SDO HMI 2014-10-07 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.14 | 142.07 | 14.09 | 82.84 | -14.19 | 122.18 | 24.30 | 229.26 | 0.5281 | 333.3 | 171.9 | |
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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 | 0.88 | 0.00 | 0.53 | -16.45 | 124.49 | 26.61 | 228.76 | 0.5735 | -745.0 | -559.0 | |
| 18.60 | 103.89 | 10.92 | 61.04 | -13.98 | 123.36 | 25.48 | 231.06 | 0.5389 | 1103.0 | 362.3 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -12.78 | 122.82 | 24.94 | 232.29 | 0.5219 | 668.0 | 549.6 | |
| 2.11 | 6.05 | 1.24 | 3.57 | -15.02 | 123.05 | 25.17 | 229.19 | 0.5447 | 855.0 | 672.6 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -14.48 | 122.54 | 24.66 | 229.40 | 0.5341 | 815.0 | 663.1 | |
| 0.53 | 2.46 | 0.31 | 1.43 | -14.60 | 122.24 | 24.36 | 228.90 | 0.5319 | 993.5 | 780.4 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -14.41 | 120.94 | 23.05 | 227.62 | 0.5156 | 670.0 | 546.3 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -15.32 | 118.36 | 20.48 | 222.92 | 0.4975 | -762.0 | -619.3 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -15.12 | 118.27 | 20.39 | 223.08 | 0.4945 | -817.0 | -674.4 | |
| 0.00 | 4.56 | 0.00 | 2.60 | -16.12 | 117.45 | 19.57 | 220.52 | 0.4972 | -950.0 | -702.6 | |
| 0.00 | 1.32 | 0.00 | 0.75 | -15.95 | 117.23 | 19.35 | 220.44 | 0.4931 | -866.0 | -742.8 | |
| 0.00 | 1.67 | 0.00 | 0.95 | -15.69 | 117.17 | 19.29 | 220.72 | 0.4896 | -700.0 | -542.8 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -13.31 | 116.93 | 19.05 | 223.83 | 0.4605 | -921.0 | -831.8 | |
| 2.90 | 9.04 | 1.62 | 5.05 | -13.69 | 116.79 | 18.91 | 223.05 | 0.4633 | -894.7 | -828.3 | |
| 0.00 | 5.70 | 0.00 | 3.20 | -15.04 | 116.16 | 18.28 | 220.11 | 0.4721 | -652.0 | -720.5 | |
| 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. | |