SDO HMI 2014-04-21 07:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.13 | 73.42 | 20.04 | 70.04 | -23.26 | 117.88 | -58.20 | 114.16 | 0.8577 | 580.5 | 354.2 | |
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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 | 1.78 | 0.00 | 1.69 | -25.39 | 118.43 | -57.66 | 116.72 | 0.8565 | 496.0 | 368.2 | |
| 16.07 | 58.50 | 15.15 | 55.10 | -23.18 | 118.46 | -57.62 | 114.16 | 0.8530 | 821.2 | 426.4 | |
| 4.53 | -2.00 | 4.34 | -2.00 | -23.36 | 117.84 | -58.24 | 114.27 | 0.8583 | 383.5 | 999999 | |
| 0.00 | 1.07 | 0.00 | 1.02 | -22.88 | 117.86 | -58.22 | 113.72 | 0.8575 | 418.0 | 287.2 | |
| 0.00 | 2.40 | 0.00 | 2.34 | -22.89 | 117.16 | -58.93 | 113.62 | 0.8633 | 393.0 | 246.1 | |
| 0.00 | 2.57 | 0.00 | 2.47 | -22.15 | 117.66 | -58.42 | 112.85 | 0.8583 | 504.0 | 343.7 | |
| 0.00 | 0.44 | 0.00 | 0.44 | -21.99 | 116.76 | -59.32 | 112.54 | 0.8654 | -460.0 | -437.0 | |
| 0.00 | 0.89 | 0.00 | 0.91 | -23.79 | 115.36 | -60.72 | 114.40 | 0.8784 | 487.0 | 332.0 | |
| 0.00 | 2.04 | 0.00 | 2.12 | -23.87 | 115.09 | -60.99 | 114.45 | 0.8805 | 412.0 | 311.4 | |
| 0.53 | 2.75 | 0.55 | 2.84 | -22.79 | 115.05 | -61.03 | 113.23 | 0.8797 | -290.5 | -295.2 | |
| 0.00 | 0.98 | 0.00 | 1.11 | -25.58 | 112.26 | -63.82 | 116.00 | 0.9024 | 81.0 | 80.9 | |
| 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. | |