scholarly journals Physics of intact capture of cometary coma dust samples

2012 ◽  
Author(s):  
William Anderson ◽  
Thomas Ahrens
Keyword(s):  
1993 ◽  
Vol 263 (1) ◽  
pp. 247-255 ◽  
Author(s):  
D. W. Hughes ◽  
N. McBride ◽  
J. Boswell ◽  
P. Jalowiczor
Keyword(s):  

1984 ◽  
Vol 78 ◽  
pp. 237-239
Author(s):  
K. Jockers ◽  
L.G. Balázs

AbstractThe main emissions of the cometary plasma tail are due to CO+ (400/402 and 425/427 nm) and H2O+ (aroud 650 nm). Emissions of CO2+ at 367 nm have also been observed (Swings and Page 1950). These ions relate much more directly to the presumed mother molecules of the cometary nucleus (like H2O, CO2, CO) than most strong emissions of the neutral cometary coma (Ruebner and Giguere, 1980, see also Jockers, 1982). Therefore it is important to determine column densities of cometary ions. So far only very few measurements of ion column densities are available (Wyckhoff and Wehinger, 1976a, b; Arpigny, 1965).


2015 ◽  
Vol 42 (13) ◽  
pp. 5125-5131 ◽  
Author(s):  
J. L. Burch ◽  
T. E. Cravens ◽  
K. Llera ◽  
R. Goldstein ◽  
P. Mokashi ◽  
...  

Icarus ◽  
1981 ◽  
Vol 47 (3) ◽  
pp. 412-430 ◽  
Author(s):  
Michael B. Swift ◽  
George F. Mitchell
Keyword(s):  

1974 ◽  
Vol 193 ◽  
pp. 263 ◽  
Author(s):  
A. C. Aikin
Keyword(s):  

1984 ◽  
Vol 4 (9) ◽  
pp. 217-220 ◽  
Author(s):  
W.C. Carey ◽  
J.A.M. McDonnell ◽  
C.S. Welch ◽  
J.C. Zarnecki
Keyword(s):  

2016 ◽  
Vol 833 (2) ◽  
pp. 160 ◽  
Author(s):  
Y. Shou ◽  
M. Combi ◽  
G. Toth ◽  
V. Tenishev ◽  
N. Fougere ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document