SDO HMI 2014-03-30 23:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.54 | 78.02 | 47.60 | 200.04 | -11.26 | 17.66 | -80.02 | 100.24 | 0.9815 | -141.7 | -203.3 | |
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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 |
| 4.47 | 10.61 | 8.23 | 19.43 | -10.03 | 22.39 | -75.29 | 98.61 | 0.9645 | 359.2 | 332.3 | |
| 0.00 | 0.61 | 0.00 | 1.15 | -9.64 | 22.17 | -75.51 | 98.22 | 0.9656 | -205.0 | -155.3 | |
| 0.00 | 0.79 | 0.00 | 1.54 | -10.34 | 21.54 | -76.14 | 98.99 | 0.9681 | 168.0 | 64.4 | |
| 1.58 | 13.41 | 3.40 | 28.84 | -11.20 | 19.99 | -77.69 | 99.99 | 0.9742 | 208.1 | -71.1 | |
| 0.00 | 4.21 | 0.00 | 9.32 | -11.59 | 19.62 | -78.06 | 100.42 | 0.9755 | 312.0 | 120.0 | |
| 0.00 | 3.42 | 0.00 | 7.27 | -10.13 | 20.21 | -77.47 | 98.87 | 0.9737 | -488.0 | -396.6 | |
| 0.00 | 1.05 | 0.00 | 2.59 | -11.04 | 18.26 | -79.42 | 99.96 | 0.9805 | -237.0 | -208.1 | |
| 0.53 | 8.33 | 1.23 | 19.82 | -9.99 | 18.97 | -78.71 | 98.83 | 0.9783 | -281.7 | -403.9 | |
| 4.56 | 30.59 | 13.71 | 94.45 | -11.79 | 15.97 | -81.71 | 100.91 | 0.9872 | -458.7 | -363.9 | |
| 6.40 | -9.00 | 21.03 | -9.00 | -12.01 | 15.16 | -82.52 | 101.20 | 0.9893 | -181.2 | 999999 | |
| 0.00 | 0.53 | 0.00 | 1.44 | -10.58 | 17.15 | -80.53 | 99.58 | 0.9841 | -390.0 | -416.8 | |
| 0.00 | 1.75 | 0.00 | 5.33 | -10.95 | 16.08 | -81.60 | 100.05 | 0.9871 | -230.0 | -207.7 | |
| 0.00 | 2.72 | 0.00 | 8.86 | -11.24 | 15.43 | -82.24 | 100.40 | 0.9888 | -28.0 | 48.7 | |
| 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. | |