SDO HMI 2011-11-25 05:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.10 | 136.08 | 16.40 | 100.09 | -24.11 | 283.18 | 41.18 | 234.46 | 0.7405 | 494.7 | 207.5 | |
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back to the solar disc SDO HMI 2011-11-25 05:58:57 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 | 1.03 | 0.00 | 0.81 | -26.10 | 286.57 | 44.57 | 233.98 | 0.7815 | 626.0 | 455.4 | |
| 22.10 | 115.88 | 16.40 | 86.08 | -23.96 | 283.96 | 41.96 | 235.14 | 0.7469 | 970.9 | 273.0 | |
| 0.00 | 1.28 | 0.00 | 0.92 | -21.89 | 282.67 | 40.67 | 236.98 | 0.7235 | 468.0 | 379.7 | |
| 0.00 | 1.20 | 0.00 | 0.84 | -21.45 | 281.81 | 39.81 | 237.05 | 0.7125 | 523.0 | 460.1 | |
| 0.00 | 2.23 | 0.00 | 1.56 | -21.58 | 281.56 | 39.56 | 236.75 | 0.7105 | 619.0 | 551.8 | |
| 0.00 | 1.28 | 0.00 | 0.90 | -22.34 | 281.07 | 39.07 | 235.50 | 0.7097 | 570.0 | 447.8 | |
| 0.00 | 1.11 | 0.00 | 0.81 | -26.92 | 281.01 | 39.02 | 229.90 | 0.7361 | 588.0 | 423.8 | |
| 0.00 | 1.71 | 0.00 | 1.15 | -23.89 | 277.08 | 35.08 | 230.94 | 0.6791 | -669.0 | -454.7 | |
| 0.00 | 0.94 | 0.00 | 0.63 | -23.82 | 276.62 | 34.62 | 230.70 | 0.6741 | -718.0 | -534.3 | |
| 0.00 | 1.54 | 0.00 | 1.05 | -26.56 | 276.00 | 34.00 | 226.88 | 0.6876 | -646.0 | -533.7 | |
| 0.00 | 1.54 | 0.00 | 1.05 | -26.86 | 275.62 | 33.62 | 226.24 | 0.6863 | -694.0 | -564.4 | |
| 0.00 | 1.80 | 0.00 | 1.23 | -27.16 | 275.64 | 33.64 | 225.90 | 0.6888 | -623.0 | -472.5 | |
| 0.00 | 1.37 | 0.00 | 0.93 | -26.92 | 275.24 | 33.24 | 225.88 | 0.6833 | -877.0 | -763.9 | |
| 0.00 | 3.17 | 0.00 | 2.13 | -27.75 | 274.17 | 32.17 | 224.06 | 0.6800 | -547.0 | -501.7 | |
| 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. | |