SDO HMI 2014-11-26 19:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.07 | 61.26 | 36.84 | 121.70 | -19.75 | 81.91 | -73.90 | 110.87 | 0.9681 | 74.6 | -94.5 | |
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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 |
| 2.74 | 30.71 | 4.67 | 54.21 | -20.03 | 84.40 | -71.40 | 111.46 | 0.9581 | 540.3 | 7.9 | |
| 8.81 | -1.00 | 15.36 | -1.00 | -19.73 | 83.93 | -71.88 | 111.08 | 0.9601 | 412.2 | 999999 | |
| 0.51 | 7.70 | 1.03 | 15.58 | -21.15 | 81.73 | -74.08 | 112.26 | 0.9702 | 95.7 | -174.4 | |
| 0.00 | 1.20 | 0.00 | 2.11 | -19.23 | 83.66 | -72.15 | 110.53 | 0.9610 | 126.0 | 109.4 | |
| 0.00 | 1.03 | 0.00 | 2.02 | -20.57 | 82.05 | -73.76 | 111.71 | 0.9687 | -24.0 | -57.2 | |
| 0.00 | 2.40 | 0.00 | 4.39 | -19.12 | 82.93 | -72.87 | 110.33 | 0.9641 | -189.0 | -165.7 | |
| 0.00 | 0.26 | 0.00 | 0.48 | -18.94 | 82.71 | -73.10 | 110.11 | 0.9650 | -330.0 | -262.7 | |
| 0.00 | 0.43 | 0.00 | 1.02 | -20.67 | 79.11 | -76.70 | 111.49 | 0.9794 | -125.0 | -66.6 | |
| 1.28 | 4.02 | 3.34 | 10.58 | -21.11 | 78.21 | -77.59 | 111.84 | 0.9824 | -21.0 | -22.5 | |
| 0.00 | 0.68 | 0.00 | 1.45 | -19.49 | 80.73 | -75.07 | 110.45 | 0.9732 | -261.0 | -238.1 | |
| 5.73 | 9.92 | 12.44 | 21.50 | -18.81 | 80.27 | -75.53 | 109.71 | 0.9747 | -348.0 | -366.7 | |
| 0.00 | 1.03 | 0.00 | 2.52 | -19.10 | 78.63 | -77.18 | 109.84 | 0.9804 | -171.0 | -143.2 | |
| 0.00 | 1.88 | 0.00 | 5.84 | -17.23 | 75.96 | -79.85 | 107.72 | 0.9877 | -233.0 | -128.8 | |
| 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. | |