SDO HMI 2014-01-07 05:00:24 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 |
| 198.65 | 856.28 | 101.82 | 439.08 | 8.97 | 100.17 | -7.55 | 29.92 | 0.2581 | 204.4 | 90.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-01-07 05:00:24 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 | 2.38 | 0.00 | 1.20 | 8.05 | 106.49 | -1.23 | 5.96 | 0.2060 | -839.0 | -499.0 | |
| 8.92 | 79.13 | 4.53 | 40.13 | 8.47 | 105.26 | -2.46 | 11.35 | 0.2164 | -1295.9 | -463.3 | |
| 11.90 | -2.00 | 6.04 | -2.00 | 8.41 | 104.94 | -2.78 | 12.87 | 0.2166 | -1184.7 | 999999 | |
| 2.97 | 9.01 | 1.51 | 4.57 | 8.54 | 104.40 | -3.32 | 15.11 | 0.2209 | -1021.0 | -928.4 | |
| 0.00 | 3.14 | 0.00 | 1.59 | 7.63 | 104.14 | -3.58 | 17.47 | 0.2073 | -1185.0 | -903.4 | |
| 0.00 | 1.53 | 0.00 | 0.78 | 7.82 | 103.90 | -3.82 | 18.28 | 0.2115 | -958.0 | -720.5 | |
| 4.59 | 132.93 | 2.34 | 67.83 | 8.90 | 103.50 | -4.22 | 18.41 | 0.2313 | -1062.6 | -580.7 | |
| 2.12 | -7.00 | 1.08 | -7.00 | 8.81 | 103.14 | -4.58 | 19.99 | 0.2319 | -1223.3 | 999999 | |
| 12.66 | -7.00 | 6.45 | -7.00 | 8.79 | 102.72 | -5.00 | 21.69 | 0.2340 | -1234.1 | 999999 | |
| 0.93 | 3.40 | 0.47 | 1.72 | 7.64 | 102.73 | -4.98 | 23.63 | 0.2159 | -1122.2 | -850.0 | |
| 7.90 | -7.00 | 4.03 | -7.00 | 9.24 | 102.45 | -5.27 | 22.03 | 0.2429 | -1018.4 | 999999 | |
| 0.00 | 2.29 | 0.00 | 1.16 | 7.67 | 102.47 | -5.25 | 24.69 | 0.2182 | -978.0 | -807.2 | |
| 1.61 | 99.27 | 0.82 | 50.60 | 8.01 | 102.31 | -5.41 | 24.68 | 0.2245 | -1222.3 | -200.3 | |
| 14.70 | -7.00 | 7.51 | -7.00 | 9.22 | 102.09 | -5.63 | 23.42 | 0.2448 | -1066.4 | 999999 | |
| 0.00 | 3.31 | 0.00 | 1.69 | 8.43 | 102.07 | -5.65 | 24.86 | 0.2328 | -965.0 | -785.3 | |
| 14.96 | -13.00 | 7.62 | -13.00 | 8.38 | 101.38 | -6.34 | 27.57 | 0.2371 | -1035.6 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 7.50 | 101.33 | -6.39 | 29.58 | 0.2245 | -719.0 | -463.9 | |
| 0.00 | 1.70 | 0.00 | 0.86 | 6.96 | 101.28 | -6.44 | 31.03 | 0.2170 | -793.0 | -562.2 | |
| 0.00 | 5.10 | 0.00 | 2.61 | 9.11 | 100.74 | -6.98 | 28.44 | 0.2532 | -65.0 | -214.6 | |
| 3.99 | -13.00 | 2.04 | -13.00 | 8.02 | 100.49 | -7.23 | 31.55 | 0.2394 | 1015.7 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.52 | 9.20 | 100.25 | -7.47 | 29.89 | 0.2586 | 885.0 | 585.1 | |
| 0.42 | -13.00 | 0.22 | -13.00 | 8.45 | 100.15 | -7.57 | 31.79 | 0.2485 | -675.6 | 999999 | |
| 2.63 | 6.03 | 1.35 | 3.10 | 9.38 | 100.07 | -7.65 | 30.14 | 0.2628 | 1063.8 | 753.6 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 8.57 | 99.87 | -7.84 | 32.44 | 0.2528 | -404.0 | -258.5 | |
| 0.59 | 503.49 | 0.31 | 259.42 | 9.03 | 99.71 | -8.00 | 32.00 | 0.2607 | 912.7 | 431.4 | |
| 3.91 | -25.00 | 2.01 | -25.00 | 9.18 | 99.47 | -8.25 | 32.46 | 0.2651 | 796.4 | 999999 | |
| 0.68 | -25.00 | 0.35 | -25.00 | 9.73 | 99.16 | -8.56 | 32.33 | 0.2757 | 968.5 | 999999 | |
| 9.18 | -25.00 | 4.72 | -25.00 | 9.36 | 99.13 | -8.59 | 33.12 | 0.2708 | 1079.1 | 999999 | |
| 2.29 | -25.00 | 1.18 | -25.00 | 9.85 | 99.03 | -8.69 | 32.46 | 0.2786 | 1037.7 | 999999 | |
| 0.93 | -25.00 | 0.48 | -25.00 | 9.61 | 98.83 | -8.89 | 33.55 | 0.2771 | 893.5 | 999999 | |
| 0.51 | -25.00 | 0.26 | -25.00 | 9.73 | 98.73 | -8.99 | 33.58 | 0.2797 | 896.5 | 999999 | |
| 89.07 | -25.00 | 45.89 | -25.00 | 9.16 | 98.20 | -9.52 | 36.31 | 0.2770 | 1369.6 | 999999 | |
| 1.19 | -25.00 | 0.61 | -25.00 | 8.59 | 98.19 | -9.53 | 37.63 | 0.2694 | 1123.6 | 999999 | |
| 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. | |