We discuss here two extraordinary increases of cosmic ray intensity that were observed by Voyager1 in the last 1.1 AU before it crossed the heliopause in August , 2012 , at 121.7AU .
These two increases are roughly similar in amplitude and result in a total increase of \sim 1 GV cosmic ray nuclei of over 50 % and of 0.01GV electrons of a factor \sim 2 .
During the 1 ^ { st } increase the changes in the magnetic , B field are small .
After the 1 ^ { st } increase , the B field changes become large and during the 2 ^ { nd } increae the B field variations and the cosmic ray changes are correlated to within \pm one day .
The intensity variations of H and He nuclei and electrons during these time intervals are measured from 0.1 to over 1 GV.The total increae of GCR in the two increases resemble those to be expected from a simple force field ” like ” solar modulation with a modulation potential \sim 80 MV .
This is nearly 1/3 of the total modulation potential \sim 250 MV that is required to produce the modulation of these particles observed at the Earth at the 2009 sunspot minimum and adds a new aspect to the heliospheric modulation .