SDO HMI 2013-01-07 09:58:54 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.33 | 282.85 | 25.29 | 151.14 | -24.38 | 250.35 | 7.78 | 199.19 | 0.3758 | 840.1 | 362.8 | |
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back to the solar disc SDO HMI 2013-01-07 09:58:54 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 |
| 47.33 | 272.17 | 25.29 | 145.49 | -24.40 | 250.60 | 8.03 | 199.81 | 0.3769 | 1453.2 | 409.0 | |
| 0.00 | 0.76 | 0.00 | 0.41 | -26.87 | 247.44 | 4.87 | 190.91 | 0.4015 | 804.0 | 584.9 | |
| 0.00 | 0.68 | 0.00 | 0.36 | -23.77 | 245.93 | 3.36 | 188.91 | 0.3478 | -836.0 | -719.5 | |
| 0.00 | 0.93 | 0.00 | 0.49 | -23.49 | 245.57 | 3.00 | 188.09 | 0.3424 | -925.0 | -663.2 | |
| 0.00 | 1.44 | 0.00 | 0.77 | -24.84 | 245.41 | 2.83 | 187.11 | 0.3640 | -841.0 | -695.7 | |
| 0.00 | 1.87 | 0.00 | 0.98 | -23.14 | 244.38 | 1.80 | 184.99 | 0.3345 | -1010.0 | -812.9 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -22.55 | 244.24 | 1.67 | 184.78 | 0.3246 | -887.0 | -745.2 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -25.16 | 242.35 | -0.22 | 179.45 | 0.3663 | -888.0 | -678.8 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -26.01 | 241.30 | -1.27 | 176.98 | 0.3807 | -887.0 | -695.3 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -20.84 | 240.69 | -1.88 | 174.04 | 0.2965 | -916.0 | -700.6 | |
| 0.00 | 0.25 | 0.00 | 0.13 | -21.58 | 240.49 | -2.08 | 173.70 | 0.3092 | -719.0 | -542.0 | |
| 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. | |