SDO HMI 2011-04-27 23:59:06 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.23 | 21.74 | 1.29 | 12.54 | 15.75 | 176.94 | 23.59 | 311.47 | 0.5162 | -32.5 | -87.7 | |
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back to the solar disc SDO HMI 2011-04-27 23:59:06 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 | 1.60 | 0.00 | 0.94 | 15.60 | 178.41 | 25.06 | 309.55 | 0.5311 | -733.0 | -595.3 | |
| 0.00 | 1.16 | 0.00 | 0.67 | 15.44 | 178.35 | 25.00 | 309.36 | 0.5290 | -590.0 | -342.2 | |
| 2.23 | 7.03 | 1.29 | 4.07 | 15.10 | 177.79 | 24.44 | 309.47 | 0.5195 | -782.3 | -670.0 | |
| 0.00 | 1.34 | 0.00 | 0.77 | 15.04 | 177.20 | 23.85 | 310.06 | 0.5123 | -852.0 | -599.1 | |
| 0.00 | 1.25 | 0.00 | 0.72 | 15.26 | 176.96 | 23.61 | 310.68 | 0.5115 | -650.0 | -553.9 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 15.95 | 176.36 | 23.01 | 312.44 | 0.5113 | -554.0 | -388.0 | |
| 0.00 | 1.69 | 0.00 | 0.98 | 16.85 | 176.23 | 22.88 | 313.93 | 0.5187 | 506.0 | 445.8 | |
| 0.00 | 1.16 | 0.00 | 0.67 | 16.94 | 176.03 | 22.69 | 314.30 | 0.5175 | 456.0 | 517.5 | |
| 0.00 | 2.05 | 0.00 | 1.18 | 16.84 | 175.92 | 22.57 | 314.29 | 0.5153 | 816.0 | 657.2 | |
| 0.00 | 1.07 | 0.00 | 0.61 | 15.95 | 175.51 | 22.16 | 313.51 | 0.5019 | 742.0 | 567.9 | |
| 0.00 | 1.16 | 0.00 | 0.66 | 16.15 | 175.53 | 22.18 | 313.77 | 0.5041 | 611.0 | 525.3 | |
| 0.00 | 1.25 | 0.00 | 0.71 | 16.10 | 175.05 | 21.70 | 314.31 | 0.4984 | 858.0 | 683.6 | |
| 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. | |