TY  -  
T1  - Radial Evolution of Magnetic Field Fluctuations in an Interplanetary Coronal Mass Ejection Sheath 
SN  -  /  
UR  - http://hdl.handle.net/10138/329216 
T3  -  
A1  - Good, S. W.; Ala-Lahti, M.; Palmerio, E.; Kilpua, E. K. J.; Osmane, A. 
A2  -  
PB  -  
Y1  - 2020 
LA  - eng 
AB  - The sheaths of compressed solar wind that precede interplanetary coronal mass ejections (ICMEs) commonly display large-amplitude magnetic field fluctuations. As ICMEs propagate radially from the Sun, the properties of these fluctuations may evolve significantly. We have analyzed magnetic field fluctuations in an ICME sheath observed by MESSENGER at 0.47 au and subsequently by STEREO-B at 1.08 au while the spacecraft were close to radial alignment. Radial changes in fluctuation amplitude, compres... 
VO  -  
IS  -  
SP  -  
OP  -  
KW  - Solar wind; Interplanetary magnetic fields; Interplanetary turbulence; SOLAR-WIND TURBULENCE; DRIVEN; WAVES; EARTH; 115 Astronomy, Space science 
N1  -   
PP  -  
ER  -