SDO HMI 2011-02-13 07:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.48 | 28.77 | 3.12 | 16.17 | -20.08 | 70.22 | 25.44 | 238.74 | 0.4725 | 172.8 | 169.3 | |
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back to the solar disc SDO HMI 2011-02-13 07:58:57 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 | 2.66 | 0.00 | 1.52 | -20.10 | 72.62 | 27.84 | 240.92 | 0.5038 | 819.0 | 642.0 | |
| 0.00 | 2.74 | 0.00 | 1.57 | -20.38 | 72.57 | 27.78 | 240.37 | 0.5047 | 824.0 | 614.6 | |
| 4.37 | 7.37 | 2.49 | 4.20 | -20.09 | 72.26 | 27.48 | 240.68 | 0.4990 | 934.7 | 671.4 | |
| 0.00 | 1.37 | 0.00 | 0.78 | -19.46 | 72.07 | 27.29 | 241.73 | 0.4928 | 810.0 | 705.0 | |
| 1.11 | 1.80 | 0.63 | 1.02 | -20.08 | 71.87 | 27.08 | 240.41 | 0.4938 | 898.5 | 825.1 | |
| 0.00 | 1.80 | 0.00 | 1.02 | -20.33 | 71.74 | 26.95 | 239.84 | 0.4936 | 862.0 | 667.3 | |
| 0.00 | 1.28 | 0.00 | 0.72 | -19.15 | 71.03 | 26.25 | 241.56 | 0.4771 | 869.0 | 700.7 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -20.03 | 70.98 | 26.19 | 239.81 | 0.4818 | 562.0 | 439.9 | |
| 0.00 | 1.88 | 0.00 | 1.05 | -19.43 | 69.00 | 24.21 | 239.33 | 0.4516 | -741.0 | -484.5 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -19.35 | 68.75 | 23.96 | 239.27 | 0.4476 | -886.0 | -760.6 | |
| 0.00 | 1.11 | 0.00 | 0.60 | -20.16 | 64.69 | 19.90 | 233.25 | 0.4006 | -994.0 | -752.2 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -20.23 | 64.50 | 19.71 | 232.87 | 0.3987 | -862.0 | -717.2 | |
| 0.00 | 1.54 | 0.00 | 0.83 | -20.73 | 63.39 | 18.61 | 230.34 | 0.3893 | -766.0 | -678.2 | |
| 0.00 | 1.71 | 0.00 | 0.92 | -21.15 | 62.58 | 17.79 | 228.28 | 0.3835 | -778.0 | -659.0 | |
| 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. | |