SDO HMI 2014-03-31 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.30 | 0.00 | 8.80 | -26.36 | 87.07 | -9.51 | 161.43 | 0.3845 | 70.0 | 128.7 | |
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back to the solar disc SDO HMI 2014-03-31 01:00:32 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 | 1.14 | 0.00 | 0.58 | -21.09 | 99.77 | 3.20 | 191.75 | 0.2566 | 583.0 | 452.8 | |
| 0.00 | 1.93 | 0.00 | 0.98 | -19.74 | 97.84 | 1.26 | 185.21 | 0.2290 | 744.0 | 515.5 | |
| 0.00 | 1.05 | 0.00 | 0.54 | -23.02 | 96.20 | -0.37 | 178.78 | 0.2837 | 768.0 | 551.4 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -26.96 | 90.77 | -5.81 | 165.47 | 0.3612 | 799.0 | 703.4 | |
| 0.00 | 3.59 | 0.00 | 1.91 | -26.70 | 90.75 | -5.83 | 165.22 | 0.3573 | 917.0 | 746.2 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -26.69 | 89.37 | -7.21 | 161.94 | 0.3633 | 723.0 | 572.0 | |
| 0.00 | 1.40 | 0.00 | 0.78 | -29.37 | 80.11 | -16.47 | 147.70 | 0.4644 | -924.0 | -758.5 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -29.08 | 80.16 | -16.42 | 147.39 | 0.4604 | -685.0 | -589.8 | |
| 0.00 | 1.40 | 0.00 | 0.79 | -29.42 | 77.75 | -18.83 | 144.42 | 0.4851 | -708.0 | -545.8 | |
| 0.00 | 1.67 | 0.00 | 0.95 | -29.03 | 76.08 | -20.50 | 141.70 | 0.4960 | -763.0 | -651.8 | |
| 0.00 | 0.61 | 0.00 | 0.37 | -29.48 | 68.69 | -27.89 | 134.51 | 0.5731 | -684.0 | -600.1 | |
| 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. | |