SDO HMI 2014-03-30 23:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.70 | 0.00 | 10.14 | -12.76 | 83.05 | -14.63 | 114.44 | 0.2718 | 411.5 | 354.3 | |
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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 | 1.23 | 0.00 | 0.62 | -13.69 | 89.14 | -8.54 | 130.76 | 0.1914 | 740.0 | 570.0 | |
| 0.00 | 0.96 | 0.00 | 0.49 | -12.70 | 85.12 | -12.56 | 117.11 | 0.2394 | 805.0 | 624.1 | |
| 0.00 | 1.58 | 0.00 | 0.80 | -12.09 | 84.90 | -12.78 | 114.41 | 0.2386 | 905.0 | 593.9 | |
| 0.00 | 1.40 | 0.00 | 0.71 | -11.70 | 84.82 | -12.86 | 112.75 | 0.2374 | 1072.0 | 891.8 | |
| 0.00 | 1.75 | 0.00 | 0.89 | -11.61 | 84.61 | -13.07 | 112.06 | 0.2401 | 856.0 | 783.0 | |
| 0.00 | 2.63 | 0.00 | 1.34 | -11.69 | 84.29 | -13.39 | 111.94 | 0.2456 | 1048.0 | 852.8 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -12.11 | 84.27 | -13.41 | 113.51 | 0.2484 | 835.0 | 650.1 | |
| 0.00 | 1.40 | 0.00 | 0.72 | -11.42 | 83.39 | -14.29 | 109.81 | 0.2583 | 913.0 | 740.9 | |
| 0.00 | 0.70 | 0.00 | 0.36 | -10.88 | 82.25 | -15.43 | 106.68 | 0.2739 | 696.0 | 611.4 | |
| 0.00 | 0.61 | 0.00 | 0.32 | -11.87 | 82.16 | -15.52 | 110.04 | 0.2799 | 720.0 | 589.7 | |
| 0.00 | 1.31 | 0.00 | 0.68 | -14.59 | 81.63 | -16.05 | 118.12 | 0.3048 | -923.0 | -725.1 | |
| 0.00 | 1.40 | 0.00 | 0.73 | -15.42 | 80.82 | -16.86 | 119.41 | 0.3225 | -929.0 | -660.9 | |
| 0.00 | 1.31 | 0.00 | 0.69 | -14.39 | 79.12 | -18.56 | 114.56 | 0.3405 | -654.0 | -470.2 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -14.94 | 78.61 | -19.07 | 115.54 | 0.3514 | -678.0 | -646.4 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -12.33 | 77.50 | -20.18 | 107.52 | 0.3550 | 766.0 | 698.3 | |
| 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. | |