SDO HMI 2011-10-27 04:59:00 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 |
| 259.30 | 1386.66 | 133.78 | 713.81 | 7.71 | 250.55 | -14.34 | 78.62 | 0.2509 | -259.7 | -127.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-10-27 04:59:00 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 | 1.39 | 0.00 | 0.70 | 16.24 | 264.23 | -0.66 | 3.20 | 0.1980 | 844.0 | 649.4 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 13.54 | 261.75 | -3.13 | 19.44 | 0.1604 | -999.0 | -753.5 | |
| 0.00 | 2.00 | 0.00 | 1.00 | 9.09 | 259.83 | -5.05 | 49.75 | 0.1144 | -834.0 | -568.0 | |
| 0.00 | 1.56 | 0.00 | 0.78 | 9.62 | 259.40 | -5.48 | 48.64 | 0.1261 | -966.0 | -698.8 | |
| 0.00 | 2.34 | 0.00 | 1.18 | 12.16 | 258.47 | -6.42 | 40.68 | 0.1684 | -913.0 | -703.5 | |
| 0.00 | 1.22 | 0.00 | 0.61 | 13.17 | 256.74 | -8.14 | 43.59 | 0.2009 | -892.0 | -661.1 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 12.74 | 256.66 | -8.22 | 45.39 | 0.1967 | -817.0 | -717.5 | |
| 1.04 | 785.79 | 0.52 | 394.65 | 5.65 | 256.01 | -8.87 | 84.68 | 0.1548 | -1163.4 | -488.0 | |
| 115.32 | -8.00 | 57.87 | -8.00 | 6.33 | 255.73 | -9.16 | 80.57 | 0.1610 | -1665.3 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 11.04 | 254.66 | -10.23 | 58.11 | 0.2062 | -824.0 | -647.0 | |
| 11.98 | -8.00 | 6.03 | -8.00 | 6.08 | 254.55 | -10.34 | 82.94 | 0.1806 | -1198.5 | 999999 | |
| 3.56 | -8.00 | 1.79 | -8.00 | 5.81 | 254.55 | -10.33 | 84.42 | 0.1801 | -1100.1 | 999999 | |
| 4.78 | -8.00 | 2.41 | -8.00 | 6.67 | 254.47 | -10.41 | 79.74 | 0.1832 | -784.7 | 999999 | |
| 0.00 | 3.82 | 0.00 | 1.94 | 12.02 | 254.28 | -10.60 | 55.10 | 0.2205 | -904.0 | -796.0 | |
| 1.91 | 2.34 | 0.96 | 1.18 | 3.87 | 254.34 | -10.54 | 95.12 | 0.1842 | 919.5 | 980.4 | |
| 0.00 | 1.39 | 0.00 | 0.70 | 4.79 | 254.02 | -10.86 | 90.08 | 0.1886 | -731.0 | -591.6 | |
| 0.00 | 1.48 | 0.00 | 0.74 | 4.61 | 253.96 | -10.92 | 91.02 | 0.1897 | -809.0 | -715.8 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 7.52 | 253.78 | -11.10 | 76.01 | 0.1976 | -827.0 | -609.2 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 11.29 | 253.60 | -11.29 | 59.49 | 0.2238 | -863.0 | -659.2 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 7.61 | 253.56 | -11.32 | 75.82 | 0.2016 | -779.0 | -561.1 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 11.42 | 252.35 | -12.54 | 61.46 | 0.2433 | -992.0 | -803.9 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 6.78 | 252.27 | -12.62 | 80.81 | 0.2207 | -914.0 | -618.8 | |
| 3.30 | 4.34 | 1.67 | 2.20 | 5.44 | 252.24 | -12.65 | 86.93 | 0.2193 | -973.8 | -785.9 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 6.30 | 252.16 | -12.73 | 83.03 | 0.2216 | -878.0 | -682.7 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 6.09 | 252.07 | -12.81 | 84.01 | 0.2228 | -830.0 | -574.5 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 11.35 | 251.76 | -13.12 | 62.75 | 0.2516 | -778.0 | -628.8 | |
| 0.00 | 1.74 | 0.00 | 0.88 | 6.32 | 251.66 | -13.22 | 83.15 | 0.2300 | -747.0 | -478.4 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 9.51 | 251.19 | -13.70 | 70.45 | 0.2490 | -844.0 | -600.3 | |
| 4.17 | 7.38 | 2.13 | 3.76 | 5.48 | 251.10 | -13.78 | 86.92 | 0.2386 | -1055.4 | -691.1 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 8.11 | 249.93 | -14.95 | 76.99 | 0.2633 | -907.0 | -783.8 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 5.71 | 249.17 | -15.71 | 86.30 | 0.2712 | 808.0 | 586.9 | |
| 0.00 | 1.48 | 0.00 | 0.76 | 8.06 | 248.94 | -15.95 | 77.86 | 0.2795 | -693.0 | -571.6 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 7.22 | 247.87 | -17.01 | 81.29 | 0.2949 | 821.0 | 648.2 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 7.31 | 247.62 | -17.27 | 81.12 | 0.2993 | 912.0 | 728.2 | |
| 0.00 | 4.25 | 0.00 | 2.21 | 7.01 | 247.57 | -17.32 | 82.13 | 0.2996 | 1046.0 | 751.5 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 7.39 | 247.39 | -17.49 | 80.93 | 0.3032 | 956.0 | 794.7 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 8.25 | 246.98 | -17.91 | 78.36 | 0.3121 | 1171.0 | 1046.6 | |
| 0.00 | 1.39 | 0.00 | 0.72 | 9.02 | 246.91 | -17.98 | 75.97 | 0.3156 | 1033.0 | 894.2 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 8.93 | 246.69 | -18.19 | 76.40 | 0.3188 | 971.0 | 713.7 | |
| 0.00 | 1.56 | 0.00 | 0.82 | 8.83 | 246.47 | -18.41 | 76.82 | 0.3219 | 792.0 | 574.8 | |
| 0.00 | 2.17 | 0.00 | 1.14 | 9.22 | 246.36 | -18.53 | 75.72 | 0.3251 | 869.0 | 760.8 | |
| 1.56 | 9.12 | 0.82 | 4.79 | 9.65 | 245.79 | -19.09 | 74.80 | 0.3357 | 986.9 | 793.8 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 9.26 | 245.65 | -19.23 | 76.03 | 0.3365 | 827.0 | 583.0 | |
| 1.48 | 4.60 | 0.78 | 2.42 | 10.27 | 245.56 | -19.32 | 73.16 | 0.3417 | 909.2 | 512.1 | |
| 10.94 | 522.50 | 5.83 | 278.95 | 10.98 | 244.02 | -20.86 | 72.30 | 0.3685 | 1144.1 | 389.3 | |
| 0.87 | -45.00 | 0.46 | -45.00 | 10.08 | 244.02 | -20.86 | 74.69 | 0.3651 | 925.7 | 999999 | |
| 1.22 | -45.00 | 0.65 | -45.00 | 9.36 | 244.04 | -20.85 | 76.63 | 0.3625 | 1108.2 | 999999 | |
| 9.38 | -45.00 | 4.99 | -45.00 | 9.68 | 243.85 | -21.03 | 75.85 | 0.3664 | 1217.6 | 999999 | |
| 9.55 | -45.00 | 5.10 | -45.00 | 10.39 | 243.42 | -21.47 | 74.23 | 0.3757 | 1096.6 | 999999 | |
| 26.31 | -45.00 | 14.02 | -45.00 | 8.57 | 243.47 | -21.41 | 79.03 | 0.3693 | 1294.4 | 999999 | |
| 1.48 | -45.00 | 0.79 | -45.00 | 10.20 | 243.27 | -21.62 | 74.79 | 0.3773 | 853.4 | 999999 | |
| 50.45 | -45.00 | 26.96 | -45.00 | 9.63 | 243.18 | -21.71 | 76.33 | 0.3769 | 1231.3 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 6.17 | 242.20 | -22.68 | 85.69 | 0.3861 | 712.0 | 593.4 | |
| 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. | |