SDO HMI 2014-07-03 10:00:40 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 |
| 47.51 | 234.41 | 36.16 | 177.85 | -7.90 | 240.84 | -47.93 | 103.27 | 0.7573 | 374.0 | 139.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-03 10:00:40 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 | 0.73 | 0.00 | 0.52 | -5.93 | 243.30 | -45.47 | 101.26 | 0.7252 | 663.0 | 598.4 | |
| 0.00 | 1.18 | 0.00 | 0.85 | -5.57 | 243.25 | -45.52 | 100.75 | 0.7251 | 441.0 | 447.2 | |
| 0.00 | 1.36 | 0.00 | 0.98 | -6.09 | 243.15 | -45.62 | 101.44 | 0.7273 | 735.0 | 636.0 | |
| 0.00 | 3.54 | 0.00 | 2.55 | -5.82 | 243.09 | -45.68 | 101.05 | 0.7274 | 554.0 | 476.9 | |
| 2.18 | 6.54 | 1.62 | 4.87 | -8.28 | 241.78 | -46.98 | 104.01 | 0.7480 | 857.4 | 555.9 | |
| 22.17 | 136.01 | 16.47 | 101.57 | -7.57 | 241.71 | -47.06 | 103.06 | 0.7472 | 945.7 | 261.3 | |
| 0.64 | 50.06 | 0.48 | 37.99 | -8.58 | 241.32 | -47.44 | 104.28 | 0.7539 | 784.9 | 29.5 | |
| 0.00 | 1.09 | 0.00 | 0.83 | -9.62 | 241.14 | -47.63 | 105.57 | 0.7584 | 511.0 | 376.2 | |
| 0.00 | 1.09 | 0.00 | 0.82 | -8.30 | 241.37 | -47.40 | 103.92 | 0.7527 | 572.0 | 484.6 | |
| 0.00 | 0.36 | 0.00 | 0.27 | -6.80 | 241.59 | -47.18 | 102.01 | 0.7469 | 358.0 | 407.5 | |
| 0.00 | 1.27 | 0.00 | 0.94 | -6.12 | 241.67 | -47.09 | 101.13 | 0.7445 | 479.0 | 426.3 | |
| 9.09 | -7.00 | 6.86 | -7.00 | -8.84 | 241.10 | -47.67 | 104.55 | 0.7570 | 702.2 | 999999 | |
| 0.27 | -6.00 | 0.20 | -6.00 | -7.81 | 241.26 | -47.50 | 103.25 | 0.7527 | 561.3 | 999999 | |
| 1.18 | -6.00 | 0.89 | -6.00 | -7.73 | 241.00 | -47.77 | 103.08 | 0.7555 | 379.0 | 999999 | |
| 1.00 | -7.00 | 0.76 | -7.00 | -8.35 | 240.81 | -47.96 | 103.85 | 0.7590 | 289.4 | 999999 | |
| 3.00 | -6.00 | 2.26 | -6.00 | -7.30 | 240.88 | -47.89 | 102.49 | 0.7559 | 393.1 | 999999 | |
| 0.00 | 2.00 | 0.00 | 1.53 | -7.91 | 240.18 | -48.58 | 103.12 | 0.7649 | -138.0 | -76.5 | |
| 0.00 | 0.91 | 0.00 | 0.71 | -9.54 | 239.32 | -49.44 | 104.97 | 0.7778 | 467.0 | 379.9 | |
| 0.00 | 1.36 | 0.00 | 1.05 | -7.04 | 239.52 | -49.25 | 101.84 | 0.7704 | -598.0 | -568.5 | |
| 0.00 | 0.55 | 0.00 | 0.43 | -9.30 | 238.94 | -49.83 | 104.57 | 0.7814 | 319.0 | 289.0 | |
| 0.00 | 1.64 | 0.00 | 1.30 | -8.05 | 238.35 | -50.42 | 102.86 | 0.7850 | -704.0 | -589.3 | |
| 0.00 | 0.82 | 0.00 | 0.66 | -9.91 | 237.84 | -50.93 | 105.05 | 0.7942 | -681.0 | -604.2 | |
| 2.45 | 3.73 | 1.97 | 2.99 | -8.16 | 238.04 | -50.73 | 102.92 | 0.7884 | -556.2 | -429.9 | |
| 0.45 | 2.45 | 0.37 | 2.01 | -10.06 | 237.31 | -51.46 | 105.10 | 0.7999 | -636.8 | -540.9 | |
| 0.00 | 0.55 | 0.00 | 0.45 | -10.01 | 237.02 | -51.75 | 104.96 | 0.8027 | -218.0 | -261.2 | |
| 0.00 | 1.18 | 0.00 | 0.96 | -7.97 | 237.38 | -51.38 | 102.53 | 0.7949 | -522.0 | -450.8 | |
| 3.63 | 10.72 | 3.05 | 9.04 | -8.40 | 235.99 | -52.78 | 102.76 | 0.8099 | -722.5 | -508.5 | |
| 0.00 | 1.36 | 0.00 | 1.16 | -6.67 | 235.22 | -53.55 | 100.50 | 0.8147 | -488.0 | -454.5 | |
| 1.45 | 3.09 | 1.23 | 2.63 | -6.36 | 235.22 | -53.55 | 100.12 | 0.8142 | -703.9 | -572.8 | |
| 0.00 | 0.82 | 0.00 | 0.74 | -10.37 | 233.14 | -55.63 | 104.49 | 0.8407 | -394.0 | -377.2 | |
| 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. | |