SDO HMI 2014-09-06 22:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.76 | 46.57 | 17.69 | 63.91 | -20.59 | 78.50 | -64.15 | 115.45 | 0.9334 | -60.1 | -68.8 | |
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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 | 3.66 | 0.00 | 4.36 | -20.54 | 82.35 | -60.30 | 116.56 | 0.9111 | 606.0 | 499.4 | |
| 1.34 | 5.26 | 1.62 | 6.41 | -20.30 | 81.78 | -60.87 | 116.13 | 0.9142 | 435.8 | 320.2 | |
| 1.25 | -2.00 | 1.53 | -2.00 | -20.60 | 81.51 | -61.14 | 116.35 | 0.9166 | 336.4 | 999999 | |
| 0.00 | 1.96 | 0.00 | 2.57 | -21.58 | 80.03 | -62.62 | 116.90 | 0.9275 | 563.0 | 438.5 | |
| 0.00 | 1.61 | 0.00 | 1.83 | -17.66 | 82.62 | -60.03 | 113.63 | 0.9028 | 581.0 | 479.6 | |
| 3.21 | 5.09 | 4.22 | 6.68 | -21.26 | 79.84 | -62.80 | 116.52 | 0.9279 | 160.5 | 41.8 | |
| 0.00 | 1.34 | 0.00 | 1.73 | -19.84 | 79.76 | -62.89 | 115.02 | 0.9256 | -339.0 | -368.2 | |
| 0.00 | 0.62 | 0.00 | 0.83 | -20.03 | 79.26 | -63.39 | 115.07 | 0.9289 | -271.0 | -357.3 | |
| 0.00 | 0.71 | 0.00 | 0.94 | -19.79 | 79.29 | -63.36 | 114.83 | 0.9283 | -600.0 | -569.1 | |
| 0.00 | 1.16 | 0.00 | 1.56 | -20.11 | 78.83 | -63.82 | 115.03 | 0.9316 | -473.0 | -438.8 | |
| 5.26 | 18.38 | 7.28 | 25.26 | -20.05 | 78.21 | -64.44 | 114.79 | 0.9350 | -494.8 | -361.1 | |
| 0.00 | 1.16 | 0.00 | 1.67 | -20.59 | 77.32 | -65.33 | 115.09 | 0.9408 | -106.0 | -90.5 | |
| 1.70 | 5.62 | 3.04 | 10.07 | -22.22 | 73.29 | -69.35 | 115.67 | 0.9624 | 65.5 | 41.8 | |
| 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. | |