| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.22 | 250.70 | 50.55 | 216.84 | -16.70 | 250.89 | 50.21 | 243.98 | 0.8184 | -138.3 | -59.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-29 19:00:33 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 |
| 10.57 | 103.10 | 10.33 | 99.35 | -17.86 | 255.61 | 54.93 | 244.64 | 0.8641 | 554.6 | 198.7 | |
| 1.50 | -1.00 | 1.47 | -1.00 | -18.14 | 255.52 | 54.84 | 244.30 | 0.8642 | 491.2 | 999999 | |
| 0.88 | -1.00 | 0.85 | -1.00 | -17.86 | 255.01 | 54.33 | 244.41 | 0.8593 | 554.1 | 999999 | |
| 6.70 | -1.00 | 6.34 | -1.00 | -17.24 | 254.63 | 53.94 | 244.96 | 0.8543 | 697.0 | 999999 | |
| 1.15 | -1.00 | 1.07 | -1.00 | -16.89 | 254.37 | 53.69 | 245.25 | 0.8511 | 625.0 | 999999 | |
| 0.00 | 1.06 | 0.00 | 1.02 | -18.27 | 254.87 | 54.19 | 243.91 | 0.8594 | 401.0 | 425.4 | |
| 3.52 | -1.00 | 3.32 | -1.00 | -17.34 | 254.35 | 53.67 | 244.74 | 0.8523 | 806.8 | 999999 | |
| 0.00 | 1.32 | 0.00 | 1.22 | -16.72 | 253.93 | 53.25 | 245.27 | 0.8469 | 627.0 | 638.7 | |
| 0.00 | 0.62 | 0.00 | 0.59 | -18.52 | 254.71 | 54.03 | 243.58 | 0.8589 | 463.0 | 433.9 | |
| 0.00 | 1.32 | 0.00 | 1.21 | -16.60 | 253.67 | 52.99 | 245.31 | 0.8443 | 582.0 | 473.2 | |
| 0.00 | 2.56 | 0.00 | 2.36 | -17.11 | 253.61 | 52.93 | 244.72 | 0.8455 | 694.0 | 572.8 | |
| 0.00 | 1.41 | 0.00 | 1.30 | -17.35 | 253.45 | 52.77 | 244.38 | 0.8449 | 434.0 | 401.6 | |
| 0.00 | 0.44 | 0.00 | 0.40 | -16.94 | 253.18 | 52.50 | 244.74 | 0.8413 | 658.0 | 622.2 | |
| 0.00 | 0.97 | 0.00 | 0.88 | -17.14 | 252.95 | 52.27 | 244.42 | 0.8400 | 490.0 | 516.4 | |
| 0.88 | 1.59 | 0.77 | 1.39 | -16.37 | 251.74 | 51.06 | 244.80 | 0.8269 | 497.6 | 480.8 | |
| 0.00 | 3.35 | 0.00 | 2.89 | -15.60 | 251.42 | 50.74 | 245.55 | 0.8214 | 522.0 | 502.9 | |
| 0.00 | 1.41 | 0.00 | 1.23 | -16.71 | 251.52 | 50.83 | 244.33 | 0.8261 | 133.0 | 262.9 | |
| 0.00 | 1.15 | 0.00 | 0.97 | -17.23 | 249.89 | 49.21 | 243.03 | 0.8135 | -318.0 | -205.7 | |
| 0.00 | 2.11 | 0.00 | 1.75 | -16.60 | 249.05 | 48.36 | 243.38 | 0.8034 | -409.0 | -335.2 | |
| 0.00 | 1.59 | 0.00 | 1.31 | -16.74 | 248.81 | 48.13 | 243.11 | 0.8018 | -330.0 | -211.3 | |
| 0.00 | 1.23 | 0.00 | 1.04 | -17.91 | 249.13 | 48.44 | 241.91 | 0.8093 | -367.0 | -287.8 | |
| 0.00 | 3.00 | 0.00 | 2.42 | -15.50 | 248.27 | 47.59 | 244.32 | 0.7917 | -566.0 | -377.0 | |
| 0.00 | 0.79 | 0.00 | 0.66 | -17.77 | 249.03 | 48.34 | 242.03 | 0.8078 | -515.0 | -471.7 | |
| 0.00 | 1.41 | 0.00 | 1.17 | -17.47 | 248.92 | 48.24 | 242.32 | 0.8056 | -238.0 | -249.9 | |
| 0.00 | 0.97 | 0.00 | 0.79 | -16.51 | 248.40 | 47.72 | 243.19 | 0.7970 | -441.0 | -338.3 | |
| 0.00 | 1.23 | 0.00 | 1.00 | -15.96 | 248.04 | 47.36 | 243.67 | 0.7914 | -338.0 | -357.5 | |
| 0.00 | 1.23 | 0.00 | 1.00 | -16.87 | 248.10 | 47.42 | 242.63 | 0.7957 | -330.0 | -266.1 | |
| 0.00 | 1.59 | 0.00 | 1.28 | -16.72 | 247.87 | 47.19 | 242.70 | 0.7929 | -550.0 | -498.5 | |
| 1.76 | 28.37 | 1.39 | 22.26 | -15.12 | 247.24 | 46.56 | 244.30 | 0.7802 | -412.2 | -163.2 | |
| 0.00 | 0.44 | 0.00 | 0.36 | -16.94 | 247.80 | 47.12 | 242.41 | 0.7931 | -440.0 | -381.6 | |
| 0.00 | 0.53 | 0.00 | 0.41 | -14.32 | 246.98 | 46.29 | 245.12 | 0.7743 | -268.0 | -211.8 | |
| 0.00 | 3.17 | 0.00 | 2.56 | -17.06 | 247.65 | 46.97 | 242.20 | 0.7923 | -530.0 | -363.7 | |
| 2.73 | -29.00 | 2.15 | -29.00 | -15.29 | 247.06 | 46.38 | 244.00 | 0.7792 | -512.7 | 999999 | |
| 3.44 | -29.00 | 2.68 | -29.00 | -14.88 | 246.72 | 46.04 | 244.34 | 0.7741 | -703.8 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.56 | -16.83 | 247.30 | 46.62 | 242.30 | 0.7880 | -457.0 | -489.6 | |
| 4.85 | -29.00 | 3.78 | -29.00 | -15.07 | 246.68 | 46.00 | 244.09 | 0.7745 | -768.5 | 999999 | |
| 0.00 | 0.35 | 0.00 | 0.28 | -17.19 | 247.33 | 46.65 | 241.89 | 0.7898 | -463.0 | -460.0 | |
| 0.00 | 0.62 | 0.00 | 0.50 | -17.69 | 247.45 | 46.77 | 241.37 | 0.7930 | -327.0 | -297.3 | |
| 0.00 | 1.06 | 0.00 | 0.83 | -15.65 | 246.76 | 46.08 | 243.43 | 0.7777 | -454.0 | -411.8 | |
| 0.00 | 1.06 | 0.00 | 0.82 | -14.43 | 246.38 | 45.69 | 244.71 | 0.7688 | -478.0 | -382.3 | |
| 0.88 | 15.77 | 0.71 | 12.58 | -17.31 | 247.18 | 46.50 | 241.69 | 0.7889 | -537.7 | -372.0 | |
| 0.35 | 2.20 | 0.28 | 1.72 | -15.70 | 246.55 | 45.87 | 243.28 | 0.7759 | -765.2 | -648.0 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -14.55 | 246.23 | 45.55 | 244.50 | 0.7678 | -403.0 | -378.0 | |
| 1.41 | -41.00 | 1.13 | -41.00 | -17.29 | 246.95 | 46.26 | 241.60 | 0.7866 | -860.3 | 999999 | |
| 0.00 | 2.47 | 0.00 | 1.93 | -15.82 | 246.49 | 45.81 | 243.10 | 0.7759 | -590.0 | -433.4 | |
| 1.59 | -41.00 | 1.26 | -41.00 | -17.14 | 246.76 | 46.08 | 241.68 | 0.7842 | -804.2 | 999999 | |
| 0.00 | 1.59 | 0.00 | 1.26 | -16.91 | 246.69 | 46.01 | 241.91 | 0.7825 | -728.0 | -555.0 | |
| 2.03 | 7.40 | 1.60 | 5.83 | -16.63 | 246.56 | 45.88 | 242.17 | 0.7800 | -817.6 | -633.4 | |
| 1.85 | 43.00 | 1.42 | 32.71 | -14.91 | 245.71 | 45.02 | 243.80 | 0.7641 | -650.5 | -546.7 | |
| 0.00 | 2.64 | 0.00 | 2.01 | -14.52 | 245.56 | 44.88 | 244.21 | 0.7609 | -577.0 | -520.2 | |
| 4.85 | -49.00 | 3.70 | -49.00 | -15.19 | 245.51 | 44.83 | 243.38 | 0.7634 | -738.1 | 999999 | |
| 8.28 | -49.00 | 6.30 | -49.00 | -15.23 | 245.26 | 44.58 | 243.20 | 0.7610 | -941.4 | 999999 | |
| 0.00 | 0.62 | 0.00 | 0.46 | -14.26 | 244.79 | 44.11 | 244.15 | 0.7519 | -585.0 | -527.1 | |
| 0.00 | 3.00 | 0.00 | 2.33 | -17.39 | 245.58 | 44.90 | 240.78 | 0.7741 | -635.0 | -519.0 | |
| 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. | |