| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 106.44 | 545.80 | 79.09 | 404.64 | 12.27 | 128.11 | -48.21 | 79.01 | 0.7440 | -172.6 | -75.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-08 03:00:39 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 |
| 60.91 | 331.91 | 43.34 | 236.54 | 13.54 | 130.27 | -46.05 | 77.20 | 0.7201 | -1099.3 | -313.1 | |
| 0.72 | -1.00 | 0.52 | -1.00 | 12.95 | 129.87 | -46.45 | 78.05 | 0.7243 | -240.8 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.60 | 15.97 | 128.48 | -47.85 | 74.09 | 0.7434 | -290.0 | -346.8 | |
| 1.72 | -1.00 | 1.25 | -1.00 | 13.43 | 128.97 | -47.35 | 77.46 | 0.7352 | -278.3 | 999999 | |
| 0.00 | 2.89 | 0.00 | 2.12 | 13.69 | 128.67 | -47.65 | 77.14 | 0.7388 | 143.0 | 115.6 | |
| 0.00 | 1.54 | 0.00 | 1.13 | 13.35 | 128.34 | -47.98 | 77.63 | 0.7423 | -424.0 | -353.1 | |
| 0.00 | 0.90 | 0.00 | 0.66 | 12.34 | 128.45 | -47.87 | 78.98 | 0.7404 | 105.0 | 142.8 | |
| 0.00 | 1.08 | 0.00 | 0.80 | 11.17 | 128.35 | -47.97 | 80.58 | 0.7410 | 359.0 | 439.2 | |
| 0.00 | 1.08 | 0.00 | 0.80 | 10.83 | 127.96 | -48.36 | 81.05 | 0.7454 | -199.0 | -209.0 | |
| 1.63 | 12.65 | 1.23 | 9.47 | 11.74 | 127.09 | -49.23 | 79.86 | 0.7556 | 684.9 | 581.4 | |
| 0.00 | 2.17 | 0.00 | 1.65 | 11.79 | 126.60 | -49.73 | 79.81 | 0.7611 | 519.0 | 482.8 | |
| 0.00 | 2.08 | 0.00 | 1.59 | 11.69 | 126.43 | -49.89 | 79.96 | 0.7629 | 473.0 | 534.9 | |
| 0.00 | 3.16 | 0.00 | 2.43 | 11.47 | 126.04 | -50.28 | 80.26 | 0.7671 | 683.0 | 534.4 | |
| 0.00 | 1.27 | 0.00 | 0.98 | 11.18 | 125.87 | -50.45 | 80.64 | 0.7689 | 687.0 | 574.1 | |
| 0.00 | 1.54 | 0.00 | 1.18 | 10.39 | 125.95 | -50.37 | 81.68 | 0.7679 | 755.0 | 631.8 | |
| 0.00 | 1.08 | 0.00 | 0.83 | 10.08 | 125.97 | -50.35 | 82.07 | 0.7677 | 608.0 | 638.9 | |
| 0.90 | 2.26 | 0.70 | 1.75 | 10.61 | 125.71 | -50.61 | 81.38 | 0.7706 | 751.7 | 691.8 | |
| 0.45 | 1.54 | 0.35 | 1.19 | 9.86 | 125.87 | -50.45 | 82.37 | 0.7687 | 677.4 | 617.4 | |
| 0.00 | 1.45 | 0.00 | 1.12 | 11.10 | 125.60 | -50.73 | 80.76 | 0.7719 | 430.0 | 461.8 | |
| 0.00 | 1.45 | 0.00 | 1.12 | 10.66 | 125.50 | -50.82 | 81.33 | 0.7729 | 583.0 | 683.3 | |
| 3.52 | 157.77 | 2.74 | 125.12 | 10.32 | 125.53 | -50.79 | 81.77 | 0.7725 | 799.0 | 211.9 | |
| 0.00 | 1.36 | 0.00 | 1.06 | 11.37 | 125.23 | -51.09 | 80.41 | 0.7759 | 176.0 | 154.2 | |
| 0.00 | 7.59 | 0.00 | 5.95 | 11.09 | 125.10 | -51.22 | 80.78 | 0.7773 | 438.0 | 386.7 | |
| 3.43 | -21.00 | 2.70 | -21.00 | 10.74 | 124.99 | -51.34 | 81.23 | 0.7785 | 746.1 | 999999 | |
| 15.90 | -21.00 | 12.52 | -21.00 | 9.99 | 124.91 | -51.41 | 82.19 | 0.7793 | 918.3 | 999999 | |
| 0.36 | 5.96 | 0.29 | 4.74 | 11.62 | 124.52 | -51.81 | 80.11 | 0.7837 | -119.0 | 208.4 | |
| 0.00 | 0.99 | 0.00 | 0.79 | 11.05 | 124.61 | -51.71 | 80.84 | 0.7825 | 308.0 | 293.7 | |
| 3.34 | -21.00 | 2.66 | -21.00 | 10.51 | 124.44 | -51.88 | 81.53 | 0.7843 | 603.5 | 999999 | |
| 1.72 | -21.00 | 1.36 | -21.00 | 10.24 | 124.50 | -51.82 | 81.88 | 0.7836 | 648.7 | 999999 | |
| 7.50 | -21.00 | 5.96 | -21.00 | 9.71 | 124.47 | -51.85 | 82.55 | 0.7840 | 617.2 | 999999 | |
| 4.34 | -21.00 | 3.47 | -21.00 | 10.52 | 124.19 | -52.14 | 81.52 | 0.7870 | 541.2 | 999999 | |
| 0.00 | 1.27 | 0.00 | 1.02 | 10.04 | 123.64 | -52.69 | 82.13 | 0.7928 | -212.0 | -166.2 | |
| 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. | |