SDO HMI 2014-10-09 13:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.64 | 313.56 | 44.71 | 300.59 | -20.62 | 18.69 | -53.35 | 118.69 | 0.8580 | 562.6 | 163.3 | |
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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 | 1.14 | 0.00 | 1.03 | -19.95 | 20.90 | -51.14 | 118.85 | 0.8379 | 176.0 | 228.8 | |
| 0.00 | 2.37 | 0.00 | 2.17 | -20.20 | 20.27 | -51.78 | 118.87 | 0.8440 | 453.0 | 464.6 | |
| 1.67 | 301.47 | 1.54 | 289.22 | -20.52 | 20.01 | -52.03 | 119.11 | 0.8472 | 829.4 | 167.5 | |
| 44.62 | -3.00 | 42.84 | -3.00 | -20.71 | 18.64 | -53.40 | 118.77 | 0.8587 | 689.9 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.24 | -17.89 | 19.80 | -52.24 | 116.11 | 0.8400 | 456.0 | 346.0 | |
| 0.00 | 0.88 | 0.00 | 0.88 | -21.77 | 17.57 | -54.47 | 119.49 | 0.8703 | -248.0 | -226.0 | |
| 0.00 | 0.79 | 0.00 | 0.72 | -17.79 | 19.43 | -52.62 | 115.86 | 0.8429 | 484.0 | 412.9 | |
| 0.00 | 2.10 | 0.00 | 1.97 | -17.90 | 18.54 | -53.51 | 115.64 | 0.8507 | 220.0 | 131.8 | |
| 0.00 | 0.26 | 0.00 | 0.25 | -17.75 | 18.44 | -53.60 | 115.44 | 0.8509 | -276.0 | -367.7 | |
| 0.35 | 1.14 | 0.33 | 1.09 | -18.32 | 17.92 | -54.12 | 115.87 | 0.8570 | 234.0 | 222.1 | |
| 0.00 | 1.31 | 0.00 | 1.23 | -16.97 | 18.20 | -53.85 | 114.47 | 0.8506 | -169.0 | -229.5 | |
| 0.00 | 1.05 | 0.00 | 0.99 | -16.92 | 18.00 | -54.04 | 114.35 | 0.8521 | -420.0 | -389.1 | |
| 0.00 | 0.79 | 0.00 | 0.80 | -14.41 | 14.42 | -57.62 | 110.38 | 0.8746 | -478.0 | -400.8 | |
| 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. | |