SDO HMI 2011-11-30 04:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.27 | 368.53 | 29.64 | 201.29 | 20.52 | 191.77 | 15.13 | 324.12 | 0.4222 | -94.1 | -127.9 | |
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back to the solar disc SDO HMI 2011-11-30 04:58:56 UT
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 |
| 35.56 | 225.69 | 19.51 | 123.89 | 19.35 | 194.73 | 18.08 | 317.10 | 0.4321 | -1376.5 | -449.8 | |
| 1.62 | -1.00 | 0.89 | -1.00 | 19.45 | 194.41 | 17.76 | 317.75 | 0.4297 | -1150.8 | 999999 | |
| 0.00 | 4.70 | 0.00 | 2.55 | 18.99 | 193.31 | 16.66 | 318.73 | 0.4129 | -489.0 | -712.5 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 21.05 | 193.41 | 16.76 | 321.89 | 0.4379 | -853.0 | -667.6 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 17.57 | 192.78 | 16.14 | 317.11 | 0.3910 | -787.0 | -599.6 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 20.62 | 192.86 | 16.22 | 322.11 | 0.4274 | -756.0 | -665.3 | |
| 0.00 | 3.16 | 0.00 | 1.73 | 20.24 | 192.79 | 16.14 | 321.64 | 0.4222 | -948.0 | -740.5 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 17.72 | 192.47 | 15.83 | 317.93 | 0.3894 | -695.0 | -637.4 | |
| 0.94 | 1.62 | 0.51 | 0.88 | 20.05 | 192.54 | 15.89 | 321.77 | 0.4175 | -954.5 | -737.9 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 19.40 | 192.24 | 15.60 | 321.22 | 0.4067 | 768.0 | 419.1 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 20.15 | 192.22 | 15.58 | 322.46 | 0.4155 | -945.0 | -754.0 | |
| 0.00 | 2.14 | 0.00 | 1.16 | 20.46 | 192.12 | 15.48 | 323.12 | 0.4184 | -744.0 | -726.3 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 20.78 | 191.96 | 15.31 | 323.88 | 0.4207 | -751.0 | -544.1 | |
| 0.00 | 2.65 | 0.00 | 1.44 | 20.27 | 191.84 | 15.20 | 323.32 | 0.4134 | -990.0 | -857.9 | |
| 0.00 | 2.22 | 0.00 | 1.21 | 21.13 | 191.31 | 14.66 | 325.54 | 0.4191 | -767.0 | -698.0 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 20.50 | 190.79 | 14.14 | 325.56 | 0.4064 | -935.0 | -695.9 | |
| 0.00 | 1.62 | 0.00 | 0.88 | 21.00 | 190.84 | 14.19 | 326.21 | 0.4133 | -895.0 | -669.9 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 20.62 | 190.80 | 14.15 | 325.72 | 0.4081 | -808.0 | -622.2 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 20.63 | 190.60 | 13.96 | 326.09 | 0.4064 | -232.0 | -272.8 | |
| 0.00 | 1.80 | 0.00 | 0.97 | 20.91 | 190.57 | 13.92 | 326.57 | 0.4097 | -717.0 | -587.0 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 21.48 | 189.15 | 12.51 | 330.05 | 0.4054 | 726.0 | 601.8 | |
| 0.00 | 2.56 | 0.00 | 1.40 | 22.98 | 188.24 | 11.59 | 333.68 | 0.4190 | 639.0 | 477.9 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 21.90 | 187.85 | 11.21 | 333.16 | 0.4012 | 864.0 | 637.6 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 21.74 | 187.68 | 11.03 | 333.33 | 0.3977 | 800.0 | 621.4 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 21.55 | 187.34 | 10.69 | 333.80 | 0.3926 | 731.0 | 607.8 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 21.52 | 186.85 | 10.21 | 334.79 | 0.3888 | 757.0 | 645.4 | |
| 5.98 | 6.92 | 3.23 | 3.73 | 22.06 | 186.86 | 10.21 | 335.40 | 0.3966 | 958.5 | 727.0 | |
| 2.05 | 24.71 | 1.11 | 13.35 | 22.66 | 186.65 | 10.00 | 336.52 | 0.4039 | 811.8 | 653.8 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 24.62 | 186.80 | 10.15 | 338.19 | 0.4330 | 686.0 | 609.1 | |
| 0.00 | 1.37 | 0.00 | 0.75 | 24.84 | 186.52 | 9.87 | 338.93 | 0.4347 | 854.0 | 686.2 | |
| 6.41 | -28.00 | 3.47 | -28.00 | 22.66 | 186.32 | 9.67 | 337.20 | 0.4018 | 948.8 | 999999 | |
| 0.00 | 1.71 | 0.00 | 0.92 | 21.68 | 186.22 | 9.57 | 336.35 | 0.3869 | 977.0 | 819.4 | |
| 0.00 | 2.82 | 0.00 | 1.52 | 22.03 | 186.18 | 9.53 | 336.82 | 0.3917 | 1007.0 | 813.2 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 21.08 | 186.12 | 9.47 | 335.89 | 0.3774 | 798.0 | 685.1 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 21.71 | 186.00 | 9.35 | 336.87 | 0.3859 | 839.0 | 664.5 | |
| 0.00 | 1.97 | 0.00 | 1.09 | 25.69 | 186.16 | 9.51 | 340.37 | 0.4450 | 615.0 | 503.4 | |
| 0.00 | 1.71 | 0.00 | 0.92 | 22.22 | 185.84 | 9.19 | 337.76 | 0.3923 | 840.0 | 722.9 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 23.97 | 185.89 | 9.25 | 339.37 | 0.4185 | 744.0 | 618.4 | |
| 0.00 | 2.48 | 0.00 | 1.32 | 20.17 | 185.52 | 8.87 | 336.19 | 0.3601 | 969.0 | 744.7 | |
| 0.00 | 4.10 | 0.00 | 2.23 | 23.81 | 185.68 | 9.04 | 339.65 | 0.4150 | 664.0 | 512.6 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 22.70 | 185.58 | 8.93 | 338.81 | 0.3978 | 945.0 | 749.6 | |
| 1.71 | 23.17 | 0.92 | 12.53 | 22.92 | 185.20 | 8.55 | 339.83 | 0.3990 | 1007.1 | 802.9 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 25.63 | 185.29 | 8.64 | 341.98 | 0.4397 | 755.0 | 675.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 19.89 | 184.77 | 8.12 | 337.66 | 0.3512 | 858.0 | 678.4 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 26.18 | 184.90 | 8.25 | 343.15 | 0.4461 | 708.0 | 584.7 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 22.76 | 184.64 | 7.99 | 340.90 | 0.3936 | 957.0 | 800.6 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 26.05 | 184.85 | 8.21 | 343.14 | 0.4439 | 827.0 | 689.9 | |
| 0.00 | 9.66 | 0.00 | 5.23 | 23.56 | 184.53 | 7.88 | 341.85 | 0.4051 | 637.0 | 671.9 | |
| 0.00 | 2.48 | 0.00 | 1.36 | 25.37 | 184.57 | 7.93 | 343.18 | 0.4325 | 1049.0 | 915.9 | |
| 0.00 | 1.37 | 0.00 | 0.75 | 25.53 | 184.49 | 7.84 | 343.47 | 0.4345 | 718.0 | 644.6 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 22.29 | 184.03 | 7.39 | 341.84 | 0.3833 | 839.0 | 647.0 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 21.24 | 183.15 | 6.50 | 343.02 | 0.3629 | 887.0 | 711.3 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 25.34 | 182.89 | 6.24 | 346.57 | 0.4251 | 652.0 | 454.6 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 28.47 | 180.13 | 3.48 | 353.39 | 0.4658 | 555.0 | 427.9 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 27.93 | 180.08 | 3.43 | 353.33 | 0.4575 | 493.0 | 449.5 | |
| 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. | |