Temperature dependence of magic number and first hydrated shell of various core water cluster ions Y−(H2O)n (Y = O2, HOx, NOx, COx) in atmospheric pressure negative corona discharge mass spectrometry

Observations of different core water clu

Observations of different core water cluster ions Y−(H2O)n (Y = O2, HOx, NOx, COx) and magic number in atmospheric pressure negative corona discharge mass spectrometry

✍ Kanako Sekimoto; Mitsuo Takayama 📂 Article 📅 2010 🏛 John Wiley and Sons 🌐 English ⚖ 405 KB

## Abstract Reliable mass spectrometry data from large water clusters Y^−^(H~2~O)~__n__~ with various negative core ions Y^−^ such as O~2~^−^, HO^−^, HO~2~^−^, NO~2~^−^, NO~3~^−^, NO~3~^−^(HNO~3~)~2~, CO~3~^−^ and HCO~4~^−^ have been obtained using atmospheric pressure negative corona discharge mas

Temperature dependence of magic number and first hydrated shell of various core water cluster ions Y−(H2O)n (Y&#xa0;=&#xa0;O2, HOx, NOx, COx) in atmospheric pressure negative corona discharge mass spectrometry

Temperature dependence of magic number and first hydrated shell of various core water cluster ions Y−(H2O)n (Y = O2, HOx, NOx, COx) in atmospheric pressure negative corona discharge mass spectrometry