TY  -  
T1  - Observational Evidence for the Associated Formation of Blobs and Raining Inflows in the Solar Corona 
SN  -  /  
UR  - http://hdl.handle.net/10138/178856 
T3  -  
A1  - Sanchez-Diaz, E.; Rouillard, A. P.; Davies, J. A.; Lavraud, B.; Sheeley, N. R.; Pinto, R. F.; Kilpua, E.; Plotnikov, I.; Genot, V. 
A2  -  
PB  -  
Y1  - 2017 
LA  - eng 
AB  - The origin of the slow solar wind is still a topic of much debate. The continual emergence of small transient structures from helmet streamers is thought to constitute one of the main sources of the slow wind. Determining the height at which these transients are released is an important factor in determining the conditions under which the slow solar wind forms. To this end, we have carried out a multipoint analysis of small transient structures released from a north-south tilted helmet streamer ... 
VO  -  
IS  -  
SP  -  
OP  -  
KW  - magnetic reconnection; solar wind; Sun: corona; Sun: heliosphere; R-CIRCLE-DOT; WIND; ORIGIN; RECONNECTION; ACCELERATION; CONNECTION; TRANSIENTS; EARTH; FLOW; 115 Astronomy, Space science 
N1  -   
PP  -  
ER  -