SDO HMI 2014-03-26 00:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.79 | 85.90 | 15.38 | 47.42 | 3.32 | 138.98 | -24.10 | 67.69 | 0.4423 | -12.0 | -96.0 | |
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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 |
| 0.35 | 1.84 | 0.19 | 1.00 | 3.68 | 141.31 | -21.76 | 64.78 | 0.4107 | -987.8 | -792.6 | |
| 3.41 | 24.47 | 1.85 | 13.30 | 3.29 | 141.10 | -21.98 | 65.85 | 0.4112 | -1078.2 | -752.0 | |
| 3.58 | -2.00 | 1.95 | -2.00 | 3.48 | 140.93 | -22.14 | 65.60 | 0.4149 | -995.5 | 999999 | |
| 2.36 | 5.59 | 1.29 | 3.05 | 3.98 | 140.79 | -22.29 | 64.68 | 0.4203 | -810.4 | -624.0 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 4.99 | 140.69 | -22.38 | 62.65 | 0.4289 | -689.0 | -645.6 | |
| 2.01 | 4.89 | 1.10 | 2.67 | 2.92 | 140.03 | -23.04 | 67.71 | 0.4242 | -876.8 | -692.0 | |
| 0.00 | 2.62 | 0.00 | 1.44 | 2.79 | 139.64 | -23.43 | 68.35 | 0.4291 | -259.0 | -183.4 | |
| 0.00 | 1.22 | 0.00 | 0.67 | 3.46 | 139.47 | -23.61 | 67.07 | 0.4359 | -760.0 | -623.7 | |
| 0.00 | 2.01 | 0.00 | 1.12 | 5.14 | 138.92 | -24.15 | 64.17 | 0.4547 | -893.0 | -673.7 | |
| 7.17 | 16.08 | 3.99 | 8.94 | 3.59 | 138.11 | -24.96 | 68.00 | 0.4561 | 932.4 | 777.2 | |
| 5.07 | 14.77 | 2.82 | 8.21 | 2.85 | 137.74 | -25.34 | 69.81 | 0.4573 | 961.6 | 638.2 | |
| 0.00 | 1.22 | 0.00 | 0.69 | 1.80 | 136.52 | -26.55 | 72.85 | 0.4695 | 810.0 | 616.9 | |
| 0.00 | 2.19 | 0.00 | 1.25 | 6.22 | 136.34 | -26.74 | 64.48 | 0.4976 | -756.0 | -520.0 | |
| 0.52 | 1.57 | 0.30 | 0.89 | 2.31 | 135.47 | -27.60 | 72.53 | 0.4874 | 953.7 | 817.3 | |
| 3.32 | 6.38 | 1.89 | 3.62 | 2.03 | 135.14 | -27.94 | 73.29 | 0.4908 | 907.6 | 665.8 | |
| 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. | |