SDO HMI 2011-06-03 05:59:10 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 83.54 | 441.71 | 44.42 | 234.93 | -21.45 | 36.42 | 2.48 | 186.59 | 0.3636 | 410.7 | 247.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-03 05:59:10 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 | 0.99 | 0.00 | 0.54 | -24.10 | 40.74 | 6.80 | 195.07 | 0.4174 | 788.0 | 587.5 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -22.51 | 40.46 | 6.52 | 195.60 | 0.3919 | 866.0 | 676.0 | |
| 0.00 | 2.08 | 0.00 | 1.11 | -21.08 | 39.74 | 5.80 | 194.98 | 0.3665 | 779.0 | 713.7 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -24.20 | 39.27 | 5.33 | 191.88 | 0.4135 | 755.0 | 569.5 | |
| 8.77 | 89.89 | 4.61 | 47.21 | -19.17 | 39.02 | 5.08 | 194.60 | 0.3333 | 1374.7 | 563.4 | |
| 0.00 | 3.89 | 0.00 | 2.10 | -23.21 | 39.10 | 5.16 | 192.05 | 0.3974 | 1003.0 | 715.4 | |
| 0.90 | 2.44 | 0.49 | 1.33 | -24.07 | 39.10 | 5.16 | 191.58 | 0.4109 | 793.1 | 725.2 | |
| 4.88 | -5.00 | 2.57 | -5.00 | -19.43 | 38.81 | 4.86 | 193.81 | 0.3366 | 1142.5 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -24.60 | 38.95 | 5.01 | 190.98 | 0.4187 | 647.0 | 561.4 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -23.80 | 38.89 | 4.95 | 191.25 | 0.4061 | 910.0 | 739.8 | |
| 8.32 | 10.76 | 4.52 | 5.85 | -24.23 | 38.81 | 4.86 | 190.85 | 0.4126 | 912.0 | 625.6 | |
| 1.36 | -5.00 | 0.71 | -5.00 | -18.98 | 38.60 | 4.66 | 193.57 | 0.3285 | 957.3 | 999999 | |
| 3.98 | -5.00 | 2.09 | -5.00 | -19.33 | 38.54 | 4.60 | 193.16 | 0.3340 | 1150.8 | 999999 | |
| 0.00 | 8.14 | 0.00 | 4.40 | -23.44 | 38.64 | 4.70 | 190.89 | 0.3996 | 891.0 | 851.5 | |
| 0.00 | 2.26 | 0.00 | 1.22 | -23.87 | 38.66 | 4.72 | 190.71 | 0.4064 | 909.0 | 779.8 | |
| 0.00 | 1.45 | 0.00 | 0.79 | -24.67 | 38.52 | 4.58 | 190.02 | 0.4185 | 797.0 | 578.6 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -24.37 | 38.44 | 4.50 | 190.00 | 0.4136 | 657.0 | 473.5 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -19.33 | 38.25 | 4.31 | 192.36 | 0.3329 | 980.0 | 786.8 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -24.07 | 38.36 | 4.42 | 189.96 | 0.4087 | 922.0 | 779.4 | |
| 0.00 | 1.54 | 0.00 | 0.84 | -24.50 | 38.31 | 4.37 | 189.65 | 0.4153 | 671.0 | 401.9 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -24.23 | 38.30 | 4.36 | 189.75 | 0.4111 | 628.0 | 430.0 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -19.36 | 38.03 | 4.09 | 191.71 | 0.3327 | 910.0 | 666.2 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -20.01 | 38.04 | 4.10 | 191.35 | 0.3431 | 495.0 | 484.7 | |
| 1.18 | 1.72 | 0.64 | 0.93 | -24.03 | 37.93 | 3.99 | 189.02 | 0.4070 | 739.4 | 774.3 | |
| 0.00 | 2.89 | 0.00 | 1.52 | -19.46 | 37.64 | 3.70 | 190.58 | 0.3330 | 753.0 | 610.2 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -19.17 | 37.57 | 3.63 | 190.55 | 0.3281 | 924.0 | 710.4 | |
| 0.99 | 7.23 | 0.52 | 3.79 | -19.40 | 37.22 | 3.28 | 189.43 | 0.3308 | 1052.5 | 884.2 | |
| 6.33 | 8.05 | 3.34 | 4.25 | -20.43 | 37.11 | 3.17 | 188.62 | 0.3473 | 979.8 | 726.1 | |
| 0.00 | 2.62 | 0.00 | 1.38 | -19.36 | 36.96 | 3.02 | 188.71 | 0.3296 | 1154.0 | 898.5 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -19.04 | 36.92 | 2.98 | 188.76 | 0.3242 | 952.0 | 806.7 | |
| 0.00 | 2.17 | 0.00 | 1.14 | -19.36 | 36.74 | 2.79 | 188.07 | 0.3290 | 951.0 | 862.6 | |
| 0.00 | 3.35 | 0.00 | 1.76 | -20.20 | 36.72 | 2.78 | 187.66 | 0.3427 | 1158.0 | 913.4 | |
| 1.90 | 1.99 | 0.99 | 1.04 | -19.20 | 36.51 | 2.57 | 187.49 | 0.3259 | 1005.2 | 948.0 | |
| 0.45 | 4.70 | 0.24 | 2.48 | -20.49 | 36.43 | 2.49 | 186.77 | 0.3468 | 1125.8 | 760.9 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -24.27 | 36.40 | 2.46 | 185.53 | 0.4076 | -857.0 | -711.0 | |
| 0.90 | 137.09 | 0.48 | 72.87 | -21.11 | 36.31 | 2.37 | 186.24 | 0.3567 | 682.9 | 378.5 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -19.04 | 36.18 | 2.24 | 186.61 | 0.3226 | 855.0 | 805.9 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -23.80 | 36.26 | 2.32 | 185.33 | 0.4000 | -887.0 | -776.5 | |
| 4.79 | 7.60 | 2.53 | 4.00 | -20.33 | 36.07 | 2.13 | 185.85 | 0.3435 | 1081.0 | 746.6 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -19.24 | 36.06 | 2.12 | 186.17 | 0.3255 | 773.0 | 676.9 | |
| 4.88 | -36.00 | 2.58 | -36.00 | -20.72 | 35.98 | 2.04 | 185.48 | 0.3497 | 1116.4 | 999999 | |
| 6.78 | -36.00 | 3.59 | -36.00 | -21.05 | 35.95 | 2.01 | 185.31 | 0.3550 | 1144.6 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -23.31 | 35.98 | 2.04 | 184.82 | 0.3916 | 599.0 | 515.6 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -19.75 | 35.80 | 1.86 | 185.29 | 0.3336 | 989.0 | 697.2 | |
| 7.51 | -36.00 | 3.99 | -36.00 | -21.70 | 35.80 | 1.86 | 184.74 | 0.3654 | 1138.2 | 999999 | |
| 1.72 | -36.00 | 0.91 | -36.00 | -21.40 | 35.76 | 1.82 | 184.72 | 0.3606 | 1181.6 | 999999 | |
| 0.00 | 4.34 | 0.00 | 2.34 | -23.47 | 35.62 | 1.68 | 183.93 | 0.3938 | 142.0 | 76.5 | |
| 4.43 | -36.00 | 2.36 | -36.00 | -21.76 | 35.57 | 1.63 | 184.15 | 0.3662 | 957.9 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -21.11 | 35.56 | 1.62 | 184.27 | 0.3555 | 858.0 | 651.5 | |
| 0.00 | 0.45 | 0.00 | 0.24 | -23.24 | 35.55 | 1.61 | 183.81 | 0.3901 | 648.0 | 465.0 | |
| 0.00 | 1.99 | 0.00 | 1.05 | -20.92 | 35.30 | 1.36 | 183.62 | 0.3520 | 887.0 | 590.9 | |
| 10.67 | 71.35 | 5.75 | 38.42 | -23.60 | 34.53 | 0.59 | 181.37 | 0.3952 | -1197.9 | -317.7 | |
| 2.80 | -52.00 | 1.51 | -52.00 | -23.84 | 34.46 | 0.52 | 181.20 | 0.3989 | -850.6 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -23.01 | 34.10 | 0.15 | 180.37 | 0.3855 | 635.0 | 449.6 | |
| 0.00 | 1.63 | 0.00 | 0.88 | -24.20 | 33.93 | -0.01 | 179.98 | 0.4046 | -950.0 | -754.3 | |
| 0.00 | 3.80 | 0.00 | 2.01 | -21.14 | 33.80 | -0.14 | 179.63 | 0.3551 | -918.0 | -843.4 | |
| 0.00 | 4.61 | 0.00 | 2.45 | -21.86 | 33.64 | -0.31 | 179.22 | 0.3668 | -1106.0 | -911.3 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -21.24 | 33.57 | -0.37 | 179.03 | 0.3567 | -866.0 | -742.2 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -24.40 | 33.46 | -0.48 | 178.93 | 0.4079 | -709.0 | -557.2 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -19.53 | 33.48 | -0.46 | 178.67 | 0.3285 | -985.0 | -787.8 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -22.19 | 33.34 | -0.60 | 178.50 | 0.3723 | -901.0 | -684.1 | |
| 0.00 | 1.45 | 0.00 | 0.78 | -23.24 | 33.30 | -0.64 | 178.48 | 0.3893 | -887.0 | -847.4 | |
| 0.00 | 2.26 | 0.00 | 1.20 | -21.53 | 33.28 | -0.66 | 178.28 | 0.3616 | -827.0 | -684.7 | |
| 0.00 | 1.63 | 0.00 | 0.86 | -21.05 | 33.21 | -0.73 | 178.07 | 0.3537 | -838.0 | -673.4 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -22.68 | 33.11 | -0.83 | 177.97 | 0.3804 | -812.0 | -667.5 | |
| 0.00 | 2.26 | 0.00 | 1.20 | -21.27 | 33.08 | -0.86 | 177.75 | 0.3575 | -872.0 | -703.4 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -21.89 | 33.05 | -0.90 | 177.73 | 0.3676 | -887.0 | -656.1 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -21.18 | 32.89 | -1.05 | 177.23 | 0.3560 | -795.0 | -581.9 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -22.91 | 32.81 | -1.13 | 177.27 | 0.3843 | -840.0 | -638.7 | |
| 0.00 | 2.98 | 0.00 | 1.57 | -19.98 | 32.80 | -1.14 | 176.79 | 0.3364 | -855.0 | -682.5 | |
| 0.00 | 1.81 | 0.00 | 0.96 | -21.99 | 32.72 | -1.22 | 176.91 | 0.3695 | -884.0 | -647.8 | |
| 0.00 | 1.18 | 0.00 | 0.63 | -21.76 | 32.69 | -1.25 | 176.80 | 0.3658 | -888.0 | -662.6 | |
| 0.00 | 3.62 | 0.00 | 1.92 | -21.37 | 32.30 | -1.64 | 175.73 | 0.3598 | -807.0 | -700.5 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -22.48 | 31.73 | -2.22 | 174.56 | 0.3786 | -649.0 | -470.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |