High resolution far infrared polarimeter for plasma diagnostics

1992 ◽  
Vol 13 (5) ◽  
pp. 591-608 ◽  
Author(s):  
S. L. Prunty ◽  
M. C. Sexton ◽  
E. Zilli
2020 ◽  
Vol 124 (12) ◽  
pp. 2427-2435 ◽  
Author(s):  
Marie-Aline Martin-Drumel ◽  
Jessica P. Porterfield ◽  
Manuel Goubet ◽  
Pierre Asselin ◽  
Robert Georges ◽  
...  

2008 ◽  
Vol 51 (5) ◽  
pp. 404-406 ◽  
Author(s):  
G.L. Carr ◽  
R.J. Smith ◽  
L. Mihaly ◽  
H. Zhang ◽  
D.H. Reitze ◽  
...  

2012 ◽  
Vol 58 ◽  
pp. 279-282
Author(s):  
M.A. Martin-Drumel ◽  
O. Pirali ◽  
S. Eliet ◽  
A. Cuisset

1968 ◽  
Vol 26 (4) ◽  
pp. 146-148 ◽  
Author(s):  
J. Boettcher ◽  
K. Dransfeld ◽  
K.F. Renk

2001 ◽  
Vol 72 (1) ◽  
pp. 1094-1097 ◽  
Author(s):  
S. Okajima ◽  
K. Nakayama ◽  
H. Tazawa ◽  
K. Kawahata ◽  
K. Tanaka ◽  
...  

Author(s):  
L. R. Zink ◽  
M. Prevedelli ◽  
K. M. Evenson ◽  
M. Inguscio

2006 ◽  
Vol 2 (S237) ◽  
pp. 412-412
Author(s):  
Marcello Felli ◽  
Fabrizio Massi ◽  
Riccardo Cesaroni

AbstractThe star forming region S235A-B has been studied at high resolution with radio (IRAM Interferometer and VLA) and infrared (JCMT and Spitzer) observations. The region was mapped in HCO+, C34S, H2CS, SO2 and CH3CN as well as in the 1.2 and 3.3 continuum, in the cm continuum at 6, 3.6, 1.3 and 0.7 cm and in the 22 GHz water maser line, in the far infrared at 450 and 850 μm and in the mid infrared from 3.6 to 8 μm. Finally, use was made of the Medicina water maser patrol, from 1987 to 2005, to study the maser variability.


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