SDO HMI 2014-11-03 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.58 | 0.00 | 9.76 | -20.94 | 77.85 | -20.61 | 142.62 | 0.5350 | 570.3 | 482.1 | |
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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 | 1.21 | 0.00 | 0.66 | -17.53 | 84.52 | -13.94 | 147.96 | 0.4349 | 907.0 | 805.4 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -20.80 | 83.01 | -15.45 | 149.27 | 0.4894 | 682.0 | 528.9 | |
| 0.00 | 1.81 | 0.00 | 1.03 | -20.90 | 82.87 | -15.59 | 149.16 | 0.4918 | 619.0 | 586.0 | |
| 0.00 | 0.69 | 0.00 | 0.37 | -14.51 | 83.34 | -15.12 | 141.48 | 0.4072 | 408.0 | 440.1 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -17.22 | 82.38 | -16.08 | 143.79 | 0.4497 | 783.0 | 645.0 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -26.00 | 79.66 | -18.80 | 149.83 | 0.5787 | 646.0 | 549.7 | |
| 0.00 | 2.33 | 0.00 | 1.34 | -20.31 | 79.78 | -18.68 | 143.77 | 0.5104 | 673.0 | 525.2 | |
| 0.00 | 1.21 | 0.00 | 0.70 | -20.46 | 79.08 | -19.37 | 142.98 | 0.5183 | 714.0 | 601.0 | |
| 0.00 | 2.51 | 0.00 | 1.46 | -20.35 | 78.09 | -20.37 | 141.48 | 0.5262 | 669.0 | 561.6 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -20.26 | 76.71 | -21.75 | 139.56 | 0.5382 | 566.0 | 582.0 | |
| 0.00 | 1.21 | 0.00 | 0.72 | -20.94 | 75.67 | -22.79 | 139.15 | 0.5552 | 641.0 | 512.9 | |
| 0.00 | 1.12 | 0.00 | 0.74 | -25.74 | 69.08 | -29.38 | 137.93 | 0.6619 | 562.0 | 485.8 | |
| 0.00 | 1.30 | 0.00 | 0.88 | -23.25 | 64.40 | -34.06 | 131.07 | 0.6850 | -456.0 | -367.1 | |
| 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. | |