SDO HMI 2014-11-13 16:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.38 | 257.53 | 65.18 | 674.35 | -12.36 | 251.20 | -77.62 | 103.34 | 0.9765 | 338.4 | -50.1 | |
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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 |
| 0.34 | 1.63 | 0.29 | 1.38 | -6.62 | 275.54 | -53.28 | 100.43 | 0.8118 | 192.5 | 336.1 | |
| 0.00 | 0.95 | 0.00 | 0.94 | -14.07 | 270.82 | -58.00 | 108.17 | 0.8678 | 140.0 | 182.5 | |
| 0.00 | 0.95 | 0.00 | 0.91 | -9.51 | 270.81 | -58.01 | 102.97 | 0.8604 | 329.0 | 316.7 | |
| 0.00 | 0.86 | 0.00 | 0.84 | -9.59 | 270.50 | -58.32 | 103.00 | 0.8632 | 538.0 | 451.5 | |
| 0.00 | 1.38 | 0.00 | 1.61 | -17.00 | 266.17 | -62.65 | 110.36 | 0.9078 | 320.0 | 290.8 | |
| 11.01 | 65.46 | 15.09 | 90.15 | -14.09 | 261.53 | -67.29 | 106.37 | 0.9341 | 519.4 | 79.1 | |
| 0.00 | 3.78 | 0.00 | 5.69 | -13.67 | 259.45 | -69.37 | 105.61 | 0.9457 | -101.0 | -64.9 | |
| 0.00 | 1.03 | 0.00 | 1.60 | -11.36 | 258.46 | -70.37 | 103.05 | 0.9493 | 251.0 | 214.2 | |
| 0.00 | 4.90 | 0.00 | 12.57 | -16.10 | 251.30 | -77.52 | 107.06 | 0.9822 | -93.0 | -72.3 | |
| 0.52 | 1.72 | 0.97 | 3.23 | -9.32 | 254.83 | -73.99 | 100.52 | 0.9659 | -96.7 | -126.5 | |
| 21.51 | 143.65 | 48.83 | 331.15 | -12.22 | 252.45 | -76.37 | 103.24 | 0.9768 | 342.7 | 22.2 | |
| 0.00 | 2.06 | 0.00 | 13.92 | -12.74 | 243.73 | -85.09 | 103.02 | 0.9978 | -151.0 | -166.1 | |
| 0.00 | 0.26 | 0.00 | 5.44 | -13.41 | 241.04 | -87.79 | 103.51 | 0.9998 | 169.0 | 182.3 | |
| 0.00 | 28.90 | 0.00 | 204.92 | -11.57 | 244.53 | -84.29 | 101.90 | 0.9966 | -350.0 | -204.3 | |
| 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. | |