SDO HMI 2014-11-01 21:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.24 | 20.86 | 2.42 | 12.57 | -17.92 | 97.77 | -26.50 | 131.58 | 0.5639 | -159.2 | -13.0 | |
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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 |
| 1.38 | 10.30 | 0.79 | 5.87 | -16.34 | 102.75 | -21.53 | 134.65 | 0.4970 | 1040.5 | 758.7 | |
| 2.86 | -1.00 | 1.63 | -1.00 | -16.28 | 102.42 | -21.85 | 134.15 | 0.5000 | 889.3 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.35 | -15.91 | 102.33 | -21.94 | 133.46 | 0.4972 | 614.0 | 542.0 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -16.71 | 102.00 | -22.28 | 134.24 | 0.5088 | 579.0 | 461.6 | |
| 0.00 | 0.95 | 0.00 | 0.58 | -17.55 | 95.91 | -28.37 | 128.78 | 0.5833 | -677.0 | -489.4 | |
| 0.00 | 2.34 | 0.00 | 1.46 | -18.68 | 93.86 | -30.41 | 128.47 | 0.6148 | -667.0 | -651.8 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -18.61 | 93.37 | -30.91 | 127.94 | 0.6196 | -558.0 | -473.6 | |
| 0.00 | 1.04 | 0.00 | 0.65 | -17.51 | 93.44 | -30.84 | 126.51 | 0.6105 | -691.0 | -636.1 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -19.72 | 91.45 | -32.83 | 127.82 | 0.6483 | -568.0 | -605.3 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -17.01 | 91.74 | -32.54 | 124.42 | 0.6258 | -774.0 | -614.7 | |
| 0.00 | 1.04 | 0.00 | 0.66 | -17.08 | 91.43 | -32.85 | 124.29 | 0.6299 | -536.0 | -425.6 | |
| 0.00 | 1.21 | 0.00 | 0.90 | -28.49 | 87.67 | -36.61 | 135.25 | 0.7470 | -534.0 | -451.8 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -24.13 | 88.84 | -35.44 | 131.23 | 0.7060 | -596.0 | -544.0 | |
| 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. | |