SDO HMI 2014-11-16 04:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.72 | 86.68 | 0.89 | 45.95 | -11.89 | 309.74 | 13.90 | 221.22 | 0.3505 | -74.2 | -101.5 | |
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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 |
| 0.00 | 1.12 | 0.00 | 0.63 | -13.42 | 320.30 | 24.46 | 235.77 | 0.4892 | 641.0 | 548.1 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -12.28 | 318.72 | 22.89 | 236.10 | 0.4598 | 505.0 | 511.9 | |
| 0.00 | 0.77 | 0.00 | 0.42 | -9.16 | 318.25 | 22.41 | 241.71 | 0.4293 | 850.0 | 723.0 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -9.82 | 317.81 | 21.97 | 239.87 | 0.4281 | 790.0 | 606.0 | |
| 0.00 | 0.77 | 0.00 | 0.43 | -11.90 | 317.90 | 22.06 | 235.87 | 0.4459 | 899.0 | 701.3 | |
| 0.00 | 1.38 | 0.00 | 0.75 | -10.09 | 317.63 | 21.79 | 239.12 | 0.4277 | 874.0 | 655.8 | |
| 0.00 | 2.24 | 0.00 | 1.24 | -12.54 | 317.83 | 21.99 | 234.57 | 0.4504 | 668.0 | 572.2 | |
| 0.00 | 1.29 | 0.00 | 0.71 | -10.88 | 317.37 | 21.53 | 237.22 | 0.4304 | 940.0 | 732.0 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -12.92 | 316.68 | 20.85 | 232.44 | 0.4394 | 658.0 | 500.5 | |
| 0.00 | 1.55 | 0.00 | 0.85 | -12.97 | 316.53 | 20.69 | 232.13 | 0.4380 | 754.0 | 545.9 | |
| 0.00 | 1.63 | 0.00 | 0.88 | -9.33 | 316.13 | 20.29 | 238.94 | 0.4013 | 886.0 | 738.6 | |
| 0.00 | 1.46 | 0.00 | 0.81 | -13.81 | 316.47 | 20.63 | 230.53 | 0.4451 | 432.0 | 461.2 | |
| 0.00 | 1.46 | 0.00 | 0.81 | -13.65 | 316.33 | 20.49 | 230.62 | 0.4419 | 849.0 | 645.6 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -13.74 | 316.07 | 20.23 | 230.12 | 0.4396 | 931.0 | 808.1 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -14.51 | 316.08 | 20.24 | 228.76 | 0.4473 | 688.0 | 535.6 | |
| 0.00 | 1.20 | 0.00 | 0.66 | -13.15 | 315.92 | 20.09 | 231.00 | 0.4322 | 933.0 | 808.6 | |
| 0.00 | 1.20 | 0.00 | 0.66 | -12.47 | 315.84 | 20.00 | 232.15 | 0.4247 | 832.0 | 731.7 | |
| 0.00 | 1.20 | 0.00 | 0.66 | -13.82 | 315.59 | 19.75 | 229.31 | 0.4347 | 750.0 | 555.9 | |
| 0.00 | 1.29 | 0.00 | 0.70 | -11.88 | 315.31 | 19.47 | 232.57 | 0.4125 | 844.0 | 708.7 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -11.96 | 314.61 | 18.77 | 231.41 | 0.4044 | 821.0 | 615.6 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -12.84 | 314.25 | 18.42 | 229.17 | 0.4088 | 1024.0 | 807.6 | |
| 0.00 | 1.81 | 0.00 | 0.97 | -12.20 | 312.77 | 16.94 | 228.07 | 0.3844 | 919.0 | 729.6 | |
| 0.00 | 3.27 | 0.00 | 1.75 | -12.14 | 312.36 | 16.52 | 227.50 | 0.3787 | 384.0 | 623.2 | |
| 0.00 | 1.81 | 0.00 | 0.99 | -16.58 | 312.66 | 16.82 | 220.16 | 0.4320 | 706.0 | 521.3 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -12.98 | 311.18 | 15.34 | 223.76 | 0.3743 | 849.0 | 709.6 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -10.76 | 310.21 | 14.37 | 226.44 | 0.3380 | 897.0 | 611.9 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -11.65 | 310.19 | 14.35 | 224.52 | 0.3478 | 822.0 | 701.3 | |
| 0.00 | 2.67 | 0.00 | 1.40 | -12.18 | 309.25 | 13.41 | 221.51 | 0.3436 | 101.0 | 200.3 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -12.24 | 308.82 | 12.98 | 220.48 | 0.3396 | -588.0 | -479.9 | |
| 0.00 | 1.38 | 0.00 | 0.72 | -12.72 | 307.57 | 11.73 | 216.76 | 0.3328 | -878.0 | -763.5 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -9.87 | 307.36 | 11.52 | 222.16 | 0.2945 | -871.0 | -737.1 | |
| 0.00 | 2.41 | 0.00 | 1.25 | -10.54 | 307.08 | 11.24 | 219.95 | 0.2997 | -527.0 | -539.6 | |
| 0.00 | 1.38 | 0.00 | 0.71 | -10.51 | 306.80 | 10.96 | 219.33 | 0.2963 | -775.0 | -585.0 | |
| 0.00 | 1.38 | 0.00 | 0.72 | -13.42 | 306.70 | 10.86 | 213.46 | 0.3339 | -778.0 | -685.7 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -13.38 | 306.54 | 10.70 | 213.13 | 0.3320 | -973.0 | -846.3 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -10.35 | 306.33 | 10.49 | 218.46 | 0.2894 | -892.0 | -739.6 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -10.41 | 306.06 | 10.22 | 217.60 | 0.2873 | -1020.0 | -874.5 | |
| 0.00 | 1.29 | 0.00 | 0.67 | -11.90 | 305.62 | 9.78 | 213.41 | 0.3032 | -878.0 | -693.0 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -10.86 | 305.46 | 9.62 | 215.01 | 0.2874 | -1063.0 | -915.0 | |
| 0.00 | 1.63 | 0.00 | 0.85 | -11.13 | 305.41 | 9.57 | 214.31 | 0.2907 | -948.0 | -805.2 | |
| 0.95 | 5.85 | 0.49 | 3.02 | -11.10 | 304.92 | 9.08 | 212.99 | 0.2856 | -1215.5 | -911.7 | |
| 0.77 | 8.86 | 0.40 | 4.58 | -11.34 | 304.68 | 8.84 | 211.85 | 0.2869 | -1200.4 | -940.6 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -10.61 | 304.63 | 8.79 | 213.12 | 0.2761 | -985.0 | -830.2 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -11.12 | 304.55 | 8.71 | 211.88 | 0.2827 | -983.0 | -765.5 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -10.57 | 304.44 | 8.61 | 212.64 | 0.2740 | -1013.0 | -817.3 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -10.05 | 304.10 | 8.26 | 212.63 | 0.2634 | -882.0 | -693.1 | |
| 0.00 | 1.12 | 0.00 | 0.57 | -9.32 | 303.99 | 8.15 | 213.86 | 0.2522 | -794.0 | -628.5 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -12.68 | 304.02 | 8.18 | 207.61 | 0.3008 | -1116.0 | -933.8 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -9.32 | 303.84 | 8.00 | 213.37 | 0.2507 | -840.0 | -577.8 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -8.99 | 303.77 | 7.93 | 213.90 | 0.2454 | -846.0 | -748.7 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -13.60 | 303.71 | 7.87 | 205.35 | 0.3122 | -683.0 | -589.2 | |
| 0.00 | 0.52 | 0.00 | 0.26 | -8.93 | 303.31 | 7.47 | 212.50 | 0.2402 | -265.0 | -416.7 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -12.58 | 303.19 | 7.35 | 205.32 | 0.2931 | -896.0 | -731.6 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -13.69 | 303.09 | 7.26 | 203.48 | 0.3093 | -805.0 | -663.3 | |
| 0.00 | 2.15 | 0.00 | 1.12 | -13.75 | 302.85 | 7.01 | 202.70 | 0.3086 | -939.0 | -661.9 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -14.76 | 300.20 | 4.36 | 193.75 | 0.3107 | -739.0 | -553.5 | |
| 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. | |