SDO HMI 2014-09-20 09:01:19 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.51 | 0.00 | 9.90 | 8.83 | 333.79 | 8.84 | 246.22 | 0.1887 | -65.5 | 53.7 | |
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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 | 1.42 | 0.00 | 0.75 | 7.08 | 345.06 | 20.11 | 271.21 | 0.3427 | -798.0 | -681.2 | |
| 0.00 | 1.24 | 0.00 | 0.65 | 7.75 | 344.39 | 19.43 | 273.17 | 0.3315 | -829.0 | -570.4 | |
| 0.00 | 0.98 | 0.00 | 0.51 | 8.87 | 344.25 | 19.29 | 276.59 | 0.3301 | -804.0 | -582.5 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 8.99 | 344.10 | 19.14 | 277.01 | 0.3277 | -876.0 | -661.8 | |
| 0.00 | 2.31 | 0.00 | 1.20 | 9.25 | 342.98 | 18.03 | 278.11 | 0.3099 | -921.0 | -658.6 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 9.91 | 339.58 | 14.62 | 282.04 | 0.2554 | -787.0 | -648.0 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 10.00 | 334.11 | 9.16 | 288.39 | 0.1659 | -772.0 | -526.6 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 8.94 | 330.40 | 5.44 | 289.27 | 0.0996 | 651.0 | 551.5 | |
| 0.00 | 3.10 | 0.00 | 1.54 | 7.63 | 329.28 | 4.32 | 277.35 | 0.0757 | 855.0 | 736.1 | |
| 0.00 | 0.98 | 0.00 | 0.48 | 7.73 | 328.09 | 3.14 | 281.72 | 0.0556 | 1035.0 | 843.9 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 7.76 | 327.94 | 2.98 | 282.85 | 0.0531 | 721.0 | 681.9 | |
| 0.00 | 1.86 | 0.00 | 0.92 | 5.67 | 325.11 | 0.15 | 186.09 | 0.0252 | 902.0 | 550.0 | |
| 0.00 | 2.04 | 0.00 | 1.03 | 14.64 | 317.04 | -7.91 | 45.20 | 0.1886 | 771.0 | 697.5 | |
| 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. | |