SDO HMI 2011-11-28 17:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.44 | 396.05 | 39.09 | 208.01 | 19.88 | 191.97 | -3.91 | 10.44 | 0.3309 | -208.9 | -152.5 | |
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back to the solar disc SDO HMI 2011-11-28 17:58:56 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 |
| 0.00 | 2.73 | 0.00 | 1.43 | 20.38 | 196.65 | 0.77 | 357.80 | 0.3296 | -812.0 | -664.2 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 21.23 | 195.93 | 0.05 | 359.88 | 0.3434 | -891.0 | -705.9 | |
| 0.00 | 2.05 | 0.00 | 1.08 | 20.47 | 194.92 | -0.96 | 2.74 | 0.3313 | -882.0 | -758.1 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 17.55 | 194.84 | -1.04 | 3.53 | 0.2828 | -814.0 | -564.8 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 22.05 | 194.81 | -1.07 | 2.79 | 0.3573 | -760.0 | -637.2 | |
| 25.64 | 223.33 | 13.32 | 116.10 | 18.73 | 194.68 | -1.20 | 3.79 | 0.3026 | -1515.6 | -478.2 | |
| 17.52 | -6.00 | 9.12 | -6.00 | 19.07 | 194.49 | -1.39 | 4.29 | 0.3085 | -1223.2 | 999999 | |
| 3.42 | -6.00 | 1.77 | -6.00 | 18.08 | 194.09 | -1.79 | 5.85 | 0.2926 | -1024.2 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 20.91 | 194.00 | -1.89 | 5.21 | 0.3396 | -629.0 | -460.2 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 19.29 | 193.77 | -2.12 | 6.42 | 0.3132 | -680.0 | -486.8 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 19.88 | 193.73 | -2.16 | 6.31 | 0.3230 | -746.0 | -522.4 | |
| 0.00 | 2.31 | 0.00 | 1.21 | 19.60 | 193.51 | -2.37 | 7.05 | 0.3188 | -801.0 | -660.1 | |
| 0.00 | 2.31 | 0.00 | 1.20 | 19.32 | 193.42 | -2.46 | 7.44 | 0.3144 | -819.0 | -675.9 | |
| 0.00 | 0.68 | 0.00 | 0.35 | 17.71 | 193.41 | -2.47 | 8.24 | 0.2878 | -944.0 | -728.0 | |
| 0.00 | 2.22 | 0.00 | 1.15 | 17.55 | 193.29 | -2.59 | 8.72 | 0.2855 | -1029.0 | -801.0 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 19.85 | 193.07 | -2.82 | 8.24 | 0.3239 | -788.0 | -548.2 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 21.07 | 192.73 | -3.16 | 8.61 | 0.3447 | -787.0 | -650.8 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 21.03 | 192.57 | -3.31 | 9.05 | 0.3445 | -759.0 | -589.3 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 20.19 | 192.30 | -3.58 | 10.22 | 0.3315 | -702.0 | -639.7 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 13.22 | 192.16 | -3.72 | 16.93 | 0.2181 | 751.0 | 558.1 | |
| 0.00 | 6.07 | 0.00 | 3.19 | 20.16 | 191.64 | -4.24 | 12.08 | 0.3331 | -765.0 | -768.1 | |
| 0.00 | 7.18 | 0.00 | 3.78 | 20.37 | 191.10 | -4.78 | 13.41 | 0.3386 | -865.0 | -745.3 | |
| 0.00 | 2.39 | 0.00 | 1.23 | 15.31 | 191.23 | -4.65 | 17.81 | 0.2567 | -975.0 | -670.2 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 19.53 | 190.34 | -5.55 | 16.18 | 0.3284 | -698.0 | -531.8 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 21.09 | 190.02 | -5.86 | 15.65 | 0.3544 | -917.0 | -686.2 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 20.53 | 189.82 | -6.06 | 16.65 | 0.3465 | 857.0 | 612.4 | |
| 0.00 | 2.48 | 0.00 | 1.28 | 16.38 | 189.85 | -6.04 | 21.11 | 0.2814 | -733.0 | -696.6 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 20.47 | 189.61 | -6.28 | 17.27 | 0.3466 | 665.0 | 463.4 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 16.16 | 189.64 | -6.25 | 22.07 | 0.2794 | -802.0 | -620.1 | |
| 0.00 | 3.59 | 0.00 | 1.90 | 20.62 | 189.28 | -6.60 | 17.95 | 0.3506 | 863.0 | 552.5 | |
| 2.05 | 4.44 | 1.08 | 2.35 | 20.59 | 188.96 | -6.92 | 18.78 | 0.3517 | 900.0 | 844.2 | |
| 0.00 | 4.62 | 0.00 | 2.47 | 22.16 | 188.60 | -7.28 | 18.19 | 0.3778 | 806.0 | 897.1 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 20.40 | 188.66 | -7.23 | 19.75 | 0.3505 | 871.0 | 724.9 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 23.12 | 187.96 | -7.92 | 18.77 | 0.3955 | 559.0 | 578.9 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 22.26 | 188.01 | -7.87 | 19.44 | 0.3823 | 612.0 | 506.9 | |
| 11.97 | 61.71 | 6.39 | 32.90 | 21.59 | 187.63 | -8.25 | 20.97 | 0.3744 | 1219.4 | 595.1 | |
| 2.65 | -36.00 | 1.41 | -36.00 | 21.43 | 187.42 | -8.46 | 21.63 | 0.3733 | 1093.4 | 999999 | |
| 3.42 | 20.77 | 1.83 | 11.13 | 21.97 | 187.29 | -8.59 | 21.36 | 0.3821 | 916.8 | 743.5 | |
| 6.15 | -38.00 | 3.30 | -38.00 | 22.06 | 187.06 | -8.82 | 21.78 | 0.3848 | 954.3 | 999999 | |
| 1.62 | -38.00 | 0.87 | -38.00 | 21.75 | 187.01 | -8.87 | 22.21 | 0.3804 | 955.4 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 24.01 | 186.80 | -9.09 | 20.43 | 0.4151 | 850.0 | 749.9 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 20.96 | 186.97 | -8.92 | 23.20 | 0.3691 | 686.0 | 589.2 | |
| 0.00 | 2.73 | 0.00 | 1.47 | 21.84 | 186.59 | -9.29 | 23.06 | 0.3844 | 811.0 | 634.9 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 22.13 | 186.41 | -9.47 | 23.14 | 0.3897 | 949.0 | 747.9 | |
| 0.00 | 3.59 | 0.00 | 1.93 | 22.38 | 186.20 | -9.69 | 23.32 | 0.3948 | 835.0 | 728.7 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 25.98 | 185.88 | -10.00 | 20.44 | 0.4488 | 689.0 | 590.5 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 24.39 | 185.75 | -10.13 | 22.16 | 0.4267 | 887.0 | 755.0 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 20.89 | 185.94 | -9.94 | 25.59 | 0.3750 | 904.0 | 717.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 19.02 | 186.06 | -9.82 | 27.81 | 0.3472 | 729.0 | 467.4 | |
| 0.00 | 2.39 | 0.00 | 1.31 | 24.42 | 185.32 | -10.57 | 22.96 | 0.4298 | 709.0 | 640.2 | |
| 0.00 | 1.62 | 0.00 | 0.90 | 25.16 | 185.22 | -10.66 | 22.42 | 0.4410 | 785.0 | 567.4 | |
| 0.00 | 3.68 | 0.00 | 2.03 | 24.97 | 184.61 | -11.28 | 23.75 | 0.4420 | 903.0 | 670.6 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 23.04 | 184.38 | -11.50 | 26.26 | 0.4164 | 817.0 | 636.5 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 22.85 | 184.27 | -11.61 | 26.71 | 0.4145 | 769.0 | 591.8 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 22.88 | 184.13 | -11.75 | 26.93 | 0.4159 | 708.0 | 549.9 | |
| 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. | |