SDO HMI 2014-05-14 20:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.77 | 278.62 | 35.66 | 172.40 | -23.71 | 193.73 | -31.20 | 127.56 | 0.6002 | 821.6 | 302.7 | |
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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 |
| 0.27 | 272.41 | 0.16 | 168.17 | -23.30 | 194.60 | -30.33 | 127.62 | 0.5878 | 1132.3 | 324.8 | |
| 4.93 | -1.00 | 3.03 | -1.00 | -23.65 | 194.43 | -30.50 | 128.01 | 0.5922 | 1195.8 | 999999 | |
| 3.68 | -1.00 | 2.25 | -1.00 | -23.39 | 194.38 | -30.55 | 127.59 | 0.5909 | 1210.2 | 999999 | |
| 8.16 | -1.00 | 5.02 | -1.00 | -23.62 | 194.21 | -30.72 | 127.78 | 0.5944 | 1191.4 | 999999 | |
| 1.79 | -1.00 | 1.11 | -1.00 | -24.04 | 194.10 | -30.83 | 128.30 | 0.5986 | 709.0 | 999999 | |
| 35.26 | -1.00 | 21.80 | -1.00 | -23.70 | 193.76 | -31.17 | 127.55 | 0.6000 | 1019.6 | 999999 | |
| 3.68 | -1.00 | 2.29 | -1.00 | -23.69 | 193.18 | -31.75 | 127.09 | 0.6063 | 430.5 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -23.22 | 192.61 | -32.32 | 125.99 | 0.6095 | 591.0 | 485.4 | |
| 0.00 | 1.53 | 0.00 | 1.04 | -25.65 | 186.58 | -38.35 | 125.49 | 0.6892 | -655.0 | -547.6 | |
| 0.00 | 0.81 | 0.00 | 0.56 | -26.17 | 186.16 | -38.77 | 125.93 | 0.6963 | -650.0 | -487.7 | |
| 0.00 | 0.81 | 0.00 | 0.56 | -26.00 | 186.10 | -38.83 | 125.67 | 0.6961 | -711.0 | -612.6 | |
| 0.00 | 0.90 | 0.00 | 0.62 | -26.55 | 185.53 | -39.40 | 126.07 | 0.7048 | -466.0 | -447.3 | |
| 0.00 | 1.17 | 0.00 | 0.83 | -24.68 | 182.93 | -42.00 | 122.34 | 0.7220 | -699.0 | -585.2 | |
| 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. | |