SDO HMI 2011-07-03 01:59:11 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 |
| 48.24 | 251.26 | 24.63 | 128.81 | 16.29 | 352.96 | -6.09 | 23.25 | 0.2552 | -289.2 | -95.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-07-03 01:59:11 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 | 0.38 | 23.45 | 359.03 | -0.02 | 0.05 | 0.3500 | 698.0 | 646.2 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 19.75 | 358.22 | -0.83 | 2.71 | 0.2889 | -802.0 | -604.0 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 11.93 | 358.04 | -1.02 | 6.41 | 0.1560 | -850.0 | -621.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 19.40 | 357.35 | -1.70 | 5.68 | 0.2841 | -995.0 | -822.3 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 19.30 | 357.06 | -1.99 | 6.68 | 0.2830 | -877.0 | -655.0 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 14.78 | 355.91 | -3.14 | 14.61 | 0.2110 | -1026.0 | -809.8 | |
| 9.90 | 152.78 | 5.04 | 77.99 | 15.77 | 355.23 | -3.82 | 16.23 | 0.2305 | -1140.4 | -461.9 | |
| 1.91 | -7.00 | 0.97 | -7.00 | 15.77 | 354.98 | -4.08 | 17.25 | 0.2317 | -1071.6 | 999999 | |
| 8.99 | -7.00 | 4.59 | -7.00 | 16.08 | 354.81 | -4.24 | 17.48 | 0.2376 | -1254.8 | 999999 | |
| 19.17 | -7.00 | 9.79 | -7.00 | 16.33 | 354.36 | -4.69 | 18.86 | 0.2440 | -1229.4 | 999999 | |
| 0.55 | -7.00 | 0.28 | -7.00 | 16.71 | 354.10 | -4.96 | 19.30 | 0.2514 | -818.7 | 999999 | |
| 0.00 | 2.36 | 0.00 | 1.23 | 19.55 | 353.75 | -5.30 | 17.03 | 0.2985 | -958.0 | -624.4 | |
| 3.18 | 4.09 | 1.62 | 2.08 | 15.55 | 353.81 | -5.25 | 22.13 | 0.2348 | -1037.7 | -969.4 | |
| 0.00 | 3.91 | 0.00 | 1.99 | 15.80 | 353.70 | -5.35 | 22.10 | 0.2394 | -508.0 | -634.5 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 21.01 | 353.47 | -5.58 | 16.38 | 0.3231 | -740.0 | -511.1 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 13.77 | 353.63 | -5.42 | 26.24 | 0.2086 | -877.0 | -724.8 | |
| 0.00 | 2.45 | 0.00 | 1.24 | 13.31 | 353.36 | -5.70 | 28.45 | 0.2037 | -832.0 | -667.1 | |
| 0.00 | 3.91 | 0.00 | 1.99 | 15.76 | 353.29 | -5.76 | 23.67 | 0.2416 | -665.0 | -602.2 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 17.36 | 352.60 | -6.45 | 23.43 | 0.2708 | -948.0 | -769.6 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 19.35 | 351.91 | -7.14 | 22.67 | 0.3058 | -886.0 | -698.0 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.19 | 351.30 | -7.75 | 31.69 | 0.2487 | 930.0 | 695.4 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 19.47 | 350.63 | -8.42 | 26.00 | 0.3163 | -842.0 | -711.6 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 15.18 | 350.51 | -8.54 | 34.23 | 0.2560 | 877.0 | 593.9 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 15.09 | 350.32 | -8.73 | 35.03 | 0.2565 | 846.0 | 591.9 | |
| 0.00 | 2.82 | 0.00 | 1.44 | 15.34 | 350.28 | -8.77 | 34.58 | 0.2603 | 930.0 | 729.0 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 15.52 | 350.05 | -9.01 | 34.85 | 0.2651 | 947.0 | 834.1 | |
| 0.00 | 2.27 | 0.00 | 1.17 | 15.34 | 349.99 | -9.06 | 35.44 | 0.2631 | 866.0 | 651.6 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 15.46 | 349.57 | -9.48 | 36.39 | 0.2689 | 1072.0 | 897.2 | |
| 0.00 | 7.63 | 0.00 | 3.95 | 16.90 | 349.34 | -9.72 | 33.93 | 0.2905 | 919.0 | 567.1 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 16.80 | 349.21 | -9.84 | 34.46 | 0.2904 | 956.0 | 767.2 | |
| 2.45 | 14.81 | 1.26 | 7.63 | 15.92 | 349.19 | -9.86 | 36.38 | 0.2788 | 983.2 | 927.7 | |
| 0.91 | -31.00 | 0.47 | -31.00 | 15.49 | 349.15 | -9.90 | 37.49 | 0.2735 | 1070.9 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 16.61 | 349.09 | -9.96 | 35.17 | 0.2890 | 945.0 | 663.4 | |
| 0.00 | 4.54 | 0.00 | 2.35 | 15.82 | 348.65 | -10.40 | 38.05 | 0.2830 | 849.0 | 774.9 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 16.04 | 348.48 | -10.57 | 38.01 | 0.2876 | 858.0 | 653.3 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 16.76 | 347.85 | -11.20 | 38.02 | 0.3032 | 928.0 | 801.3 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 16.57 | 347.77 | -11.28 | 38.63 | 0.3017 | 899.0 | 630.2 | |
| 0.00 | 6.81 | 0.00 | 3.55 | 17.07 | 347.51 | -11.54 | 38.19 | 0.3107 | 702.0 | 800.4 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 17.66 | 347.47 | -11.58 | 37.06 | 0.3188 | 922.0 | 803.9 | |
| 0.00 | 1.91 | 0.00 | 0.99 | 16.82 | 347.43 | -11.62 | 38.91 | 0.3084 | 897.0 | 791.0 | |
| 1.18 | 4.09 | 0.61 | 2.12 | 16.44 | 347.29 | -11.76 | 40.06 | 0.3051 | 906.0 | 766.2 | |
| 0.00 | 6.54 | 0.00 | 3.43 | 17.98 | 347.19 | -11.86 | 37.09 | 0.3256 | 323.0 | 743.2 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 17.32 | 347.14 | -11.92 | 38.54 | 0.3177 | 799.0 | 615.2 | |
| 0.00 | 0.27 | 0.00 | 0.14 | 16.90 | 346.87 | -12.18 | 40.01 | 0.3154 | 768.0 | 621.3 | |
| 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. | |