SDO HMI 2014-11-05 09:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.06 | 37.41 | 5.49 | 18.77 | 5.73 | 70.13 | -8.01 | 72.75 | 0.1440 | -121.8 | 117.2 | |
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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 |
| 7.26 | 16.76 | 3.60 | 8.32 | 5.75 | 74.49 | -3.65 | 63.40 | 0.0712 | -1211.7 | -803.5 | |
| 3.80 | -1.00 | 1.89 | -1.00 | 5.84 | 74.36 | -3.77 | 63.04 | 0.0737 | -1087.7 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.60 | 6.18 | 72.50 | -5.63 | 67.94 | 0.1058 | -901.0 | -583.3 | |
| 0.00 | 1.30 | 0.00 | 0.65 | 5.37 | 70.77 | -7.37 | 78.67 | 0.1308 | -994.0 | -796.1 | |
| 0.00 | 0.60 | 0.00 | 0.30 | 5.92 | 68.92 | -9.22 | 77.45 | 0.1639 | -506.0 | -443.6 | |
| 0.00 | 1.64 | 0.00 | 0.83 | 6.24 | 68.67 | -9.46 | 75.86 | 0.1693 | -951.0 | -788.1 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 5.47 | 66.32 | -11.82 | 82.11 | 0.2068 | 865.0 | 740.4 | |
| 0.00 | 1.04 | 0.00 | 0.52 | 5.30 | 66.32 | -11.82 | 82.97 | 0.2064 | 966.0 | 747.8 | |
| 0.00 | 3.37 | 0.00 | 1.71 | 4.70 | 66.08 | -12.05 | 85.94 | 0.2096 | 797.0 | 696.3 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 5.05 | 65.83 | -12.30 | 84.34 | 0.2142 | 861.0 | 750.1 | |
| 0.00 | 2.33 | 0.00 | 1.18 | 6.51 | 65.74 | -12.39 | 77.72 | 0.2192 | 891.0 | 824.0 | |
| 0.00 | 1.47 | 0.00 | 0.75 | 6.27 | 65.75 | -12.39 | 78.78 | 0.2184 | 936.0 | 798.3 | |
| 0.00 | 0.95 | 0.00 | 0.48 | 6.71 | 65.34 | -12.80 | 77.18 | 0.2266 | 794.0 | 547.5 | |
| 0.00 | 1.56 | 0.00 | 0.79 | 5.81 | 65.15 | -12.99 | 81.23 | 0.2273 | 872.0 | 561.8 | |
| 0.00 | 3.28 | 0.00 | 1.67 | 5.45 | 64.91 | -13.23 | 82.92 | 0.2306 | 536.0 | 542.7 | |
| 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. | |