SDO HMI 2014-07-06 18:00:40 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 |
| 108.85 | 659.45 | 59.67 | 361.32 | -19.27 | 255.67 | 11.03 | 205.00 | 0.4279 | 696.6 | 334.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-06 18:00:40 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 | 1.36 | 0.00 | 0.84 | -22.95 | 270.07 | 25.43 | 221.99 | 0.5933 | -678.0 | -556.5 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -21.46 | 267.41 | 22.77 | 220.83 | 0.5531 | 760.0 | 559.8 | |
| 0.00 | 3.09 | 0.00 | 1.81 | -20.92 | 266.06 | 21.42 | 219.84 | 0.5345 | 798.0 | 667.3 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -20.77 | 265.48 | 20.84 | 219.28 | 0.5274 | 831.0 | 650.8 | |
| 0.00 | 1.36 | 0.00 | 0.82 | -24.39 | 264.95 | 20.31 | 214.28 | 0.5633 | 682.0 | 483.7 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -20.49 | 263.50 | 18.86 | 216.92 | 0.5060 | 715.0 | 542.1 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -24.26 | 263.89 | 19.25 | 213.05 | 0.5533 | 564.0 | 535.4 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -20.12 | 263.01 | 18.37 | 216.69 | 0.4972 | 725.0 | 571.1 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -20.61 | 262.83 | 18.19 | 215.80 | 0.5014 | 650.0 | 488.9 | |
| 6.81 | 9.17 | 3.90 | 5.25 | -21.10 | 262.34 | 17.70 | 214.48 | 0.5030 | 906.1 | 590.9 | |
| 0.00 | 1.73 | 0.00 | 1.00 | -22.76 | 262.48 | 17.84 | 212.76 | 0.5242 | 798.0 | 624.0 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -22.59 | 262.25 | 17.61 | 212.62 | 0.5202 | 504.0 | 415.7 | |
| 0.00 | 2.18 | 0.00 | 1.24 | -21.09 | 261.86 | 17.22 | 213.77 | 0.4988 | 371.0 | 357.2 | |
| 0.00 | 1.73 | 0.00 | 1.00 | -23.13 | 262.11 | 17.47 | 211.83 | 0.5257 | -585.0 | -534.2 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -18.71 | 260.15 | 15.51 | 214.03 | 0.4545 | -736.0 | -623.7 | |
| 0.00 | 3.90 | 0.00 | 2.20 | -21.99 | 257.13 | 12.49 | 205.10 | 0.4749 | -924.0 | -801.0 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -21.91 | 256.66 | 12.02 | 204.33 | 0.4708 | -722.0 | -611.2 | |
| 0.00 | 1.73 | 0.00 | 0.96 | -21.57 | 256.13 | 11.49 | 203.70 | 0.4626 | -1052.0 | -802.0 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -21.56 | 255.82 | 11.18 | 203.15 | 0.4607 | -806.0 | -726.7 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -23.22 | 255.89 | 11.25 | 201.82 | 0.4845 | -953.0 | -759.2 | |
| 0.27 | 561.46 | 0.15 | 306.37 | -18.30 | 255.50 | 10.86 | 205.82 | 0.4124 | 1361.7 | 416.6 | |
| 92.15 | -21.00 | 50.29 | -21.00 | -18.90 | 255.50 | 10.86 | 205.18 | 0.4209 | 1471.3 | 999999 | |
| 1.18 | -21.00 | 0.65 | -21.00 | -19.62 | 255.52 | 10.88 | 204.45 | 0.4313 | 630.5 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -22.92 | 255.73 | 11.09 | 201.79 | 0.4792 | -749.0 | -605.7 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -21.93 | 255.42 | 10.78 | 202.08 | 0.4634 | 673.0 | 461.6 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -22.98 | 255.47 | 10.83 | 201.27 | 0.4786 | -734.0 | -653.6 | |
| 0.27 | -21.00 | 0.15 | -21.00 | -18.53 | 254.99 | 10.35 | 204.52 | 0.4122 | 1572.0 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -22.19 | 254.80 | 10.16 | 200.72 | 0.4637 | -835.0 | -727.9 | |
| 0.00 | 2.63 | 0.00 | 1.47 | -22.39 | 254.78 | 10.14 | 200.51 | 0.4665 | -501.0 | -519.5 | |
| 3.36 | 12.26 | 1.86 | 6.80 | -21.48 | 254.52 | 9.88 | 200.78 | 0.4519 | 868.8 | 232.7 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -21.01 | 254.49 | 9.85 | 201.12 | 0.4449 | 721.0 | 490.8 | |
| 3.54 | 7.99 | 1.98 | 4.47 | -22.59 | 254.46 | 9.82 | 199.76 | 0.4677 | -1038.9 | -666.3 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -22.12 | 254.23 | 9.59 | 199.70 | 0.4596 | 335.0 | 293.9 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -17.79 | 253.94 | 9.30 | 203.04 | 0.3947 | 926.0 | 691.2 | |
| 0.00 | 2.18 | 0.00 | 1.18 | -18.19 | 253.83 | 9.19 | 202.40 | 0.3998 | 306.0 | 230.8 | |
| 0.00 | 1.73 | 0.00 | 0.97 | -23.40 | 253.81 | 9.17 | 197.97 | 0.4762 | -710.0 | -384.4 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -20.96 | 253.56 | 8.92 | 199.33 | 0.4392 | -124.0 | -109.5 | |
| 0.00 | 1.54 | 0.00 | 0.83 | -18.57 | 252.81 | 8.17 | 199.78 | 0.3996 | -778.0 | -532.5 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -19.62 | 252.24 | 7.60 | 197.65 | 0.4125 | 856.0 | 737.0 | |
| 0.00 | 2.00 | 0.00 | 1.08 | -19.02 | 252.15 | 7.51 | 197.92 | 0.4030 | -853.0 | -726.4 | |
| 0.00 | 0.73 | 0.00 | 0.40 | -19.88 | 252.09 | 7.45 | 197.12 | 0.4158 | 746.0 | 583.0 | |
| 0.00 | 0.91 | 0.00 | 0.49 | -19.35 | 251.48 | 6.84 | 196.18 | 0.4048 | -882.0 | -627.1 | |
| 0.00 | 3.00 | 0.00 | 1.62 | -19.44 | 251.22 | 6.58 | 195.54 | 0.4052 | 227.0 | 227.5 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -20.37 | 251.13 | 6.49 | 194.71 | 0.4191 | -717.0 | -535.8 | |
| 1.27 | 3.27 | 0.69 | 1.77 | -19.14 | 250.98 | 6.34 | 195.21 | 0.3996 | -963.4 | -756.8 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -19.41 | 250.83 | 6.19 | 194.68 | 0.4030 | -783.0 | -670.3 | |
| 0.00 | 1.00 | 0.00 | 0.54 | -19.57 | 250.61 | 5.97 | 194.07 | 0.4047 | -813.0 | -649.5 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -24.29 | 250.03 | 5.39 | 190.43 | 0.4751 | -705.0 | -499.3 | |
| 0.00 | 2.36 | 0.00 | 1.28 | -19.70 | 249.70 | 5.06 | 191.94 | 0.4034 | -991.0 | -796.1 | |
| 0.00 | 0.82 | 0.00 | 0.44 | -20.19 | 248.90 | 4.26 | 189.87 | 0.4087 | -773.0 | -602.8 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -26.51 | 246.89 | 2.25 | 184.02 | 0.5026 | -697.0 | -527.8 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -24.86 | 245.92 | 1.28 | 182.44 | 0.4767 | -680.0 | -501.4 | |
| 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. | |