SDO HMI 2014-07-18 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.08 | 26.97 | 3.54 | 15.79 | -21.96 | 67.24 | -18.59 | 146.37 | 0.5357 | -23.7 | -84.8 | |
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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 |
| 3.45 | 5.17 | 2.00 | 3.01 | -21.87 | 68.41 | -17.43 | 147.90 | 0.5250 | 984.2 | 766.8 | |
| 1.72 | 3.72 | 1.00 | 2.17 | -22.14 | 68.37 | -17.46 | 148.14 | 0.5286 | 799.7 | 700.0 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -21.60 | 68.23 | -17.60 | 147.35 | 0.5231 | 885.0 | 841.1 | |
| 0.00 | 2.45 | 0.00 | 1.42 | -21.71 | 68.01 | -17.82 | 147.15 | 0.5262 | 734.0 | 530.9 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -22.18 | 67.95 | -17.88 | 147.59 | 0.5325 | 348.0 | 312.0 | |
| 0.00 | 0.82 | 0.00 | 0.48 | -21.97 | 67.08 | -18.75 | 146.12 | 0.5369 | -571.0 | -453.7 | |
| 0.00 | 2.36 | 0.00 | 1.39 | -22.08 | 66.75 | -19.08 | 145.79 | 0.5410 | -608.0 | -548.2 | |
| 0.00 | 0.91 | 0.00 | 0.53 | -21.98 | 66.45 | -19.38 | 145.28 | 0.5424 | -673.0 | -455.5 | |
| 0.00 | 3.27 | 0.00 | 1.93 | -22.13 | 66.08 | -19.75 | 144.94 | 0.5472 | -594.0 | -564.5 | |
| 0.00 | 0.82 | 0.00 | 0.48 | -21.72 | 66.14 | -19.69 | 144.56 | 0.5419 | -712.0 | -615.4 | |
| 0.00 | 0.82 | 0.00 | 0.48 | -21.86 | 66.05 | -19.78 | 144.59 | 0.5443 | -834.0 | -695.7 | |
| 0.91 | 2.27 | 0.54 | 1.34 | -21.80 | 65.85 | -19.98 | 144.26 | 0.5453 | -829.0 | -695.9 | |
| 0.00 | 2.09 | 0.00 | 1.24 | -22.17 | 65.76 | -20.07 | 144.57 | 0.5504 | -617.0 | -527.4 | |
| 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. | |