SDO HMI 2014-10-03 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.21 | 32.17 | 3.75 | 16.87 | -11.11 | 139.72 | -7.08 | 158.29 | 0.3280 | 385.7 | 389.3 | |
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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 | 1.32 | 0.00 | 0.69 | -11.55 | 141.78 | -5.01 | 164.61 | 0.3241 | 938.0 | 698.6 | |
| 4.31 | 16.62 | 2.24 | 8.65 | -9.96 | 140.37 | -6.42 | 158.82 | 0.3063 | 1198.5 | 766.7 | |
| 0.79 | 2.99 | 0.41 | 1.55 | -9.40 | 140.20 | -6.60 | 157.60 | 0.2987 | 1079.2 | 832.2 | |
| 2.11 | -2.00 | 1.10 | -2.00 | -9.87 | 140.13 | -6.67 | 157.98 | 0.3064 | 1049.2 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -16.15 | 139.79 | -7.01 | 163.12 | 0.4050 | 734.0 | 606.3 | |
| 0.00 | 2.20 | 0.00 | 1.16 | -12.43 | 139.79 | -7.01 | 159.88 | 0.3478 | 908.0 | 555.1 | |
| 0.00 | 0.35 | 0.00 | 0.18 | -11.48 | 139.66 | -7.14 | 158.53 | 0.3340 | 764.0 | 711.0 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -10.80 | 139.09 | -7.70 | 156.16 | 0.3272 | 653.0 | 568.6 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -15.49 | 138.81 | -7.99 | 160.35 | 0.3998 | -713.0 | -570.0 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -15.53 | 138.31 | -8.49 | 159.25 | 0.4032 | -677.0 | -565.4 | |
| 0.00 | 1.49 | 0.00 | 0.79 | -12.74 | 137.85 | -8.94 | 155.32 | 0.3646 | -794.0 | -652.9 | |
| 0.00 | 1.93 | 0.00 | 1.03 | -12.44 | 137.21 | -9.58 | 153.40 | 0.3646 | -763.0 | -523.0 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -12.34 | 135.94 | -10.86 | 150.29 | 0.3729 | -722.0 | -603.8 | |
| 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. | |