SDO HMI 2014-11-03 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.53 | 36.10 | 6.66 | 19.28 | -17.22 | 98.76 | 0.30 | 181.26 | 0.3743 | 52.5 | -187.3 | |
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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 |
| 6.05 | 14.86 | 3.22 | 7.90 | -16.53 | 103.93 | 5.47 | 194.55 | 0.3656 | 988.6 | 769.4 | |
| 3.80 | -1.00 | 2.02 | -1.00 | -16.37 | 103.83 | 5.37 | 194.41 | 0.3627 | 1116.7 | 999999 | |
| 2.68 | 4.23 | 1.42 | 2.25 | -16.85 | 100.36 | 1.90 | 185.07 | 0.3610 | 1099.0 | 856.4 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -17.04 | 99.21 | 0.75 | 181.99 | 0.3629 | 741.0 | 603.1 | |
| 0.00 | 2.33 | 0.00 | 1.24 | -16.85 | 96.10 | -2.35 | 173.73 | 0.3616 | -789.0 | -553.9 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -17.07 | 96.04 | -2.42 | 173.63 | 0.3654 | -796.0 | -599.3 | |
| 0.00 | 2.07 | 0.00 | 1.11 | -17.62 | 94.25 | -4.21 | 169.30 | 0.3785 | -785.0 | -675.8 | |
| 0.00 | 3.28 | 0.00 | 1.76 | -18.20 | 93.80 | -4.66 | 168.50 | 0.3891 | -840.0 | -691.8 | |
| 0.00 | 1.73 | 0.00 | 0.92 | -17.46 | 93.63 | -4.83 | 167.68 | 0.3780 | -825.0 | -692.0 | |
| 0.00 | 1.56 | 0.00 | 0.84 | -18.11 | 93.30 | -5.16 | 167.26 | 0.3893 | -882.0 | -643.7 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -16.36 | 91.67 | -6.79 | 162.01 | 0.3691 | -880.0 | -767.4 | |
| 0.00 | 2.07 | 0.00 | 1.13 | -19.61 | 91.38 | -7.08 | 163.88 | 0.4202 | -665.0 | -482.6 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -21.77 | 91.04 | -7.41 | 164.64 | 0.4543 | -403.0 | -404.5 | |
| 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. | |