SDO HMI 2014-11-15 09:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.26 | 93.13 | 27.65 | 131.48 | 13.87 | 15.72 | 69.43 | 283.78 | 0.9370 | -418.8 | -74.7 | |
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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 |
| 5.59 | 23.48 | 8.42 | 35.65 | 13.25 | 17.28 | 70.99 | 283.05 | 0.9461 | -317.8 | 38.1 | |
| 0.00 | 0.77 | 0.00 | 1.13 | 13.25 | 16.63 | 70.33 | 283.07 | 0.9425 | -390.0 | -386.1 | |
| 0.00 | 0.86 | 0.00 | 1.19 | 12.57 | 15.48 | 69.19 | 282.39 | 0.9356 | -385.0 | -357.2 | |
| 3.78 | 13.42 | 5.25 | 18.57 | 13.43 | 15.49 | 69.19 | 283.30 | 0.9359 | -566.9 | -456.5 | |
| 9.89 | 40.60 | 13.98 | 57.83 | 14.23 | 15.85 | 69.56 | 284.15 | 0.9382 | -516.7 | 19.6 | |
| 0.00 | 2.06 | 0.00 | 2.78 | 13.92 | 14.77 | 68.48 | 283.85 | 0.9316 | -519.0 | -381.0 | |
| 0.00 | 1.20 | 0.00 | 1.63 | 14.16 | 14.84 | 68.55 | 284.11 | 0.9321 | -423.0 | -348.0 | |
| 0.00 | 2.06 | 0.00 | 2.70 | 15.24 | 13.98 | 67.68 | 285.32 | 0.9271 | -530.0 | -446.5 | |
| 0.00 | 1.46 | 0.00 | 1.71 | 14.81 | 11.09 | 64.80 | 285.05 | 0.9076 | -521.0 | -455.9 | |
| 0.00 | 2.84 | 0.00 | 3.27 | 14.28 | 10.72 | 64.43 | 284.48 | 0.9047 | 301.0 | 201.1 | |
| 0.00 | 2.58 | 0.00 | 2.92 | 13.96 | 10.27 | 63.98 | 284.16 | 0.9013 | 590.0 | 417.2 | |
| 0.00 | 1.03 | 0.00 | 1.21 | 15.86 | 10.98 | 64.69 | 286.21 | 0.9074 | -423.0 | -392.6 | |
| 0.00 | 0.77 | 0.00 | 0.89 | 15.61 | 10.47 | 64.18 | 285.97 | 0.9036 | -591.0 | -559.9 | |
| 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. | |