SDO HMI 2014-01-05 02:00:24 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 |
| 15.46 | 88.17 | 8.08 | 47.10 | -12.50 | 116.13 | -19.57 | 116.45 | 0.3652 | 142.3 | 146.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-01-05 02:00:24 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 | 1.19 | 0.00 | 0.60 | -10.05 | 126.38 | -9.32 | 125.86 | 0.1976 | 894.0 | 686.0 | |
| 0.00 | 6.03 | 0.00 | 3.14 | -12.98 | 120.42 | -15.27 | 123.05 | 0.3077 | 556.0 | 784.8 | |
| 0.00 | 0.93 | 0.00 | 0.49 | -12.21 | 119.50 | -16.20 | 119.49 | 0.3146 | 950.0 | 729.9 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -19.24 | 118.83 | -16.86 | 135.02 | 0.3891 | 819.0 | 717.3 | |
| 0.00 | 1.70 | 0.00 | 0.89 | -13.50 | 119.22 | -16.47 | 122.59 | 0.3288 | 865.0 | 692.0 | |
| 5.18 | 29.48 | 2.70 | 15.34 | -11.02 | 119.29 | -16.41 | 115.73 | 0.3091 | 1125.3 | 699.8 | |
| 0.00 | 2.04 | 0.00 | 1.07 | -12.39 | 119.20 | -16.49 | 119.56 | 0.3202 | 1045.0 | 871.8 | |
| 7.90 | -6.00 | 4.11 | -6.00 | -10.84 | 119.24 | -16.46 | 115.13 | 0.3087 | 1209.8 | 999999 | |
| 0.00 | 1.70 | 0.00 | 0.89 | -12.21 | 119.12 | -16.57 | 118.94 | 0.3200 | 991.0 | 828.0 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -9.86 | 119.23 | -16.47 | 112.12 | 0.3028 | -881.0 | -728.9 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -12.50 | 118.69 | -17.00 | 119.16 | 0.3284 | 773.0 | 581.3 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -11.81 | 118.55 | -17.15 | 117.07 | 0.3255 | 793.0 | 721.1 | |
| 0.00 | 8.33 | 0.00 | 4.36 | -11.51 | 118.50 | -17.19 | 116.17 | 0.3241 | 941.0 | 709.6 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -16.46 | 116.75 | -18.94 | 126.18 | 0.3874 | 620.0 | 503.5 | |
| 2.38 | 4.42 | 1.27 | 2.35 | -12.54 | 116.05 | -19.65 | 116.10 | 0.3671 | -1126.4 | -896.1 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -21.46 | 112.98 | -22.71 | 131.06 | 0.4786 | 652.0 | 555.3 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -11.86 | 112.67 | -23.02 | 111.46 | 0.4131 | -803.0 | -587.5 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -13.87 | 111.74 | -23.95 | 115.20 | 0.4375 | -877.0 | -677.6 | |
| 0.00 | 3.48 | 0.00 | 1.90 | -11.72 | 111.83 | -23.87 | 110.54 | 0.4249 | -653.0 | -739.3 | |
| 0.00 | 1.70 | 0.00 | 0.93 | -11.39 | 111.79 | -23.90 | 109.77 | 0.4239 | -878.0 | -582.5 | |
| 0.00 | 2.29 | 0.00 | 1.27 | -14.13 | 111.15 | -24.55 | 115.26 | 0.4474 | -938.0 | -815.0 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -11.74 | 111.30 | -24.40 | 110.22 | 0.4328 | -676.0 | -526.9 | |
| 0.00 | 2.12 | 0.00 | 1.18 | -13.04 | 110.73 | -24.96 | 112.65 | 0.4474 | -719.0 | -695.5 | |
| 0.00 | 2.72 | 0.00 | 1.51 | -13.15 | 110.45 | -25.24 | 112.69 | 0.4520 | -842.0 | -669.4 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -16.12 | 107.81 | -27.89 | 116.66 | 0.5048 | -791.0 | -644.9 | |
| 0.00 | 1.87 | 0.00 | 1.07 | -15.18 | 107.81 | -27.88 | 114.91 | 0.4997 | -653.0 | -628.1 | |
| 0.00 | 1.36 | 0.00 | 0.78 | -15.32 | 107.44 | -28.25 | 114.93 | 0.5055 | -756.0 | -583.7 | |
| 0.00 | 1.53 | 0.00 | 0.89 | -16.27 | 106.77 | -28.92 | 116.22 | 0.5196 | -700.0 | -544.1 | |
| 0.00 | 2.12 | 0.00 | 1.23 | -15.36 | 106.67 | -29.02 | 114.50 | 0.5162 | -729.0 | -652.5 | |
| 0.00 | 1.61 | 0.00 | 0.94 | -15.92 | 106.30 | -29.39 | 115.29 | 0.5241 | -592.0 | -371.5 | |
| 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. | |