TY  -  
T1  - The nature of moving solar radio bursts associated with coronal mass ejections 
SN  -  /  
UR  - URN:NBN:fi:hulib-202105212323; http://hdl.handle.net/10138/330168 
T3  -  
A1  - Räsänen, Juska 
A2  -  
PB  - Helsingin yliopisto 
Y1  - 2021 
LA  - eng 
AB  - Coronal mass ejections (CMEs) are large-scale eruptions of plasma entrained in a magnetic field. They occur in the solar corona, and from there they propagate into interplanetary space along with the solar wind. If a CME travels faster than the surrounding solar wind, a shock wave forms. Shocks driven by CMEs can act as powerful accelerators of charged particles. When charged particles like electrons are accelerated, they emit electromagnetic radiation, especially in the form of radio waves.

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VO  -  
IS  -  
SP  -  
OP  -  
KW  - Alkeishiukkasfysiikka ja kosmologia; Particle Physics and Cosmology; Elementarpartikelfysik och kosmologi; Alkeishiukkasfysiikan ja astrofysikaalisten tieteiden maisteriohjelma; Master's Programme in Particle physics and Astrophysical Sciences; Magisterprogrammet i elementarpartikelfysik och astrofysikaliska vetenskaper 
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PP  -  
ER  -