SDO HMI 2011-12-12 23:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.15 | 15.92 | 2.01 | 10.00 | 7.75 | 45.20 | 37.13 | 283.46 | 0.6169 | -304.6 | -190.6 | |
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back to the solar disc SDO HMI 2011-12-12 23:58:55 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 | 0.55 | 7.55 | 47.46 | 39.38 | 282.48 | 0.6465 | -602.0 | -512.1 | |
| 0.00 | 1.62 | 0.00 | 1.04 | 8.15 | 47.02 | 38.95 | 283.52 | 0.6423 | -578.0 | -468.7 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 8.44 | 46.71 | 38.64 | 284.06 | 0.6390 | -729.0 | -594.2 | |
| 2.13 | 2.89 | 1.36 | 1.85 | 7.82 | 46.60 | 38.53 | 283.13 | 0.6360 | -739.7 | -700.6 | |
| 1.02 | 1.36 | 0.65 | 0.86 | 7.63 | 45.67 | 37.60 | 283.11 | 0.6232 | -804.0 | -736.0 | |
| 0.00 | 1.96 | 0.00 | 1.23 | 7.63 | 45.33 | 37.26 | 283.20 | 0.6186 | -892.0 | -672.3 | |
| 0.00 | 1.28 | 0.00 | 0.80 | 7.84 | 45.36 | 37.28 | 283.53 | 0.6195 | -772.0 | -646.1 | |
| 0.00 | 0.68 | 0.00 | 0.42 | 7.89 | 44.47 | 36.39 | 283.90 | 0.6077 | -524.0 | -427.2 | |
| 0.00 | 2.13 | 0.00 | 1.31 | 7.53 | 43.36 | 35.29 | 283.66 | 0.5916 | 834.0 | 664.0 | |
| 0.00 | 1.19 | 0.00 | 0.73 | 7.49 | 42.78 | 34.70 | 283.81 | 0.5835 | 656.0 | 528.1 | |
| 0.00 | 1.02 | 0.00 | 0.61 | 7.36 | 40.55 | 32.47 | 284.39 | 0.5519 | 782.0 | 634.7 | |
| 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. | |