SDO HMI 2014-07-08 03:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.18 | 26.25 | 1.28 | 16.08 | -21.46 | 200.47 | -25.95 | 136.25 | 0.5878 | 1.6 | -70.3 | |
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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 |
| 2.18 | 5.72 | 1.28 | 3.35 | -21.21 | 205.42 | -21.00 | 141.23 | 0.5357 | 869.3 | 621.3 | |
| 0.00 | 3.91 | 0.00 | 2.33 | -22.95 | 204.75 | -21.67 | 142.50 | 0.5608 | -970.0 | -731.8 | |
| 0.00 | 1.00 | 0.00 | 0.60 | -21.82 | 203.77 | -22.66 | 139.93 | 0.5576 | 460.0 | 490.2 | |
| 0.00 | 2.18 | 0.00 | 1.30 | -21.62 | 203.77 | -22.66 | 139.67 | 0.5555 | 662.0 | 500.2 | |
| 0.00 | 0.64 | 0.00 | 0.38 | -21.29 | 203.68 | -22.74 | 139.15 | 0.5529 | 590.0 | 502.7 | |
| 0.00 | 1.18 | 0.00 | 0.71 | -22.56 | 202.53 | -23.90 | 139.38 | 0.5769 | 582.0 | 338.5 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -20.55 | 202.31 | -24.12 | 136.58 | 0.5588 | 612.0 | 490.5 | |
| 0.00 | 1.54 | 0.00 | 0.96 | -22.85 | 199.50 | -26.93 | 136.48 | 0.6082 | 695.0 | 510.1 | |
| 0.00 | 0.73 | 0.00 | 0.46 | -20.95 | 195.57 | -30.86 | 130.39 | 0.6312 | -691.0 | -595.5 | |
| 0.00 | 3.54 | 0.00 | 2.27 | -21.26 | 195.46 | -30.97 | 130.69 | 0.6347 | -518.0 | -515.0 | |
| 0.00 | 0.73 | 0.00 | 0.46 | -20.76 | 195.23 | -31.20 | 129.85 | 0.6332 | -656.0 | -462.0 | |
| 0.00 | 1.18 | 0.00 | 0.76 | -21.11 | 194.76 | -31.66 | 129.91 | 0.6407 | -632.0 | -556.2 | |
| 0.00 | 0.73 | 0.00 | 0.47 | -20.98 | 194.60 | -31.83 | 129.61 | 0.6414 | -554.0 | -452.1 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -22.06 | 192.48 | -33.94 | 129.30 | 0.6709 | -121.0 | -244.0 | |
| 0.00 | 1.63 | 0.00 | 1.09 | -18.66 | 190.03 | -36.39 | 123.18 | 0.6739 | -547.0 | -477.7 | |
| 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. | |