SDO HMI 2011-03-03 03:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.91 | 0.00 | 11.55 | 18.38 | 175.31 | 5.40 | 348.62 | 0.4447 | -463.2 | -432.9 | |
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back to the solar disc SDO HMI 2011-03-03 03:58:59 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 | 1.12 | 0.00 | 0.62 | 18.11 | 178.56 | 8.65 | 341.49 | 0.4521 | -796.0 | -642.8 | |
| 0.00 | 2.94 | 0.00 | 1.64 | 18.89 | 177.80 | 7.90 | 343.52 | 0.4601 | -859.0 | -705.9 | |
| 0.00 | 1.90 | 0.00 | 1.06 | 19.11 | 177.21 | 7.30 | 344.83 | 0.4609 | -883.0 | -717.3 | |
| 0.00 | 1.30 | 0.00 | 0.72 | 19.34 | 177.13 | 7.22 | 345.13 | 0.4640 | -725.0 | -583.7 | |
| 0.00 | 2.07 | 0.00 | 1.15 | 18.84 | 176.79 | 6.88 | 345.51 | 0.4551 | -933.0 | -743.2 | |
| 0.00 | 2.68 | 0.00 | 1.49 | 18.92 | 176.00 | 6.09 | 347.15 | 0.4536 | -820.0 | -630.8 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 18.59 | 175.83 | 5.92 | 347.33 | 0.4479 | -815.0 | -730.9 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 18.76 | 175.81 | 5.90 | 347.47 | 0.4504 | -783.0 | -633.9 | |
| 0.00 | 1.30 | 0.00 | 0.72 | 18.94 | 174.33 | 4.42 | 350.61 | 0.4488 | -744.0 | -645.7 | |
| 0.00 | 1.73 | 0.00 | 0.95 | 18.61 | 174.23 | 4.32 | 350.70 | 0.4434 | -864.0 | -645.5 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 16.03 | 171.10 | 1.19 | 357.10 | 0.3974 | 642.0 | 526.9 | |
| 0.00 | 1.90 | 0.00 | 1.03 | 16.39 | 170.11 | 0.21 | 359.51 | 0.4027 | 824.0 | 696.9 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 16.39 | 169.90 | -0.01 | 0.03 | 0.4027 | 735.0 | 550.3 | |
| 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. | |