SDO HMI 2014-03-13 06:00:29 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 |
| 209.81 | 1048.76 | 107.39 | 535.87 | -18.72 | 324.15 | -7.02 | 153.52 | 0.2406 | 39.8 | 23.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-13 06:00:29 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 | -15.99 | 332.13 | 0.96 | 186.03 | 0.1543 | 735.0 | 600.6 | |
| 0.96 | 403.63 | 0.48 | 203.39 | -17.01 | 329.98 | -1.18 | 173.39 | 0.1723 | 1099.5 | 508.6 | |
| 60.96 | -2.00 | 30.71 | -2.00 | -17.62 | 329.64 | -1.53 | 171.98 | 0.1834 | 1447.1 | 999999 | |
| 1.82 | -2.00 | 0.92 | -2.00 | -16.86 | 329.52 | -1.65 | 170.68 | 0.1708 | 853.0 | 999999 | |
| 1.13 | -2.00 | 0.57 | -2.00 | -18.07 | 328.85 | -2.32 | 168.46 | 0.1934 | 850.2 | 999999 | |
| 1.04 | -2.00 | 0.53 | -2.00 | -17.92 | 328.66 | -2.51 | 167.39 | 0.1915 | 1010.2 | 999999 | |
| 0.96 | -2.00 | 0.48 | -2.00 | -17.82 | 328.22 | -2.94 | 165.15 | 0.1917 | 969.6 | 999999 | |
| 0.00 | 2.34 | 0.00 | 1.19 | -18.27 | 327.97 | -3.20 | 164.57 | 0.2003 | 701.0 | 649.4 | |
| 2.26 | 3.47 | 1.14 | 1.76 | -19.03 | 327.82 | -3.34 | 164.96 | 0.2135 | -803.2 | -477.3 | |
| 0.00 | 2.69 | 0.00 | 1.36 | -18.52 | 327.68 | -3.49 | 163.61 | 0.2056 | 598.0 | 600.8 | |
| 4.69 | 42.73 | 2.37 | 21.58 | -18.06 | 327.66 | -3.51 | 162.83 | 0.1983 | 1114.9 | 679.3 | |
| 10.59 | -11.00 | 5.35 | -11.00 | -17.72 | 327.38 | -3.79 | 161.01 | 0.1942 | 1186.9 | 999999 | |
| 0.00 | 1.39 | 0.00 | 0.70 | -18.24 | 327.27 | -3.89 | 161.40 | 0.2032 | 538.0 | 447.9 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -16.51 | 327.10 | -4.07 | 157.20 | 0.1766 | 750.0 | 453.3 | |
| 0.00 | 0.43 | 0.00 | 0.22 | -17.96 | 326.97 | -4.20 | 159.56 | 0.2005 | 884.0 | 840.8 | |
| 0.00 | 3.39 | 0.00 | 1.71 | -18.11 | 326.37 | -4.80 | 157.23 | 0.2065 | 884.0 | 740.9 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -18.29 | 326.24 | -4.93 | 157.04 | 0.2102 | 810.0 | 621.8 | |
| 0.00 | 2.08 | 0.00 | 1.05 | -17.71 | 325.75 | -5.42 | 153.80 | 0.2047 | 1163.0 | 872.8 | |
| 0.00 | 0.78 | 0.00 | 0.40 | -17.55 | 325.41 | -5.76 | 152.03 | 0.2050 | 540.0 | 528.8 | |
| 0.00 | 3.99 | 0.00 | 2.04 | -19.64 | 324.60 | -6.57 | 153.51 | 0.2425 | 1005.0 | 876.8 | |
| 0.00 | 0.96 | 0.00 | 0.49 | -19.85 | 324.59 | -6.57 | 153.89 | 0.2458 | 842.0 | 668.4 | |
| 2.17 | 7.73 | 1.11 | 3.95 | -19.41 | 323.59 | -7.57 | 149.66 | 0.2472 | -1028.5 | -615.5 | |
| 0.00 | 1.22 | 0.00 | 0.61 | -14.41 | 323.43 | -7.74 | 134.14 | 0.1826 | 750.0 | 571.9 | |
| 4.43 | 164.30 | 2.26 | 84.18 | -19.06 | 323.01 | -8.16 | 147.01 | 0.2475 | -1211.3 | -457.3 | |
| 5.99 | -24.00 | 3.07 | -24.00 | -19.27 | 322.64 | -8.52 | 146.37 | 0.2537 | -1369.9 | 999999 | |
| 0.69 | 2.52 | 0.35 | 1.29 | -18.51 | 322.65 | -8.52 | 144.56 | 0.2433 | 633.2 | 378.8 | |
| 0.00 | 3.73 | 0.00 | 1.88 | -13.02 | 322.80 | -8.37 | 125.90 | 0.1759 | 856.0 | 757.5 | |
| 9.99 | -24.00 | 5.12 | -24.00 | -19.54 | 322.37 | -8.79 | 146.17 | 0.2600 | -1106.9 | 999999 | |
| 11.38 | -24.00 | 5.85 | -24.00 | -20.27 | 322.11 | -9.06 | 147.00 | 0.2725 | 1020.7 | 999999 | |
| 0.00 | 1.39 | 0.00 | 0.71 | -18.41 | 322.15 | -9.02 | 142.77 | 0.2470 | 746.0 | 581.6 | |
| 0.00 | 1.39 | 0.00 | 0.72 | -20.57 | 321.90 | -9.27 | 147.04 | 0.2785 | 713.0 | 594.6 | |
| 0.00 | 2.87 | 0.00 | 1.47 | -19.71 | 321.88 | -9.28 | 145.15 | 0.2670 | 187.0 | 181.1 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -20.68 | 321.60 | -9.57 | 146.47 | 0.2829 | 596.0 | 453.6 | |
| 0.00 | 1.39 | 0.00 | 0.72 | -20.01 | 321.54 | -9.62 | 144.87 | 0.2742 | 606.0 | 437.0 | |
| 0.00 | 2.43 | 0.00 | 1.23 | -15.49 | 321.76 | -9.41 | 132.79 | 0.2156 | 1082.0 | 775.2 | |
| 0.00 | 2.95 | 0.00 | 1.52 | -19.45 | 320.94 | -10.23 | 141.94 | 0.2729 | -550.0 | -591.3 | |
| 0.00 | 7.73 | 0.00 | 4.00 | -20.23 | 320.34 | -10.83 | 142.21 | 0.2891 | -1092.0 | -876.8 | |
| 0.00 | 0.96 | 0.00 | 0.49 | -19.40 | 320.27 | -10.90 | 140.10 | 0.2794 | -875.0 | -581.0 | |
| 1.48 | 17.11 | 0.76 | 8.79 | -18.24 | 320.09 | -11.08 | 136.69 | 0.2673 | -1195.2 | -876.7 | |
| 0.00 | 1.30 | 0.00 | 0.68 | -20.34 | 319.84 | -11.33 | 141.26 | 0.2956 | -809.0 | -630.9 | |
| 1.13 | 3.39 | 0.59 | 1.76 | -20.15 | 319.63 | -11.54 | 140.32 | 0.2954 | -1019.9 | -783.9 | |
| 21.88 | 91.96 | 11.40 | 47.94 | -21.02 | 319.14 | -12.03 | 141.14 | 0.3115 | -1199.4 | -270.7 | |
| 1.82 | 213.89 | 0.94 | 110.65 | -18.95 | 319.30 | -11.87 | 136.66 | 0.2847 | -1276.5 | -431.1 | |
| 16.85 | -43.00 | 8.71 | -43.00 | -18.88 | 319.14 | -12.02 | 136.13 | 0.2857 | -1362.3 | 999999 | |
| 23.53 | -43.00 | 12.18 | -43.00 | -18.90 | 318.76 | -12.41 | 135.31 | 0.2904 | -1183.2 | 999999 | |
| 10.33 | -43.00 | 5.36 | -43.00 | -19.36 | 318.56 | -12.61 | 136.01 | 0.2979 | -1036.8 | 999999 | |
| 0.61 | -43.00 | 0.31 | -43.00 | -18.44 | 318.63 | -12.54 | 133.84 | 0.2868 | -706.6 | 999999 | |
| 9.47 | 44.55 | 4.93 | 23.25 | -20.42 | 318.34 | -12.83 | 138.06 | 0.3127 | -1118.8 | -348.2 | |
| 3.65 | -48.00 | 1.90 | -48.00 | -20.23 | 318.06 | -13.10 | 137.04 | 0.3136 | -976.0 | 999999 | |
| 0.00 | 3.47 | 0.00 | 1.80 | -18.76 | 317.80 | -13.37 | 132.90 | 0.3002 | -173.0 | -256.1 | |
| 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. | |