SDO HMI 2014-11-03 14:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.31 | 0.00 | 10.67 | -19.17 | 80.12 | -21.65 | 138.48 | 0.5254 | 707.9 | 565.8 | |
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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 |
| 0.00 | 1.12 | 0.00 | 0.62 | -16.79 | 84.78 | -16.99 | 141.70 | 0.4532 | 806.0 | 556.7 | |
| 0.00 | 1.38 | 0.00 | 0.77 | -17.11 | 84.72 | -17.05 | 142.05 | 0.4576 | 751.0 | 510.7 | |
| 0.00 | 1.38 | 0.00 | 0.77 | -17.40 | 84.59 | -17.18 | 142.26 | 0.4623 | 802.0 | 631.5 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -20.94 | 82.86 | -18.91 | 144.23 | 0.5199 | 790.0 | 647.1 | |
| 0.00 | 1.56 | 0.00 | 0.86 | -14.77 | 83.12 | -18.65 | 136.02 | 0.4471 | 679.0 | 498.7 | |
| 0.00 | 3.37 | 0.00 | 1.98 | -20.23 | 79.70 | -22.07 | 139.15 | 0.5410 | 792.0 | 673.1 | |
| 0.00 | 1.38 | 0.00 | 0.82 | -19.93 | 79.07 | -22.70 | 137.96 | 0.5440 | 215.0 | 206.1 | |
| 0.00 | 1.12 | 0.00 | 0.67 | -20.52 | 78.94 | -22.83 | 138.57 | 0.5514 | 732.0 | 654.8 | |
| 0.00 | 1.12 | 0.00 | 0.67 | -20.41 | 78.09 | -23.68 | 137.43 | 0.5585 | 737.0 | 555.8 | |
| 0.00 | 1.30 | 0.00 | 0.77 | -20.32 | 77.90 | -23.87 | 137.08 | 0.5595 | 677.0 | 513.1 | |
| 0.00 | 1.30 | 0.00 | 0.78 | -20.06 | 76.58 | -25.19 | 135.26 | 0.5702 | 817.0 | 668.5 | |
| 0.00 | 1.38 | 0.00 | 0.83 | -20.23 | 76.55 | -25.22 | 135.45 | 0.5720 | 753.0 | 618.2 | |
| 0.00 | 1.04 | 0.00 | 0.63 | -19.85 | 76.02 | -25.75 | 134.38 | 0.5739 | 652.0 | 499.8 | |
| 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. | |