SDO HMI 2014-11-05 07:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.93 | 35.09 | 5.93 | 17.67 | 5.89 | 70.04 | -9.19 | 75.24 | 0.1641 | -103.4 | 136.0 | |
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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 |
| 2.07 | 16.25 | 1.03 | 8.08 | 5.90 | 74.50 | -4.73 | 67.26 | 0.0893 | -1128.2 | -825.5 | |
| 6.40 | -1.00 | 3.18 | -1.00 | 5.72 | 74.41 | -4.81 | 69.49 | 0.0896 | -1219.6 | 999999 | |
| 3.46 | -1.00 | 1.72 | -1.00 | 5.84 | 74.32 | -4.91 | 68.61 | 0.0918 | -1067.0 | 999999 | |
| 0.00 | 1.47 | 0.00 | 0.74 | 5.37 | 70.84 | -8.39 | 80.00 | 0.1482 | -1049.0 | -801.9 | |
| 0.00 | 3.11 | 0.00 | 1.57 | 6.25 | 68.73 | -10.49 | 77.17 | 0.1865 | -957.0 | -699.7 | |
| 0.00 | 1.47 | 0.00 | 0.75 | 5.47 | 66.28 | -12.95 | 82.77 | 0.2259 | 971.0 | 741.6 | |
| 0.00 | 3.37 | 0.00 | 1.71 | 4.73 | 66.14 | -13.09 | 86.11 | 0.2272 | 768.0 | 646.4 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 5.02 | 65.86 | -13.37 | 84.91 | 0.2323 | 917.0 | 702.7 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 6.29 | 65.61 | -13.61 | 79.62 | 0.2389 | 1008.0 | 835.3 | |
| 0.00 | 2.42 | 0.00 | 1.23 | 6.47 | 65.61 | -13.62 | 78.89 | 0.2395 | 1065.0 | 798.4 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 5.87 | 65.13 | -14.09 | 81.64 | 0.2460 | 909.0 | 659.2 | |
| 0.00 | 2.68 | 0.00 | 1.37 | 5.45 | 64.90 | -14.33 | 83.44 | 0.2492 | 813.0 | 643.5 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 10.96 | 62.53 | -16.70 | 66.12 | 0.3099 | 784.0 | 579.3 | |
| 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. | |