SDO HMI 2014-04-02 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.77 | 68.55 | 25.85 | 80.71 | 10.25 | 359.86 | -63.21 | 75.51 | 0.9087 | 107.2 | 71.2 | |
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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 |
| 0.88 | 3.77 | 0.94 | 4.02 | 10.63 | 2.88 | -60.19 | 74.39 | 0.8874 | -296.9 | -259.5 | |
| 0.79 | 5.53 | 0.87 | 6.07 | 10.21 | 1.82 | -61.25 | 75.11 | 0.8947 | -399.0 | -419.9 | |
| 6.85 | 21.16 | 7.72 | 23.93 | 10.68 | 1.21 | -61.86 | 74.75 | 0.9000 | -242.8 | -81.7 | |
| 2.19 | -3.00 | 2.50 | -3.00 | 10.44 | 0.84 | -62.23 | 75.10 | 0.9023 | 160.9 | 999999 | |
| 0.00 | 0.97 | 0.00 | 1.10 | 9.60 | 0.59 | -62.48 | 76.07 | 0.9027 | 563.0 | 457.0 | |
| 0.70 | 1.84 | 0.84 | 2.21 | 10.97 | 359.56 | -63.51 | 74.82 | 0.9122 | -356.4 | -248.1 | |
| 0.00 | 0.53 | 0.00 | 0.61 | 9.43 | 0.11 | -62.96 | 76.36 | 0.9059 | 607.0 | 503.0 | |
| 0.00 | 2.28 | 0.00 | 2.74 | 10.77 | 359.43 | -63.64 | 75.07 | 0.9128 | 319.0 | 266.2 | |
| 2.46 | 15.80 | 2.90 | 18.71 | 9.54 | 359.60 | -63.47 | 76.35 | 0.9098 | 558.2 | 357.7 | |
| 1.14 | -9.00 | 1.37 | -9.00 | 9.44 | 359.07 | -63.99 | 76.57 | 0.9132 | 354.6 | 999999 | |
| 0.79 | 1.93 | 0.96 | 2.35 | 9.68 | 358.85 | -64.22 | 76.36 | 0.9151 | 374.2 | 323.5 | |
| 0.00 | 1.05 | 0.00 | 1.28 | 9.19 | 358.88 | -64.19 | 76.89 | 0.9142 | 119.0 | 161.3 | |
| 0.00 | 1.05 | 0.00 | 1.30 | 9.96 | 358.54 | -64.53 | 76.13 | 0.9176 | 395.0 | 376.5 | |
| 0.00 | 1.14 | 0.00 | 1.45 | 11.13 | 358.07 | -65.00 | 74.99 | 0.9223 | -121.0 | -133.2 | |
| 5.97 | 11.50 | 7.75 | 14.94 | 10.52 | 357.36 | -65.70 | 75.79 | 0.9260 | 189.1 | 96.4 | |
| 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. | |