SDO HMI 2014-11-15 12:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.89 | 80.48 | 32.38 | 122.70 | 13.91 | 15.66 | 71.01 | 283.76 | 0.9461 | -335.3 | -27.6 | |
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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 |
| 5.67 | 22.87 | 9.26 | 37.67 | 13.27 | 17.11 | 72.46 | 283.04 | 0.9540 | -288.0 | 23.2 | |
| 0.00 | 0.86 | 0.00 | 1.31 | 12.88 | 15.74 | 71.09 | 282.66 | 0.9466 | -435.0 | -372.1 | |
| 0.00 | 0.26 | 0.00 | 0.39 | 12.50 | 15.40 | 70.74 | 282.27 | 0.9447 | -216.0 | -308.7 | |
| 4.21 | 8.34 | 6.32 | 12.48 | 13.41 | 15.54 | 70.88 | 283.22 | 0.9456 | -518.5 | -441.8 | |
| 11.01 | 36.03 | 16.80 | 55.35 | 14.28 | 15.79 | 71.14 | 284.14 | 0.9472 | -408.0 | 34.5 | |
| 0.00 | 1.46 | 0.00 | 2.12 | 13.87 | 14.75 | 70.09 | 283.74 | 0.9412 | -412.0 | -369.4 | |
| 0.00 | 0.95 | 0.00 | 1.37 | 14.17 | 14.78 | 70.12 | 284.06 | 0.9415 | -309.0 | -282.5 | |
| 0.00 | 0.86 | 0.00 | 1.20 | 15.19 | 13.99 | 69.33 | 285.18 | 0.9372 | -460.0 | -324.4 | |
| 0.00 | 1.46 | 0.00 | 1.79 | 13.99 | 10.75 | 66.10 | 284.06 | 0.9163 | 106.0 | 100.1 | |
| 0.00 | 1.29 | 0.00 | 1.58 | 14.17 | 10.71 | 66.05 | 284.26 | 0.9160 | 342.0 | 261.5 | |
| 0.00 | 2.06 | 0.00 | 2.48 | 13.98 | 10.22 | 65.57 | 284.08 | 0.9126 | 569.0 | 448.4 | |
| 0.00 | 2.92 | 0.00 | 3.60 | 15.82 | 10.80 | 66.15 | 286.06 | 0.9174 | -164.0 | -216.6 | |
| 0.00 | 1.12 | 0.00 | 1.36 | 15.56 | 10.48 | 65.83 | 285.79 | 0.9151 | -432.0 | -385.3 | |
| 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. | |