SDO HMI 2014-11-27 01:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.90 | 35.86 | 9.27 | 37.90 | -23.85 | 94.05 | -58.45 | 118.10 | 0.8854 | -62.1 | -137.4 | |
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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 | 1.88 | 0.00 | 1.90 | -24.24 | 95.81 | -56.69 | 119.03 | 0.8734 | 139.0 | 302.0 | |
| 6.68 | 11.21 | 6.85 | 11.49 | -24.35 | 95.25 | -57.24 | 118.98 | 0.8778 | 270.0 | 266.2 | |
| 0.00 | 0.86 | 0.00 | 0.89 | -24.10 | 94.70 | -57.79 | 118.55 | 0.8813 | 14.0 | 123.7 | |
| 0.00 | 1.28 | 0.00 | 1.35 | -24.11 | 94.45 | -58.04 | 118.49 | 0.8831 | 170.0 | 169.0 | |
| 0.00 | 0.34 | 0.00 | 0.36 | -24.21 | 94.19 | -58.31 | 118.53 | 0.8852 | 126.0 | 143.8 | |
| 0.00 | 2.74 | 0.00 | 2.95 | -24.78 | 93.69 | -58.80 | 119.01 | 0.8899 | -114.0 | -55.3 | |
| 0.00 | 1.03 | 0.00 | 1.07 | -23.49 | 94.58 | -57.91 | 117.84 | 0.8807 | -339.0 | -296.2 | |
| 0.00 | 0.94 | 0.00 | 1.01 | -24.62 | 93.69 | -58.80 | 118.83 | 0.8896 | -12.0 | 40.7 | |
| 0.00 | 0.77 | 0.00 | 0.80 | -23.65 | 94.41 | -58.09 | 117.98 | 0.8824 | -416.0 | -435.6 | |
| 0.00 | 1.63 | 0.00 | 1.72 | -23.66 | 94.03 | -58.46 | 117.88 | 0.8851 | -470.0 | -472.2 | |
| 0.00 | 1.63 | 0.00 | 1.72 | -23.15 | 93.71 | -58.78 | 117.24 | 0.8864 | -258.0 | -302.7 | |
| 0.00 | 0.86 | 0.00 | 0.93 | -23.49 | 93.08 | -59.41 | 117.44 | 0.8915 | -257.0 | -306.5 | |
| 0.68 | 1.88 | 0.74 | 2.02 | -22.87 | 93.22 | -59.27 | 116.80 | 0.8893 | -440.1 | -435.9 | |
| 1.54 | 5.73 | 1.68 | 6.25 | -23.17 | 92.81 | -59.68 | 117.02 | 0.8928 | -524.8 | -429.4 | |
| 0.00 | 3.08 | 0.00 | 3.44 | -23.25 | 92.03 | -60.46 | 116.92 | 0.8984 | -547.0 | -349.7 | |
| 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. | |