SDO HMI 2014-07-11 07:00:40 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 |
| 31.71 | 154.05 | 16.82 | 81.43 | 5.82 | 204.64 | 20.11 | 276.29 | 0.3458 | -212.8 | -265.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-11 07:00:40 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 |
| 0.00 | 0.82 | 0.00 | 0.44 | 6.91 | 207.57 | 23.04 | 278.37 | 0.3944 | -798.0 | -687.8 | |
| 15.17 | 83.85 | 8.08 | 44.69 | 5.85 | 206.13 | 21.60 | 275.93 | 0.3697 | -1115.3 | -416.3 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 4.85 | 205.83 | 21.30 | 273.24 | 0.3641 | -684.0 | -541.0 | |
| 0.82 | 2.36 | 0.43 | 1.25 | 4.52 | 205.72 | 21.19 | 272.33 | 0.3622 | -1037.8 | -877.3 | |
| 7.81 | -2.00 | 4.15 | -2.00 | 5.87 | 205.64 | 21.11 | 276.06 | 0.3618 | -1189.2 | 999999 | |
| 0.00 | 12.63 | 0.00 | 6.68 | 3.44 | 205.04 | 20.50 | 269.26 | 0.3512 | -863.0 | -773.9 | |
| 0.36 | 1.45 | 0.19 | 0.77 | 3.99 | 204.95 | 20.42 | 270.84 | 0.3496 | -700.0 | -637.8 | |
| 0.55 | 4.45 | 0.29 | 2.35 | 6.38 | 204.51 | 19.98 | 277.81 | 0.3443 | -868.5 | -696.3 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 5.50 | 204.45 | 19.91 | 275.25 | 0.3420 | -798.0 | -578.9 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 6.97 | 204.34 | 19.81 | 279.56 | 0.3426 | -720.0 | -694.0 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 5.23 | 204.18 | 19.64 | 274.50 | 0.3373 | -887.0 | -672.8 | |
| 0.91 | 1.91 | 0.48 | 1.01 | 7.82 | 204.25 | 19.72 | 282.09 | 0.3434 | 809.4 | 619.7 | |
| 1.36 | 3.45 | 0.72 | 1.81 | 6.19 | 203.82 | 19.29 | 277.44 | 0.3326 | -1012.2 | -766.1 | |
| 0.00 | 1.64 | 0.00 | 0.86 | 7.99 | 203.61 | 19.08 | 282.92 | 0.3335 | 705.0 | 592.4 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 7.84 | 203.44 | 18.91 | 282.57 | 0.3303 | 877.0 | 737.0 | |
| 0.00 | 5.72 | 0.00 | 3.00 | 6.29 | 203.27 | 18.74 | 277.93 | 0.3239 | -728.0 | -795.5 | |
| 3.91 | 5.81 | 2.05 | 3.05 | 8.09 | 203.32 | 18.79 | 283.38 | 0.3292 | 1099.8 | 747.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 5.38 | 203.21 | 18.68 | 275.11 | 0.3215 | -876.0 | -745.4 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 6.42 | 202.95 | 18.42 | 278.44 | 0.3189 | -751.0 | -590.8 | |
| 0.82 | 2.63 | 0.43 | 1.37 | 7.07 | 202.43 | 17.90 | 280.73 | 0.3118 | 977.0 | 835.4 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 5.31 | 202.24 | 17.71 | 275.08 | 0.3054 | 691.0 | 591.3 | |
| 0.00 | 4.72 | 0.00 | 2.46 | 4.97 | 202.13 | 17.60 | 274.00 | 0.3033 | 973.0 | 832.6 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 5.90 | 201.74 | 17.21 | 277.17 | 0.2980 | 1016.0 | 752.8 | |
| 0.00 | 2.00 | 0.00 | 1.04 | 7.07 | 201.30 | 16.77 | 281.31 | 0.2934 | 882.0 | 649.0 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 5.63 | 200.11 | 15.58 | 276.78 | 0.2703 | 810.0 | 586.9 | |
| 0.00 | 2.00 | 0.00 | 1.02 | 5.76 | 199.44 | 14.91 | 277.54 | 0.2594 | 829.0 | 648.9 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 5.23 | 198.64 | 14.11 | 275.73 | 0.2450 | 774.0 | 586.9 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 6.74 | 197.51 | 12.98 | 282.74 | 0.2297 | 809.0 | 661.7 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 6.35 | 197.22 | 12.69 | 281.28 | 0.2236 | 851.0 | 677.4 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 6.46 | 196.19 | 11.65 | 282.67 | 0.2067 | 892.0 | 721.3 | |
| 0.00 | 1.64 | 0.00 | 0.83 | 6.67 | 196.10 | 11.57 | 283.79 | 0.2060 | 936.0 | 732.7 | |
| 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. | |