scholarly journals A Statistical Study of Slow-Mode Shocks Observed by MMS in the Dayside Magnetopause

2018 ◽  
Vol 45 (10) ◽  
pp. 4675-4684
Author(s):  
N. K. Walia ◽  
K. Seki ◽  
M. Hoshino ◽  
T. Amano ◽  
N. Kitamura ◽  
...  
1994 ◽  
Vol 99 (A8) ◽  
pp. 14815 ◽  
Author(s):  
L. Scurry ◽  
C. T. Russell ◽  
J. T. Gosling

2016 ◽  
Vol 121 (1) ◽  
pp. 492-506 ◽  
Author(s):  
S. H. Lee ◽  
H. Zhang ◽  
Q.‐G. Zong ◽  
A. Otto ◽  
H. Rème ◽  
...  

1994 ◽  
Vol 99 (A12) ◽  
pp. 23705 ◽  
Author(s):  
D. W. Walthour ◽  
J. T. Gosling ◽  
B. U. Ö. Sonnerup ◽  
C. T. Russell

1994 ◽  
Vol 21 (7) ◽  
pp. 629-632 ◽  
Author(s):  
M. Yan ◽  
L. C. Lee

2016 ◽  
Vol 121 (7) ◽  
pp. 6480-6492 ◽  
Author(s):  
Jong-Sun Park ◽  
Jih-Hong Shue ◽  
Khan-Hyuk Kim ◽  
Gilbert Pi ◽  
Zdeněk Němeček ◽  
...  

1995 ◽  
Vol 15 (8-9) ◽  
pp. 501-506 ◽  
Author(s):  
D.W Walthour ◽  
B.U.Ö Sonnerup ◽  
C.T Russell

1976 ◽  
Vol 32 ◽  
pp. 675-683
Author(s):  
Keiichi Kodaira

SummaryExcess of [m1] index of Am stars, relative to normal stars, is statistically found to be correlated with rotation velocity; the coefficient is estimated at ∆׀m1׀ /∆V(km/sec) ˜ - 0.0007 among Am stars. This result supports the general view that slow rotation is essential for Am phenomena.


Sign in / Sign up

Export Citation Format

Share Document