SDO HMI 2011-12-08 06:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.28 | 35.63 | 9.25 | 20.21 | 8.69 | 42.23 | -27.90 | 71.95 | 0.4892 | 245.7 | 59.4 | |
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back to the solar disc SDO HMI 2011-12-08 06:58:56 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 | 0.85 | 0.00 | 0.47 | 9.48 | 44.88 | -25.25 | 68.62 | 0.4537 | -733.0 | -558.7 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 8.94 | 44.32 | -25.81 | 70.13 | 0.4592 | -894.0 | -777.3 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 8.19 | 44.15 | -25.98 | 71.81 | 0.4584 | -823.0 | -702.8 | |
| 0.00 | 1.53 | 0.00 | 0.85 | 8.01 | 44.06 | -26.07 | 72.23 | 0.4589 | -821.0 | -570.6 | |
| 0.00 | 1.19 | 0.00 | 0.67 | 7.78 | 43.94 | -26.19 | 72.80 | 0.4596 | -803.0 | -715.2 | |
| 1.36 | 2.56 | 0.76 | 1.43 | 7.92 | 43.80 | -26.33 | 72.57 | 0.4624 | -688.8 | -626.8 | |
| 0.00 | 1.71 | 0.00 | 0.97 | 11.04 | 42.35 | -27.78 | 67.28 | 0.4979 | -680.0 | -602.2 | |
| 0.00 | 4.01 | 0.00 | 2.31 | 13.12 | 41.84 | -28.29 | 63.80 | 0.5165 | 778.0 | 461.4 | |
| 2.30 | 4.26 | 1.30 | 2.41 | 7.84 | 42.33 | -27.80 | 73.56 | 0.4837 | 1018.4 | 800.0 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 7.84 | 42.06 | -28.07 | 73.70 | 0.4877 | 733.0 | 649.8 | |
| 12.62 | 16.71 | 7.19 | 9.53 | 7.84 | 41.42 | -28.71 | 74.01 | 0.4971 | 929.2 | 611.1 | |
| 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. | |