Transport of charged particle pulses in interplanetary magnetic fields

1995 ◽  
Vol 45 (9) ◽  
pp. 767-775
Author(s):  
Y. I. Fedorov ◽  
B. A. Shakhov ◽  
M. Stehlík
Keyword(s):  
Charged Particle ◽  
Magnetic Fields ◽  
Interplanetary Magnetic Fields

Cosmic-ray fluctuations and interplanetary magnetic fields

1993 ◽  
Vol 199 (1) ◽  
pp. 125-132 ◽  
Author(s):  
K. Kudela ◽  
M. Slivka ◽  
M. Stehl�k ◽  
A. Geranios
Keyword(s):  
Magnetic Fields ◽  
Cosmic Ray ◽  
Interplanetary Magnetic Fields

scholarly journals Magnetosonic Mach number dependence of the efficiency of reconnection between planetary and interplanetary magnetic fields

2009 ◽  
Vol 114 (A7) ◽  
pp. n/a-n/a ◽  
Author(s):  
A. Grocott ◽  
S. V. Badman ◽  
S. W. H. Cowley ◽  
S. E. Milan ◽  
J. D. Nichols ◽  
...  
Keyword(s):  
Mach Number ◽  
Magnetic Fields ◽  
Interplanetary Magnetic Fields

scholarly journals Extremely intense (SML ≤–2500 nT) substorms: isolated events that are externally triggered?

2015 ◽  
Vol 33 (5) ◽  
pp. 519-524 ◽  
Author(s):  
B. T. Tsurutani ◽  
R. Hajra ◽  
E. Echer ◽  
J. W. Gjerloev
Keyword(s):  
Solar Wind ◽  
Magnetic Fields ◽  
Magnetic Storm ◽  
Solar Wind Plasma ◽  
Magnetic Storms ◽  
Input Energy ◽  
Stored Energy ◽  
Ionospheric Currents ◽  
Interplanetary Magnetic Fields ◽  
Very High

Abstract. We examine particularly intense substorms (SML ≤–2500 nT), hereafter called "supersubstorms" or SSS events, to identify their nature and their magnetic storm dependences. It is found that these intense substorms are typically isolated events and are only loosely related to magnetic storms. SSS events can occur during super (Dst ≤–250 nT) and intense (−100 nT ≥ Dst >–250) magnetic storms. SSS events can also occur during nonstorm (Dst ≥–50 nT) intervals. SSSs are important because the strongest ionospheric currents will flow during these events, potentially causing power outages on Earth. Several SSS examples are shown. SSS events appear to be externally triggered by small regions of very high density (~30 to 50 cm−3) solar wind plasma parcels (PPs) impinging upon the magnetosphere. Precursor southward interplanetary magnetic fields are detected prior to the PPs hitting the magnetosphere. Our hypothesis is that these southward fields input energy into the magnetosphere/magnetotail and the PPs trigger the release of the stored energy.

scholarly journals Anomalous magnetosheath flows and distorted subsolar magnetopause for radial interplanetary magnetic fields

2009 ◽  
Vol 36 (18) ◽  
Author(s):  
J.-H. Shue ◽  
J.-K. Chao ◽  
P. Song ◽  
J. P. McFadden ◽  
A. Suvorova ◽  
...  
Keyword(s):  
Magnetic Fields ◽  
Interplanetary Magnetic Fields
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