SDO HMI 2014-11-04 04:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.55 | 42.02 | 5.57 | 22.51 | 5.64 | 71.80 | -22.25 | 84.97 | 0.3796 | -400.1 | -330.2 | |
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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 |
| 3.11 | 25.51 | 1.64 | 13.48 | 5.81 | 73.76 | -20.29 | 84.26 | 0.3483 | -1253.2 | -750.1 | |
| 4.41 | -1.00 | 2.33 | -1.00 | 5.90 | 73.60 | -20.45 | 84.05 | 0.3510 | -981.4 | 999999 | |
| 3.03 | -1.00 | 1.60 | -1.00 | 5.69 | 73.57 | -20.48 | 84.65 | 0.3512 | -1061.2 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.01 | 5.15 | 73.40 | -20.65 | 86.21 | 0.3536 | -835.0 | -646.1 | |
| 0.00 | 1.82 | 0.00 | 0.96 | 5.46 | 72.88 | -21.17 | 85.39 | 0.3623 | -797.0 | -551.8 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 3.39 | 71.98 | -22.08 | 91.04 | 0.3769 | -805.0 | -666.4 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 6.86 | 71.56 | -22.49 | 81.92 | 0.3852 | -698.0 | -525.3 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 5.40 | 70.59 | -23.46 | 85.81 | 0.3992 | -663.0 | -487.0 | |
| 0.00 | 1.47 | 0.00 | 0.80 | 5.88 | 69.49 | -24.57 | 84.77 | 0.4171 | -729.0 | -548.2 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 6.03 | 67.39 | -26.66 | 84.68 | 0.4501 | 757.0 | 603.5 | |
| 0.00 | 1.38 | 0.00 | 0.77 | 5.69 | 66.94 | -27.12 | 85.48 | 0.4569 | 884.0 | 793.6 | |
| 0.00 | 1.47 | 0.00 | 0.82 | 4.65 | 66.34 | -27.71 | 87.75 | 0.4657 | 920.0 | 806.3 | |
| 0.00 | 2.42 | 0.00 | 1.36 | 4.53 | 66.18 | -27.87 | 88.02 | 0.4683 | 890.0 | 729.2 | |
| 0.00 | 1.30 | 0.00 | 0.73 | 5.04 | 66.16 | -27.89 | 86.93 | 0.4686 | 756.0 | 603.7 | |
| 0.00 | 0.69 | 0.00 | 0.39 | 9.28 | 65.60 | -28.45 | 78.08 | 0.4825 | -669.0 | -467.5 | |
| 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. | |