SDO HMI 2014-10-02 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.03 | 0.00 | 11.06 | -4.81 | 139.01 | -29.23 | 110.73 | 0.5226 | -734.1 | -530.2 | |
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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 | 1.32 | 0.00 | 0.76 | -4.43 | 140.26 | -27.97 | 110.94 | 0.5027 | -967.0 | -840.3 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -4.54 | 139.95 | -28.28 | 110.91 | 0.5077 | -770.0 | -483.2 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -4.43 | 139.72 | -28.52 | 110.54 | 0.5104 | -767.0 | -632.4 | |
| 0.00 | 1.15 | 0.00 | 0.66 | -4.22 | 139.66 | -28.58 | 110.11 | 0.5101 | -870.0 | -723.5 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -3.76 | 139.68 | -28.56 | 109.28 | 0.5074 | -742.0 | -565.6 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -5.99 | 139.12 | -29.12 | 112.92 | 0.5275 | -860.0 | -655.4 | |
| 0.00 | 1.50 | 0.00 | 0.88 | -6.49 | 138.98 | -29.25 | 113.68 | 0.5323 | -713.0 | -583.5 | |
| 0.00 | 1.15 | 0.00 | 0.67 | -5.88 | 139.02 | -29.21 | 112.64 | 0.5281 | -878.0 | -738.7 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -5.51 | 139.04 | -29.19 | 112.00 | 0.5257 | -882.0 | -703.5 | |
| 0.00 | 3.17 | 0.00 | 1.84 | -4.11 | 138.90 | -29.33 | 109.40 | 0.5201 | -754.0 | -615.7 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -6.41 | 138.78 | -29.46 | 113.39 | 0.5345 | -694.0 | -531.6 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -6.58 | 138.53 | -29.71 | 113.49 | 0.5390 | -623.0 | -458.5 | |
| 0.00 | 3.70 | 0.00 | 2.16 | -3.88 | 137.98 | -30.26 | 108.41 | 0.5320 | -23.0 | -119.3 | |
| 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. | |