SDO HMI 2014-11-01 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 |
| 7.71 | 27.02 | 4.89 | 17.37 | -16.20 | 101.13 | -34.13 | 122.25 | 0.6386 | 416.2 | 399.1 | |
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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 | 0.78 | 0.00 | 0.49 | -16.39 | 102.38 | -32.88 | 123.38 | 0.6260 | 735.0 | 626.6 | |
| 3.03 | 4.33 | 1.92 | 2.74 | -16.14 | 102.28 | -32.98 | 122.96 | 0.6255 | 931.0 | 732.8 | |
| 0.00 | 2.68 | 0.00 | 1.70 | -15.85 | 102.33 | -32.92 | 122.60 | 0.6229 | 959.0 | 831.8 | |
| 0.00 | 1.21 | 0.00 | 0.77 | -16.49 | 102.17 | -33.08 | 123.37 | 0.6290 | 714.0 | 643.1 | |
| 4.68 | 11.26 | 2.97 | 7.16 | -16.06 | 101.89 | -33.37 | 122.56 | 0.6294 | 847.1 | 576.1 | |
| 0.00 | 1.91 | 0.00 | 1.22 | -16.10 | 101.66 | -33.60 | 122.44 | 0.6323 | 428.0 | 414.8 | |
| 0.00 | 0.78 | 0.00 | 0.50 | -15.71 | 101.21 | -34.05 | 121.57 | 0.6349 | 450.0 | 308.9 | |
| 0.00 | 1.21 | 0.00 | 0.79 | -15.38 | 99.42 | -35.83 | 119.89 | 0.6534 | 216.0 | 327.1 | |
| 0.00 | 1.21 | 0.00 | 0.82 | -15.59 | 96.97 | -38.29 | 118.65 | 0.6824 | -728.0 | -602.0 | |
| 0.00 | 0.87 | 0.00 | 0.62 | -18.73 | 94.67 | -40.59 | 121.35 | 0.7239 | -701.0 | -605.3 | |
| 0.00 | 0.78 | 0.00 | 0.56 | -18.64 | 94.03 | -41.23 | 120.87 | 0.7300 | -595.0 | -531.7 | |
| 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. | |