SDO HMI 2014-04-22 19:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.26 | 34.56 | 2.19 | 18.40 | -19.90 | 140.73 | -15.55 | 136.89 | 0.3649 | 413.1 | 114.0 | |
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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 |
| 4.26 | 5.95 | 2.19 | 3.06 | -17.63 | 146.86 | -9.41 | 144.69 | 0.2709 | 1131.7 | 785.6 | |
| 0.00 | 0.98 | 0.00 | 0.51 | -18.81 | 145.41 | -10.87 | 143.42 | 0.3009 | 705.0 | 528.0 | |
| 0.00 | 2.13 | 0.00 | 1.10 | -18.38 | 145.37 | -10.91 | 142.40 | 0.2956 | 1046.0 | 798.4 | |
| 0.00 | 2.75 | 0.00 | 1.43 | -18.73 | 144.18 | -12.10 | 140.34 | 0.3124 | 1124.0 | 864.3 | |
| 0.00 | 1.07 | 0.00 | 0.56 | -20.20 | 141.72 | -14.56 | 138.35 | 0.3565 | 828.0 | 622.2 | |
| 0.00 | 0.98 | 0.00 | 0.52 | -21.73 | 140.99 | -15.28 | 139.92 | 0.3819 | 759.0 | 603.6 | |
| 0.00 | 3.91 | 0.00 | 2.09 | -20.71 | 140.53 | -15.74 | 137.21 | 0.3752 | 1036.0 | 720.9 | |
| 0.00 | 3.55 | 0.00 | 1.90 | -20.67 | 140.14 | -16.14 | 136.45 | 0.3791 | 567.0 | 626.6 | |
| 0.00 | 5.15 | 0.00 | 2.81 | -21.44 | 137.33 | -18.95 | 133.60 | 0.4191 | -1028.0 | -834.4 | |
| 0.00 | 0.98 | 0.00 | 0.52 | -16.80 | 137.29 | -18.99 | 123.91 | 0.3770 | 808.0 | 656.9 | |
| 0.00 | 2.49 | 0.00 | 1.36 | -20.72 | 136.37 | -19.91 | 130.93 | 0.4233 | -726.0 | -647.5 | |
| 0.00 | 1.42 | 0.00 | 0.78 | -20.62 | 136.14 | -20.13 | 130.44 | 0.4251 | -831.0 | -724.1 | |
| 0.00 | 3.20 | 0.00 | 1.76 | -21.19 | 135.30 | -20.98 | 130.45 | 0.4405 | -905.0 | -648.6 | |
| 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. | |