SDO HMI 2011-12-07 16:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.11 | 19.42 | 3.19 | 11.97 | 8.39 | 42.24 | -35.59 | 75.88 | 0.5959 | 2.0 | -19.2 | |
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back to the solar disc SDO HMI 2011-12-07 16:58:56 UT
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 | 0.51 | 0.00 | 0.31 | 8.54 | 44.13 | -33.70 | 74.99 | 0.5703 | -767.0 | -717.3 | |
| 0.00 | 1.19 | 0.00 | 0.72 | 8.66 | 43.97 | -33.85 | 74.84 | 0.5728 | -716.0 | -552.8 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 9.29 | 43.73 | -34.10 | 73.87 | 0.5782 | -709.0 | -611.0 | |
| 0.00 | 0.68 | 0.00 | 0.41 | 8.21 | 43.66 | -34.17 | 75.72 | 0.5758 | -721.0 | -523.8 | |
| 0.00 | 2.73 | 0.00 | 1.65 | 7.88 | 43.55 | -34.28 | 76.32 | 0.5765 | -920.0 | -765.2 | |
| 0.00 | 1.02 | 0.00 | 0.63 | 10.13 | 42.86 | -34.97 | 72.81 | 0.5928 | 620.0 | 504.2 | |
| 0.00 | 1.02 | 0.00 | 0.63 | 10.55 | 42.81 | -35.02 | 72.15 | 0.5950 | -631.0 | -492.8 | |
| 0.51 | 2.98 | 0.31 | 1.83 | 7.73 | 42.32 | -35.51 | 76.96 | 0.5930 | 833.0 | 702.7 | |
| 0.00 | 1.62 | 0.00 | 1.00 | 7.62 | 41.97 | -35.86 | 77.27 | 0.5976 | 720.0 | 444.6 | |
| 1.36 | 2.64 | 0.85 | 1.65 | 8.03 | 41.00 | -36.83 | 76.87 | 0.6118 | 615.6 | 541.3 | |
| 3.24 | 4.09 | 2.03 | 2.57 | 8.51 | 40.68 | -37.15 | 76.20 | 0.6173 | 755.6 | 612.1 | |
| 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. | |