An ISEE 3 high time resolution study of interplanetary parameter correlations with magnetospheric activity

1983 ◽  
Vol 88 (A8) ◽  
pp. 6230 ◽  
Author(s):  
D. N. Baker ◽  
R. D. Zwickl ◽  
S. J. Bame ◽  
E. W. Hones ◽  
B. T. Tsurutani ◽  
...  
2019 ◽  
Vol 882 (2) ◽  
pp. 133
Author(s):  
D. Kaur ◽  
N. D. R. Bhat ◽  
S. E. Tremblay ◽  
R. M. Shannon ◽  
S. J. McSweeney ◽  
...  

1982 ◽  
Vol 2 (7) ◽  
pp. 75-79 ◽  
Author(s):  
V.M. Balebanov ◽  
O.L. Vaisberg ◽  
E.M. Vasiliev ◽  
G.N. Zastenker ◽  
V.P. Evdokimov ◽  
...  

1982 ◽  
Vol 30 (6) ◽  
pp. 537-543 ◽  
Author(s):  
S.-I. Akasofu ◽  
J.F. Carbary ◽  
C.-I. Meng ◽  
J.P. Sullivan ◽  
R.P. Lepping

1997 ◽  
Vol 24 (8) ◽  
pp. 987-990 ◽  
Author(s):  
D. Lummerzheim ◽  
M. Brittnacher ◽  
D. Evans ◽  
G. A. Germany ◽  
G. K. Parks ◽  
...  

1981 ◽  
Vol 8 (2) ◽  
pp. 179-182 ◽  
Author(s):  
D. N. Baker ◽  
E. W. Hones ◽  
J. B. Payne ◽  
W. C. Feldman

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Vol 223 ◽  
pp. 117241 ◽  
Author(s):  
Rosa M. Flores ◽  
Elif Mertoğlu ◽  
Hüseyin Özdemir ◽  
Bülent O. Akkoyunlu ◽  
Göksel Demir ◽  
...  

1994 ◽  
Vol 144 ◽  
pp. 431-434
Author(s):  
M. Minarovjech ◽  
M. Rybanský

AbstractThis paper deals with a possibility to use the ground-based method of observation in order to solve basic problems connected with the solar corona research. Namely:1.heating of the solar corona2.course of the global cycle in the corona3.rotation of the solar corona and development of active regions.There is stressed a possibility of high-time resolution of the coronal line photometer at Lomnický Peak coronal station, and use of the latter to obtain crucial observations.


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