Venus water loss is dominated by HCO+ dissociative recombination

  • M. S. Chaffin
  • , E. M. Cangi
  • , B. S. Gregory
  • , R. V. Yelle
  • , J. Deighan
  • , R. D. Elliott
  • , H. Gröller

Research output: Contribution to journalArticlepeer-review

Fingerprint

Dive into the research topics of 'Venus water loss is dominated by HCO+ dissociative recombination'. Together they form a unique fingerprint.
Sort by

Physics

Earth and Planetary Sciences

Keyphrases