Optical design of the coronal diagnostic spectrometer (an instrument on the Solar and Heliospheric Observatory)

1997 ◽  
Vol 36 (8) ◽  
pp. 2311 ◽  
Author(s):  
Kate A. Lidiard
Metrologia ◽  
1995 ◽  
Vol 32 (6) ◽  
pp. 647-652 ◽  
Author(s):  
R A Harrison ◽  
B J Kent ◽  
E C Sawyer ◽  
J Hollandt ◽  
M K hne ◽  
...  

1995 ◽  
pp. 233-290
Author(s):  
R. A. Harrison ◽  
E. C. Sawyer ◽  
M. K. Carter ◽  
A. M. Cruise ◽  
R. M. Cutler ◽  
...  

Solar Physics ◽  
1995 ◽  
Vol 162 (1-2) ◽  
pp. 233-290 ◽  
Author(s):  
R. A. Harrison ◽  
E. C. Sawyer ◽  
M. K. Carter ◽  
A. M. Cruise ◽  
R. M. Cutler ◽  
...  

2001 ◽  
Vol 203 ◽  
pp. 505-507
Author(s):  
C. R. Foley ◽  
J. L. Culhane ◽  
D. MacKay

We use the Coronal Diagnostic Spectrometer instrument on board the Solar and Heliospheric Observatory to analyse coronal helmet streamer structures observed close to the solar minimum / maximum on the 1996 July 8 / 1999 August 4-5th. The radial variation of peak electron temperature is extracted out to 2 solar radii. These are found to agree well with Yohkoh observations close to the solar maximum, but are found to be reduced by around half a million close to the solar minimum.


1995 ◽  
Author(s):  
Barry J. Kent ◽  
Richard A. Harrison ◽  
Eric C. Sawyer ◽  
R. W. Hayes ◽  
Anthony G. Richards ◽  
...  

Author(s):  
John W. Coleman

In the design engineering of high performance electromagnetic lenses, the direct conversion of electron optical design data into drawings for reliable hardware is oftentimes difficult, especially in terms of how to mount parts to each other, how to tolerance dimensions, and how to specify finishes. An answer to this is in the use of magnetostatic analytics, corresponding to boundary conditions for the optical design. With such models, the magnetostatic force on a test pole along the axis may be examined, and in this way one may obtain priority listings for holding dimensions, relieving stresses, etc..The development of magnetostatic models most easily proceeds from the derivation of scalar potentials of separate geometric elements. These potentials can then be conbined at will because of the superposition characteristic of conservative force fields.


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