SDO HMI 2011-06-13 06:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.63 | 24.29 | 0.88 | 12.97 | -15.05 | 245.99 | -15.06 | 137.59 | 0.3723 | 403.3 | 359.4 | |
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back to the solar disc SDO HMI 2011-06-13 06:59:11 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 | 1.72 | 0.00 | 0.90 | -14.96 | 250.44 | -10.61 | 146.73 | 0.3255 | 437.0 | 438.5 | |
| 0.00 | 1.00 | 0.00 | 0.52 | -13.64 | 248.65 | -12.40 | 140.00 | 0.3260 | 761.0 | 576.8 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -14.33 | 248.45 | -12.60 | 140.94 | 0.3367 | 566.0 | 519.3 | |
| 0.00 | 0.73 | 0.00 | 0.38 | -14.68 | 247.68 | -13.36 | 139.98 | 0.3491 | 862.0 | 699.6 | |
| 0.00 | 2.08 | 0.00 | 1.11 | -15.67 | 247.36 | -13.68 | 141.14 | 0.3646 | 934.0 | 699.2 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -15.32 | 247.32 | -13.72 | 140.42 | 0.3607 | 818.0 | 611.1 | |
| 0.00 | 1.72 | 0.00 | 0.92 | -15.48 | 247.18 | -13.87 | 140.43 | 0.3641 | 801.0 | 705.7 | |
| 0.00 | 2.90 | 0.00 | 1.55 | -14.76 | 245.66 | -15.38 | 136.18 | 0.3720 | 995.0 | 860.5 | |
| 0.00 | 3.54 | 0.00 | 1.89 | -14.69 | 245.37 | -15.67 | 135.54 | 0.3746 | 921.0 | 750.6 | |
| 0.00 | 1.72 | 0.00 | 0.92 | -14.92 | 244.83 | -16.21 | 135.02 | 0.3832 | 686.0 | 438.6 | |
| 0.45 | 5.53 | 0.24 | 2.99 | -15.27 | 243.68 | -17.36 | 133.78 | 0.4003 | -1118.4 | -873.5 | |
| 1.18 | -11.00 | 0.64 | -11.00 | -15.27 | 243.55 | -17.49 | 133.57 | 0.4018 | -951.8 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -17.19 | 241.35 | -19.69 | 133.71 | 0.4471 | -591.0 | -481.9 | |
| 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. | |