SDO HMI 2014-03-30 01:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.29 | 0.00 | 8.38 | -27.87 | 84.85 | -24.92 | 136.21 | 0.5262 | -23.8 | 100.3 | |
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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 | 0.35 | 0.00 | 0.18 | -22.46 | 98.34 | -11.43 | 146.27 | 0.3313 | 593.0 | 584.0 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -22.50 | 97.54 | -12.23 | 144.60 | 0.3393 | 656.0 | 495.0 | |
| 0.00 | 2.02 | 0.00 | 1.12 | -27.00 | 90.82 | -18.95 | 140.67 | 0.4584 | 896.0 | 681.1 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -27.00 | 89.93 | -19.84 | 139.47 | 0.4672 | 819.0 | 670.9 | |
| 0.00 | 3.42 | 0.00 | 1.92 | -26.99 | 89.47 | -20.30 | 138.83 | 0.4717 | 590.0 | 602.4 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -27.65 | 82.68 | -27.09 | 132.47 | 0.5490 | -769.0 | -634.6 | |
| 0.00 | 1.75 | 0.00 | 1.10 | -30.00 | 77.97 | -31.80 | 132.02 | 0.6165 | -649.0 | -572.8 | |
| 0.00 | 0.96 | 0.00 | 0.61 | -29.73 | 76.72 | -33.05 | 130.74 | 0.6274 | -601.0 | -496.8 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -28.19 | 76.83 | -32.94 | 128.66 | 0.6160 | -728.0 | -658.5 | |
| 0.00 | 1.23 | 0.00 | 0.82 | -32.35 | 73.93 | -35.84 | 132.42 | 0.6723 | -548.0 | -423.4 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -27.78 | 74.89 | -34.88 | 126.81 | 0.6343 | -521.0 | -463.8 | |
| 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. | |