TY  -  
T1  - Fine structure and radial evolution of sheath regions driven by interplanetary coronal mass ejections 
SN  -  /  
UR  - URN:ISBN:978-951-51-6896-2; http://hdl.handle.net/10138/322391 
T3  -  
A1  - Ala-Lahti, Matti 
A2  -  
PB  - Helsingin yliopisto 
Y1  - 2021 
LA  - eng 
AB  - A continuous flow of charged particles emanating from the Sun is ubiquitous in the solar system. This solar wind carries the magnetic field of the star and constitutes a fluid that has an electromagnetic interplay with flow obstacles, such as planetary magnetic fields. The regular conditions in the solar wind flow are drastically disturbed by transients that originate from huge eruptions of plasma and magnetic flux in the Sun. In interplanetary space, these eruptions are known as interplanetary ... 
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KW  - fysiikka 
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