Emission Measure Distribution for an Active Region Using Coordinated SERTS andYohkohSXT Observations

1999 ◽  
Vol 523 (1) ◽  
pp. 432-443 ◽  
Author(s):  
J. T. Schmelz ◽  
J. L. R. Saba ◽  
K. T. Strong ◽  
H. D. Winter ◽  
J. W. Brosius
2011 ◽  
Vol 740 (2) ◽  
pp. 111 ◽  
Author(s):  
Durgesh Tripathi ◽  
James A. Klimchuk ◽  
Helen E. Mason

2015 ◽  
Vol 573 ◽  
pp. A104 ◽  
Author(s):  
Giulio Del Zanna ◽  
Durgesh Tripathi ◽  
Helen Mason ◽  
Srividya Subramanian ◽  
Brendan O’Dwyer

1996 ◽  
Vol 152 ◽  
pp. 81-88 ◽  
Author(s):  
Carole Jordan

Following a summary of early solar EUV spectroscopy the spectra of some late-type stars obtained with the Extreme Ultraviolet Explorer (EUVE) are briefly surveyed. Some transitions which are not included in current emissivity codes but could lead to numerous weak lines, and an apparent continuum in the EUVE short wavelength region, are discussed. The importance of the geometry adopted when interpreting the emission measure distribution is stressed, since radial factors can lead to an apparent emission measure distribution gradient that is steeper than the value of 3/2 expected in plane parallel geometry.


2008 ◽  
Vol 686 (1) ◽  
pp. 363-378 ◽  
Author(s):  
Alex S. Hill ◽  
Robert A. Benjamin ◽  
Grzegorz Kowal ◽  
Ronald J. Reynolds ◽  
L. Matthew Haffner ◽  
...  

2004 ◽  
Vol 2004 (IAUS223) ◽  
pp. 461-462 ◽  
Author(s):  
A. K[ecedilla]pa ◽  
J. Sylwester ◽  
B. Sylwester ◽  
M. Siarkowski

2011 ◽  
Vol 742 (1) ◽  
pp. L6 ◽  
Author(s):  
Fana M. Mulu-Moore ◽  
Amy R. Winebarger ◽  
Harry P. Warren

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