SDO HMI 2014-10-09 16:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.96 | 22.60 | 3.16 | 12.12 | -13.46 | 59.86 | -10.53 | 152.49 | 0.3827 | 412.6 | 177.6 | |
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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 | 1.05 | 0.00 | 0.56 | -14.77 | 63.12 | -7.27 | 161.11 | 0.3798 | 612.0 | 458.5 | |
| 3.51 | 5.17 | 1.86 | 2.74 | -13.03 | 62.34 | -8.05 | 157.47 | 0.3578 | 1115.0 | 863.3 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -13.95 | 62.09 | -8.30 | 157.84 | 0.3733 | 843.0 | 735.2 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -12.90 | 62.13 | -8.27 | 156.80 | 0.3573 | 773.0 | 597.6 | |
| 0.00 | 1.31 | 0.00 | 0.70 | -13.22 | 62.08 | -8.31 | 157.05 | 0.3623 | 798.0 | 656.1 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -13.99 | 60.12 | -10.27 | 153.30 | 0.3869 | 880.0 | 593.3 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -12.30 | 60.07 | -10.33 | 151.04 | 0.3633 | -803.0 | -697.9 | |
| 2.45 | 5.17 | 1.30 | 2.74 | -11.93 | 59.77 | -10.62 | 149.83 | 0.3604 | -1022.6 | -877.0 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -13.52 | 59.61 | -10.79 | 151.59 | 0.3841 | 751.0 | 555.6 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -16.58 | 56.63 | -13.76 | 149.36 | 0.4493 | 693.0 | 509.1 | |
| 0.00 | 1.31 | 0.00 | 0.72 | -14.93 | 55.50 | -14.89 | 145.23 | 0.4373 | 703.0 | 603.8 | |
| 0.00 | 0.44 | 0.00 | 0.25 | -16.72 | 54.81 | -15.58 | 146.35 | 0.4662 | 721.0 | 586.0 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -15.22 | 52.40 | -17.99 | 140.45 | 0.4699 | -873.0 | -659.5 | |
| 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. | |