SDO HMI 2014-04-10 20:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.68 | 18.06 | 0.89 | 9.39 | -13.91 | 300.34 | -13.85 | 122.73 | 0.2833 | -12.0 | -0.5 | |
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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 | 0.79 | 0.00 | 0.39 | -10.59 | 313.38 | -0.80 | 170.34 | 0.0825 | 910.0 | 781.1 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -14.88 | 311.53 | -2.66 | 163.92 | 0.1624 | 802.0 | 552.5 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -17.51 | 308.81 | -5.38 | 156.01 | 0.2208 | 837.0 | 617.6 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -11.53 | 306.86 | -7.32 | 128.16 | 0.1595 | 715.0 | 552.4 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -24.53 | 305.44 | -8.74 | 156.62 | 0.3499 | -9.0 | -10.0 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -5.62 | 305.89 | -8.30 | 88.17 | 0.1443 | 821.0 | 577.1 | |
| 0.00 | 2.56 | 0.00 | 1.28 | -6.58 | 305.84 | -8.34 | 94.83 | 0.1453 | 901.0 | 706.5 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -17.07 | 297.57 | -16.61 | 125.78 | 0.3384 | -842.0 | -616.7 | |
| 1.68 | 1.68 | 0.89 | 0.89 | -16.57 | 296.41 | -17.78 | 122.87 | 0.3500 | -792.4 | 0.0 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -14.11 | 296.59 | -17.59 | 116.58 | 0.3292 | -865.0 | -739.2 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -16.84 | 296.12 | -18.07 | 123.14 | 0.3561 | -807.0 | -683.2 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -14.34 | 296.28 | -17.91 | 116.86 | 0.3354 | -399.0 | -495.9 | |
| 0.00 | 1.76 | 0.00 | 0.95 | -17.44 | 293.15 | -21.04 | 121.01 | 0.4013 | -767.0 | -580.8 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -8.06 | 293.77 | -20.42 | 97.16 | 0.3497 | -2.0 | -16.6 | |
| 0.00 | 1.76 | 0.00 | 0.97 | -19.94 | 291.54 | -22.65 | 124.56 | 0.4414 | -769.0 | -627.0 | |
| 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. | |