SDO HMI 2014-11-07 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.19 | 19.34 | 2.13 | 12.80 | -16.12 | 16.54 | -36.87 | 119.61 | 0.6646 | -406.3 | -389.7 | |
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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 | 0.60 | 0.00 | 0.36 | -13.95 | 24.04 | -29.36 | 121.86 | 0.5624 | 589.0 | 480.3 | |
| 0.00 | 0.95 | 0.00 | 0.57 | -13.51 | 24.04 | -29.37 | 121.17 | 0.5595 | 704.0 | 571.4 | |
| 0.00 | 1.38 | 0.00 | 0.89 | -14.66 | 17.96 | -35.45 | 118.45 | 0.6404 | 496.0 | 404.7 | |
| 0.00 | 1.12 | 0.00 | 0.75 | -17.16 | 16.23 | -37.17 | 120.79 | 0.6743 | -724.0 | -613.8 | |
| 0.00 | 1.30 | 0.00 | 0.86 | -16.49 | 16.31 | -37.09 | 119.94 | 0.6697 | -822.0 | -698.9 | |
| 0.00 | 3.11 | 0.00 | 2.07 | -16.56 | 16.10 | -37.30 | 119.91 | 0.6725 | -762.0 | -620.0 | |
| 0.00 | 0.78 | 0.00 | 0.52 | -17.14 | 15.85 | -37.56 | 120.53 | 0.6785 | -627.0 | -494.4 | |
| 3.19 | 5.87 | 2.13 | 3.91 | -16.15 | 16.04 | -37.37 | 119.32 | 0.6709 | -903.5 | -694.1 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -16.17 | 15.64 | -37.76 | 119.10 | 0.6755 | -735.0 | -550.9 | |
| 0.00 | 0.60 | 0.00 | 0.41 | -15.90 | 15.15 | -38.25 | 118.46 | 0.6796 | -653.0 | -600.0 | |
| 0.00 | 0.95 | 0.00 | 0.66 | -18.86 | 14.40 | -39.00 | 121.89 | 0.7037 | -401.0 | -376.9 | |
| 0.00 | 0.78 | 0.00 | 0.54 | -18.77 | 14.22 | -39.18 | 121.67 | 0.7051 | -354.0 | -248.9 | |
| 0.00 | 1.21 | 0.00 | 0.80 | -13.30 | 15.34 | -38.06 | 114.99 | 0.6643 | -528.0 | -364.6 | |
| 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. | |