SDO HMI 2014-10-03 02:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.96 | 0.00 | 14.90 | -5.19 | 139.38 | -17.86 | 123.65 | 0.3672 | -675.3 | -541.2 | |
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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 |
| 0.00 | 0.88 | 0.00 | 0.45 | -4.96 | 146.25 | -10.98 | 136.36 | 0.2762 | 798.0 | 653.9 | |
| 0.00 | 2.90 | 0.00 | 1.50 | -5.31 | 145.79 | -11.45 | 136.02 | 0.2859 | 308.0 | 368.7 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -4.10 | 141.00 | -16.23 | 123.09 | 0.3342 | -841.0 | -751.4 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -4.70 | 140.20 | -17.03 | 123.28 | 0.3507 | -989.0 | -819.1 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -4.38 | 139.74 | -17.49 | 121.80 | 0.3542 | -810.0 | -560.4 | |
| 0.00 | 1.67 | 0.00 | 0.89 | -5.73 | 139.61 | -17.63 | 124.73 | 0.3682 | -1094.0 | -937.5 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -4.11 | 139.62 | -17.61 | 120.97 | 0.3535 | -929.0 | -713.4 | |
| 0.00 | 2.02 | 0.00 | 1.07 | -3.87 | 139.59 | -17.64 | 120.34 | 0.3518 | -916.0 | -814.0 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -5.52 | 139.55 | -17.68 | 124.16 | 0.3670 | -934.0 | -748.8 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -6.27 | 139.27 | -17.96 | 125.39 | 0.3777 | -839.0 | -686.8 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -3.31 | 138.88 | -18.35 | 117.97 | 0.3575 | -726.0 | -630.9 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -6.07 | 138.70 | -18.53 | 124.12 | 0.3833 | -665.0 | -634.4 | |
| 0.00 | 2.73 | 0.00 | 1.47 | -6.40 | 138.28 | -18.96 | 124.19 | 0.3920 | -767.0 | -648.1 | |
| 0.00 | 2.20 | 0.00 | 1.18 | -6.00 | 138.07 | -19.16 | 123.06 | 0.3912 | -825.0 | -600.6 | |
| 0.00 | 3.17 | 0.00 | 1.72 | -5.68 | 136.22 | -21.02 | 119.96 | 0.4136 | -723.0 | -608.5 | |
| 0.00 | 3.17 | 0.00 | 1.72 | -5.04 | 135.98 | -21.25 | 118.33 | 0.4119 | -853.0 | -646.4 | |
| 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. | |