Observing the Solar Wind with Interplanetary Scintillation
Observing the Solar Wind with Interplanetary Scintillation
Observing the Solar Wind with Interplanetary Scintillation
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Coronal Mass Ejections (CMEs)<br />
●<br />
Presence of CME can<br />
be indicated by<br />
different features:<br />
●<br />
●<br />
●<br />
Substantial changes in<br />
form of crosscorrelation<br />
function<br />
Sudden increase in<br />
scintillation level<br />
Negative lobe on<br />
cross-correlation<br />
function.<br />
Large “negative lobe” indicates magnetic field rotation
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