SDO HMI 2014-07-08 13:00:40 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 |
| 51.40 | 180.39 | 44.54 | 158.38 | 9.30 | 165.24 | -55.70 | 81.21 | 0.8267 | -194.6 | -51.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-08 13:00:40 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 |
| 5.00 | 7.36 | 4.01 | 5.90 | 9.18 | 169.03 | -51.91 | 81.19 | 0.7885 | -645.2 | -437.0 | |
| 0.00 | 1.27 | 0.00 | 1.02 | 8.84 | 168.95 | -51.99 | 81.63 | 0.7892 | -508.0 | -429.9 | |
| 0.00 | 1.18 | 0.00 | 0.98 | 11.25 | 167.77 | -53.16 | 78.68 | 0.8028 | -637.0 | -521.3 | |
| 2.54 | 4.54 | 2.09 | 3.74 | 10.42 | 167.93 | -53.01 | 79.70 | 0.8006 | -597.1 | -452.2 | |
| 0.00 | 0.91 | 0.00 | 0.76 | 11.39 | 167.53 | -53.41 | 78.52 | 0.8054 | -518.0 | -481.5 | |
| 2.27 | 9.08 | 1.89 | 7.54 | 10.96 | 167.54 | -53.40 | 79.06 | 0.8050 | -595.7 | -459.4 | |
| 0.82 | 2.27 | 0.67 | 1.86 | 8.46 | 168.05 | -52.89 | 82.15 | 0.7984 | -534.7 | -348.6 | |
| 0.00 | 0.73 | 0.00 | 0.59 | 7.78 | 168.03 | -52.91 | 83.00 | 0.7985 | 580.0 | 541.2 | |
| 0.00 | 2.27 | 0.00 | 1.87 | 7.34 | 167.80 | -53.14 | 83.56 | 0.8008 | 92.0 | 294.4 | |
| 2.72 | 6.54 | 2.26 | 5.41 | 8.37 | 167.55 | -53.38 | 82.28 | 0.8036 | 37.9 | -17.9 | |
| 0.00 | 1.09 | 0.00 | 0.91 | 7.99 | 167.32 | -53.62 | 82.76 | 0.8059 | -374.0 | -250.7 | |
| 6.54 | 13.99 | 5.49 | 11.73 | 9.17 | 167.02 | -53.92 | 81.30 | 0.8093 | -421.6 | -119.9 | |
| 0.54 | 1.45 | 0.47 | 1.24 | 11.67 | 166.38 | -54.56 | 78.26 | 0.8170 | -522.8 | -458.2 | |
| 0.00 | 1.18 | 0.00 | 1.01 | 10.89 | 166.22 | -54.72 | 79.23 | 0.8181 | 545.0 | 419.2 | |
| 0.82 | 4.00 | 0.71 | 3.46 | 11.83 | 165.85 | -55.09 | 78.11 | 0.8224 | -479.0 | -450.5 | |
| 0.00 | 0.27 | 0.00 | 0.23 | 7.90 | 166.17 | -54.77 | 82.90 | 0.8175 | 452.0 | 440.0 | |
| 0.00 | 1.73 | 0.00 | 1.51 | 10.57 | 165.44 | -55.50 | 79.67 | 0.8256 | -136.0 | -38.2 | |
| 0.00 | 1.27 | 0.00 | 1.11 | 10.79 | 165.38 | -55.56 | 79.42 | 0.8263 | 326.0 | 301.0 | |
| 0.00 | 0.91 | 0.00 | 0.79 | 10.14 | 165.44 | -55.50 | 80.19 | 0.8254 | 252.0 | 192.9 | |
| 3.00 | 5.09 | 2.59 | 4.39 | 6.99 | 165.80 | -55.14 | 84.02 | 0.8211 | 543.5 | 393.9 | |
| 6.72 | 10.45 | 5.87 | 9.11 | 8.69 | 165.41 | -55.53 | 81.96 | 0.8252 | -463.7 | -360.7 | |
| 0.00 | 0.27 | 0.00 | 0.24 | 10.62 | 164.48 | -56.46 | 79.67 | 0.8349 | 375.0 | 442.7 | |
| 2.54 | 86.56 | 2.27 | 78.15 | 9.85 | 164.63 | -56.31 | 80.58 | 0.8331 | 580.1 | -66.0 | |
| 0.00 | 2.45 | 0.00 | 2.23 | 12.04 | 163.93 | -57.01 | 78.00 | 0.8407 | 570.0 | 473.0 | |
| 0.00 | 0.82 | 0.00 | 0.74 | 10.80 | 163.85 | -57.09 | 79.49 | 0.8408 | 628.0 | 586.4 | |
| 0.00 | 1.18 | 0.00 | 1.09 | 11.74 | 163.50 | -57.44 | 78.39 | 0.8445 | 401.0 | 327.7 | |
| 13.62 | -23.00 | 12.28 | -23.00 | 8.81 | 164.15 | -56.79 | 81.85 | 0.8373 | -727.5 | 999999 | |
| 2.18 | 4.54 | 2.00 | 4.17 | 10.78 | 163.51 | -57.43 | 79.53 | 0.8439 | 634.9 | 495.7 | |
| 1.27 | -23.00 | 1.16 | -23.00 | 8.70 | 163.72 | -57.22 | 82.00 | 0.8413 | -378.7 | 999999 | |
| 0.00 | 1.27 | 0.00 | 1.17 | 8.80 | 163.29 | -57.65 | 81.89 | 0.8453 | 283.0 | 209.9 | |
| 0.00 | 0.27 | 0.00 | 0.26 | 10.88 | 162.42 | -58.52 | 79.47 | 0.8539 | 457.0 | 431.0 | |
| 0.82 | 3.45 | 0.78 | 3.27 | 10.59 | 162.27 | -58.67 | 79.81 | 0.8551 | 521.6 | 482.4 | |
| 0.00 | 1.09 | 0.00 | 1.03 | 9.61 | 162.26 | -58.68 | 80.97 | 0.8549 | 484.0 | 393.3 | |
| 0.00 | 0.91 | 0.00 | 0.87 | 9.78 | 162.09 | -58.85 | 80.77 | 0.8565 | 517.0 | 457.3 | |
| 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. | |