Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95325/1/grl18052.pd
Coronal mass ejections (CMEs) have been recognized as the most energetic phenomenon in the heliosphe...
This thesis describes several studies of fundamental questions relating to the nature of coronal mas...
On 2015 January 6&-7, an interplanetary coronal mass ejection (ICME) was observed at L1. This event,...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95193/1/grl11810.pd
We analyze the physical origin of plasmas that are ejected from the solar corona. To address this is...
Interplanetary coronal mass ejection (ICME) associated plasma can exhibit signatures in elemental, i...
We present a novel procedure for deriving the physical properties of coronal mass ejections (CMEs) i...
We present results from a comparison of CME and slow solar wind ejecta detected at the ACE spacecraf...
We analyze the physical origin of plasmas that are ejected from the solar corona. To address this is...
We present the first analysis of the complete charge state distributions of heavy ions in interplane...
We examine Fe charge state distributions in the solar wind. The ionic composition of the solar wind ...
We examine Fe charge state distributions in the solar wind. The ionic composition of the solar wind ...
Solar wind ionic composition measurements are powerful tools in discriminating between different sou...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94738/1/jgra16138.pd
The solar wind ionic charge composition is a powerful tool to distinguish between the slow wind and ...
Coronal mass ejections (CMEs) have been recognized as the most energetic phenomenon in the heliosphe...
This thesis describes several studies of fundamental questions relating to the nature of coronal mas...
On 2015 January 6&-7, an interplanetary coronal mass ejection (ICME) was observed at L1. This event,...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95193/1/grl11810.pd
We analyze the physical origin of plasmas that are ejected from the solar corona. To address this is...
Interplanetary coronal mass ejection (ICME) associated plasma can exhibit signatures in elemental, i...
We present a novel procedure for deriving the physical properties of coronal mass ejections (CMEs) i...
We present results from a comparison of CME and slow solar wind ejecta detected at the ACE spacecraf...
We analyze the physical origin of plasmas that are ejected from the solar corona. To address this is...
We present the first analysis of the complete charge state distributions of heavy ions in interplane...
We examine Fe charge state distributions in the solar wind. The ionic composition of the solar wind ...
We examine Fe charge state distributions in the solar wind. The ionic composition of the solar wind ...
Solar wind ionic composition measurements are powerful tools in discriminating between different sou...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94738/1/jgra16138.pd
The solar wind ionic charge composition is a powerful tool to distinguish between the slow wind and ...
Coronal mass ejections (CMEs) have been recognized as the most energetic phenomenon in the heliosphe...
This thesis describes several studies of fundamental questions relating to the nature of coronal mas...
On 2015 January 6&-7, an interplanetary coronal mass ejection (ICME) was observed at L1. This event,...