Changes between Version 3 and Version 4 of MP2019

Timestamp:

Aug 16, 2018 6:42:04 PM (6 years ago)

Author:

mhapgood

Comment:

--

MP2019

@@ -10 +10 @@
 
 The figure below shows the relative timings of the inbound crossings of the Cluster spacecraft. Two additional lines have been included in the plot:
-a. the bow shock crossing time of C1 is shown as a dashed black line. This highlights how there is a period (roughly 20 January to 14 April) when C3 and C4 are likely to cross the magnetopause whilst C1 is still in the solar wind and C2 is the magnetosheath just outside the magnetopause.
+a. the bow shock crossing time of C1 is shown as a dashed black line. This highlights how there is a period (roughly 20 January to 14 April) when C3 and C4 are likely to cross the magnetopause whilst C1 is still in the solar wind and C2 is in the magnetosheath just outside the magnetopause.
 b. the crossing time of the centroid of C3 and C4 is shown as a dashed light blue line. 
 
@@ -17 +17 @@
 == Outbound crossings ==
 
+The figure below shows the relative timings of the outbound crossings of the Cluster spacecraft. One additional line has been included in the plot:
+a. the crossing time of the centroid of C2, C3 and C4 is shown as a dashed light blue line. 
 
 [[Image(outbound_mp_2019.png)]]