.00 | 76.53 | -41.08 | 111.38 | 0.6773 | 552.0 | 555.3 | |
| 0.00 | 1.02 | 0.00 | 0.71 | -18.68 | 74.23 | -43.39 | 112.98 | 0.7092 | 606.0 | 557.7 | |
| 0.00 | 1.02 | 0.00 | 0.73 | -20.89 | 73.20 | -44.42 | 115.62 | 0.7276 | 688.0 | 588.8 | |
| 0.00 | 0.59 | 0.00 | 0.42 | -18.69 | 73.80 | -43.82 | 112.86 | 0.7142 | 443.0 | 379.1 | |
| 0.00 | 0.85 | 0.00 | 0.60 | -17.78 | 74.00 | -43.62 | 111.67 | 0.7092 | 659.0 | 549.5 | |
| 0.00 | 3.06 | 0.00 | 2.04 | -10.07 | 75.75 | -41.87 | 101.03 | 0.6719 | -142.0 | -173.0 | |
| 0.00 | 0.76 | 0.00 | 0.56 | -21.09 | 72.04 | -45.57 | 115.49 | 0.7406 | 386.0 | 302.8 | |
| 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. | |