SDO HMI 2014-07-18 20:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.99 | 31.39 | 4.05 | 18.26 | -21.96 | 67.28 | -17.44 | 148.02 | 0.5266 | 20.8 | 26.0 | |
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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 |
| 2.00 | 9.16 | 1.15 | 5.29 | -22.00 | 68.52 | -16.21 | 149.85 | 0.5174 | 824.7 | 744.1 | |
| 2.72 | -1.00 | 1.57 | -1.00 | -21.79 | 68.51 | -16.22 | 149.62 | 0.5149 | 1051.1 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -21.56 | 68.36 | -16.36 | 149.16 | 0.5130 | 1061.0 | 766.7 | |
| 0.00 | 2.09 | 0.00 | 1.21 | -22.24 | 68.14 | -16.58 | 149.55 | 0.5233 | 686.0 | 550.0 | |
| 0.36 | 4.08 | 0.21 | 2.36 | -21.84 | 68.09 | -16.63 | 149.04 | 0.5186 | 745.8 | 737.8 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -22.09 | 67.47 | -17.25 | 148.40 | 0.5265 | -132.0 | -117.7 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -21.86 | 66.88 | -17.84 | 147.30 | 0.5284 | -781.0 | -553.1 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -22.00 | 66.86 | -17.86 | 147.43 | 0.5302 | -702.0 | -577.2 | |
| 0.00 | 1.81 | 0.00 | 1.06 | -22.08 | 66.54 | -18.18 | 147.06 | 0.5337 | -414.0 | -409.2 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -22.02 | 66.14 | -18.59 | 146.42 | 0.5364 | -812.0 | -680.6 | |
| 1.09 | 4.54 | 0.64 | 2.66 | -21.82 | 65.85 | -18.87 | 145.80 | 0.5364 | -855.6 | -742.1 | |
| 0.82 | 3.63 | 0.48 | 2.13 | -22.20 | 65.80 | -18.93 | 146.15 | 0.5412 | -673.7 | -537.3 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -22.34 | 65.67 | -19.05 | 146.14 | 0.5439 | -570.0 | -446.1 | |
| 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. | |