On the differential ion velocity in the inner solar corona and the observed solar wind ionic charge states

1998 ◽  
Vol 103 (A7) ◽  
pp. 14539-14545 ◽  
Author(s):  
Yuan-Kuen Ko ◽  
Johannes Geiss ◽  
George Gloeckler
1999 ◽  
Author(s):  
Yuan-Kuen Ko ◽  
George Gloeckler ◽  
Christina M. S. Cohen ◽  
Antoinette B. Galvin

1999 ◽  
Vol 104 (A8) ◽  
pp. 17005-17019 ◽  
Author(s):  
Yuan-Kuen Ko ◽  
George Gloeckler ◽  
Christina M. S. Cohen ◽  
Antoinette B. Galvin

Solar Physics ◽  
2017 ◽  
Vol 292 (9) ◽  
Author(s):  
Peter Bochsler ◽  
Andrzej Fludra ◽  
Alessandra Giunta
Keyword(s):  

Solar Physics ◽  
2019 ◽  
Vol 294 (1) ◽  
Author(s):  
Roberto Lionello ◽  
Cooper Downs ◽  
Jon A. Linker ◽  
Zoran Mikić ◽  
John Raymond ◽  
...  

1988 ◽  
Vol 123 ◽  
pp. 545-548
Author(s):  
V. Domingo

As a cornerstone of its long term plan for space science research, the European Space Agency (ESA) is developing the Solar Terrestrial Physics Programme that consists of two parts: one, the Solar and Heliospheric Observatory (SOHO) for the study of the solar internal structure and the physics of the solar corona and the solar wind, and another, CLUSTER, a series of four spacecraft flying in formation to study small scale plasma phenomena in several regions of the magnetosphere and in the near Earth solar wind. The feasibility of the missions was demonstrated in Phase A studies carried out by industrial consortia under the supervision of ESA (1,2). According to the current plans an announcement of opportunity calling for instrument proposals will be issued by ESA during the first quarter of 1987. It is foreseen that the spacecraft will be launched by the end of 1994.


2007 ◽  
Vol 130 (1-4) ◽  
pp. 273-282 ◽  
Author(s):  
B. Klecker ◽  
E. Möbius ◽  
M. A. Popecki

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