SDO HMI 2014-10-06 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.23 | 0.00 | 10.87 | -19.20 | 100.02 | -9.95 | 161.26 | 0.4712 | -119.3 | -90.8 | |
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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 | 1.32 | 0.00 | 0.69 | -13.16 | 112.01 | 2.04 | 185.90 | 0.3384 | 805.0 | 660.6 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -15.14 | 110.23 | 0.25 | 180.67 | 0.3692 | 859.0 | 757.8 | |
| 0.00 | 1.93 | 0.00 | 1.11 | -24.47 | 109.11 | -0.86 | 178.47 | 0.5158 | 781.0 | 579.7 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -15.33 | 107.52 | -2.45 | 173.65 | 0.3746 | 788.0 | 612.2 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -16.83 | 106.34 | -3.63 | 171.27 | 0.4010 | 751.0 | 623.6 | |
| 0.00 | 1.58 | 0.00 | 0.85 | -16.73 | 106.16 | -3.82 | 170.79 | 0.4000 | 864.0 | 610.4 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -17.38 | 99.62 | -10.35 | 156.90 | 0.4388 | -702.0 | -566.3 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -19.14 | 98.90 | -11.07 | 157.10 | 0.4683 | -711.0 | -600.5 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -18.73 | 97.96 | -12.01 | 155.00 | 0.4685 | -725.0 | -599.5 | |
| 0.00 | 2.02 | 0.00 | 1.12 | -16.65 | 96.02 | -13.96 | 149.27 | 0.4542 | -909.0 | -697.4 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -13.35 | 95.41 | -14.56 | 143.86 | 0.4164 | -913.0 | -740.5 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -21.69 | 93.86 | -16.11 | 151.11 | 0.5358 | -734.0 | -576.7 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -23.35 | 93.55 | -16.42 | 152.21 | 0.5588 | -721.0 | -550.1 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -17.90 | 89.88 | -20.09 | 141.13 | 0.5229 | -670.0 | -435.0 | |
| 0.00 | 1.23 | 0.00 | 0.88 | -32.60 | 83.54 | -26.43 | 148.83 | 0.7268 | -553.0 | -474.4 | |
| 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. | |