SDO HMI 2014-11-06 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.54 | 23.38 | 2.57 | 16.82 | -16.46 | 16.61 | -42.29 | 117.07 | 0.7269 | -191.8 | -289.3 | |
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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 | 0.52 | 0.00 | 0.33 | -13.34 | 23.89 | -35.01 | 116.90 | 0.6282 | 626.0 | 569.5 | |
| 0.00 | 1.55 | 0.00 | 1.09 | -19.95 | 20.01 | -38.89 | 123.39 | 0.7093 | 184.0 | 203.1 | |
| 0.00 | 1.21 | 0.00 | 0.80 | -13.77 | 20.88 | -38.02 | 115.73 | 0.6665 | 573.0 | 428.2 | |
| 0.00 | 1.29 | 0.00 | 0.90 | -14.81 | 17.70 | -41.20 | 115.48 | 0.7077 | 793.0 | 684.1 | |
| 0.00 | 1.29 | 0.00 | 0.91 | -14.98 | 17.37 | -41.53 | 115.54 | 0.7121 | 477.0 | 449.8 | |
| 0.00 | 1.90 | 0.00 | 1.37 | -15.94 | 16.26 | -42.65 | 116.24 | 0.7286 | -465.0 | -501.6 | |
| 0.00 | 1.73 | 0.00 | 1.26 | -16.97 | 15.84 | -43.06 | 117.34 | 0.7375 | -621.0 | -552.8 | |
| 2.07 | 7.85 | 1.50 | 5.69 | -16.08 | 16.01 | -42.89 | 116.29 | 0.7318 | -912.1 | -700.1 | |
| 0.00 | 0.69 | 0.00 | 0.50 | -16.69 | 15.75 | -43.15 | 116.95 | 0.7372 | -554.0 | -438.1 | |
| 1.47 | 2.42 | 1.07 | 1.76 | -16.13 | 15.61 | -43.29 | 116.17 | 0.7363 | -643.1 | -506.5 | |
| 0.00 | 1.55 | 0.00 | 1.17 | -18.84 | 14.74 | -44.16 | 119.12 | 0.7571 | -585.0 | -509.6 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -15.98 | 15.57 | -43.33 | 115.95 | 0.7360 | -557.0 | -465.0 | |
| 0.00 | 1.12 | 0.00 | 0.85 | -18.98 | 14.47 | -44.43 | 119.16 | 0.7604 | -417.0 | -388.8 | |
| 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. | |