SDO HMI 2014-03-08 09:01:13 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.63 | 55.01 | 14.40 | 42.85 | -26.55 | 84.62 | 49.21 | 241.32 | 0.7738 | -536.0 | -370.9 | |
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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 | 0.52 | 0.00 | 0.48 | -23.05 | 93.55 | 58.14 | 247.29 | 0.8494 | 619.0 | 522.5 | |
| 0.00 | 0.87 | 0.00 | 0.78 | -23.99 | 92.08 | 56.67 | 245.98 | 0.8378 | 493.0 | 406.6 | |
| 0.00 | 0.69 | 0.00 | 0.65 | -25.91 | 93.16 | 57.75 | 243.88 | 0.8493 | 195.0 | 239.1 | |
| 0.00 | 0.61 | 0.00 | 0.51 | -25.67 | 88.42 | 53.01 | 243.35 | 0.8077 | -372.0 | -299.4 | |
| 7.45 | 40.89 | 5.80 | 31.64 | -26.47 | 84.61 | 49.20 | 241.46 | 0.7736 | -637.0 | -396.3 | |
| 4.94 | -5.00 | 3.80 | -5.00 | -26.34 | 83.98 | 48.56 | 241.46 | 0.7671 | -852.4 | 999999 | |
| 0.00 | 3.03 | 0.00 | 2.38 | -27.72 | 84.79 | 49.38 | 239.95 | 0.7786 | -819.0 | -587.1 | |
| 1.91 | -5.00 | 1.47 | -5.00 | -26.77 | 84.17 | 48.76 | 240.97 | 0.7702 | -611.1 | 999999 | |
| 1.13 | -5.00 | 0.87 | -5.00 | -26.56 | 83.95 | 48.54 | 241.17 | 0.7675 | -974.2 | 999999 | |
| 3.20 | 5.11 | 2.46 | 3.92 | -26.87 | 83.77 | 48.36 | 240.73 | 0.7666 | -754.0 | -596.0 | |
| 0.00 | 1.56 | 0.00 | 1.20 | -27.31 | 83.88 | 48.47 | 240.20 | 0.7688 | -616.0 | -448.6 | |
| 0.00 | 0.78 | 0.00 | 0.59 | -28.11 | 82.98 | 47.57 | 238.92 | 0.7624 | -361.0 | -393.9 | |
| 0.00 | 0.95 | 0.00 | 0.70 | -28.45 | 80.47 | 45.06 | 237.64 | 0.7391 | -611.0 | -399.5 | |
| 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. | |