SDO HMI 2014-11-02 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.25 | 28.30 | 1.26 | 16.56 | -17.14 | 98.17 | -23.90 | 133.47 | 0.5304 | -244.9 | 123.8 | |
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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 | 4.15 | 0.00 | 2.33 | -16.36 | 102.95 | -19.12 | 138.00 | 0.4716 | 889.0 | 835.5 | |
| 0.00 | 0.61 | 0.00 | 0.34 | -16.56 | 102.93 | -19.14 | 138.25 | 0.4739 | 460.0 | 486.7 | |
| 2.25 | 10.47 | 1.26 | 5.88 | -16.25 | 102.57 | -19.50 | 137.27 | 0.4743 | 944.0 | 747.4 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -16.75 | 99.18 | -22.89 | 133.52 | 0.5157 | 600.0 | 550.1 | |
| 0.00 | 0.69 | 0.00 | 0.41 | -17.59 | 95.91 | -26.16 | 131.02 | 0.5592 | -761.0 | -599.9 | |
| 0.00 | 1.47 | 0.00 | 0.90 | -18.72 | 93.92 | -28.15 | 130.58 | 0.5906 | -895.0 | -732.6 | |
| 0.00 | 0.78 | 0.00 | 0.47 | -17.21 | 94.01 | -28.06 | 128.56 | 0.5770 | -707.0 | -599.6 | |
| 0.00 | 0.69 | 0.00 | 0.43 | -18.86 | 93.57 | -28.50 | 130.44 | 0.5955 | -573.0 | -483.4 | |
| 0.00 | 1.38 | 0.00 | 0.84 | -16.93 | 93.91 | -28.16 | 128.07 | 0.5757 | -479.0 | -352.6 | |
| 0.00 | 1.13 | 0.00 | 0.69 | -18.67 | 93.43 | -28.64 | 130.05 | 0.5955 | -548.0 | -479.2 | |
| 0.00 | 1.38 | 0.00 | 0.84 | -17.52 | 93.42 | -28.65 | 128.45 | 0.5860 | -809.0 | -686.8 | |
| 0.00 | 1.56 | 0.00 | 0.98 | -19.59 | 91.47 | -30.61 | 129.49 | 0.6238 | -689.0 | -539.4 | |
| 0.00 | 0.61 | 0.00 | 0.37 | -17.00 | 91.79 | -30.28 | 126.26 | 0.6002 | -478.0 | -540.3 | |
| 0.00 | 1.13 | 0.00 | 0.72 | -19.58 | 90.88 | -31.19 | 128.97 | 0.6299 | -632.0 | -537.7 | |
| 0.00 | 1.30 | 0.00 | 0.81 | -16.86 | 91.31 | -30.76 | 125.65 | 0.6046 | -304.0 | -307.7 | |
| 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. | |