Charged particle and photon interactions with matter: recent advances, applications, and interfaces
Y Hatano, Y Katsumura, A Mozumder - 2010 - books.google.com
Covering state-of-the-art advances, novel applications, and future perspectives, this volume
presents new directions on the basic studies of charged particle and photon interactions with …
presents new directions on the basic studies of charged particle and photon interactions with …
The production of Titan's ultraviolet nitrogen airglow
MH Stevens, J Gustin, JM Ajello… - Journal of …, 2011 - Wiley Online Library
The Cassini Ultraviolet Imaging Spectrograph (UVIS) observed Titan's dayside limb in the
extreme ultraviolet (EUV) and far ultraviolet (FUV) on 22 June 2009 from a mean distance of …
extreme ultraviolet (EUV) and far ultraviolet (FUV) on 22 June 2009 from a mean distance of …
Integral cross sections for the electron-impact excitation of the , , , , , , and states of N
CP Malone, PV Johnson, X Liu, B Ajdari, I Kanik… - Physical Review A …, 2012 - APS
Integral cross sections for electron-impact excitation out of the ground-state level X 1 Σ
g+(v′′= 0) to the b 1 Π u, c 3 1 Π u, o 3 1 Π u, b′ 1 Σ u+, c 4′ 1 Σ u+, G 3 Π u, and F 3 Π …
g+(v′′= 0) to the b 1 Π u, c 3 1 Π u, o 3 1 Π u, b′ 1 Σ u+, c 4′ 1 Σ u+, G 3 Π u, and F 3 Π …
Oscillator strength and linewidth measurements of dipole-allowed transitions in N214 between 93.5 and 99.5 nm
G Stark, KP Huber, K Yoshino, PL Smith… - The Journal of chemical …, 2005 - pubs.aip.org
Oscillator strength and linewidth measurements of dipole-allowed transitions in N214 between
93.5 and 99.5nm | The Journal of Chemical Physics | AIP Publishing Skip to Main Content …
93.5 and 99.5nm | The Journal of Chemical Physics | AIP Publishing Skip to Main Content …
Titan airglow spectra from Cassini ultraviolet imaging spectrograph (UVIS): Euv analysis
We present the first UV airglow observations of Titan's atmosphere by the Ultraviolet Imaging
Spectrograph (UVIS) on Cassini. Using one spectral channel in the EUV from 561–1182 Å …
Spectrograph (UVIS) on Cassini. Using one spectral channel in the EUV from 561–1182 Å …
Rotational effects in the band oscillator strengths and predissociation linewidths for the lowest Πu1–XΣg+ 1 transitions of N2
A coupled-channel Schrödinger equation (CSE) model of N 2 photodissociation, which
includes the effects of all interactions between the b, c, and o Π u 1 and the C and C′ Π …
includes the effects of all interactions between the b, c, and o Π u 1 and the C and C′ Π …
Lifetime and predissociation yield of N214bΠu1 (v= 1) revisited: Effects of rotation
BR Lewis, ST Gibson, JP Sprengers… - The Journal of …, 2005 - pubs.aip.org
Coupled-channel Schrödinger-equation calculations of the lifetime of the b (v= 1) level of N
2 14 reveal strong rotational effects, with extreme lifetime shortening at high J as a result of …
2 14 reveal strong rotational effects, with extreme lifetime shortening at high J as a result of …
The high-resolution extreme-ultraviolet spectrum of N2 by electron impact
AN Heays, JM Ajello, A Aguilar… - The Astrophysical …, 2014 - iopscience.iop.org
We have analyzed high-resolution (FWHM= 0.2 Å) extreme-ultraviolet (EUV, 800–1350 Å)
laboratory emission spectra of molecular nitrogen excited by an electron impact at 20 and …
laboratory emission spectra of molecular nitrogen excited by an electron impact at 20 and …
Experimental and coupled‐channels investigation of the radiative properties of the N2c′41Σu+ − X1Σg+ band system
X Liu, DE Shemansky, CP Malone… - Journal of …, 2008 - Wiley Online Library
The emission properties of the N2c′ 41Σu+− X1Σg+ band system have been investigated in
a joint experimental and coupled‐channels theoretical study. Relative intensities of the c …
a joint experimental and coupled‐channels theoretical study. Relative intensities of the c …
Molecular nitrogen Carroll‐Yoshino v′ = 0 emission in the thermospheric dayglow as seen by the Far Ultraviolet Spectroscopic Explorer
J Bishop, MH Stevens… - Journal of Geophysical …, 2007 - Wiley Online Library
Molecular nitrogen (N2) Carroll‐Yoshino excitation is of considerable interest in the analysis
of EUV‐FUV observations obtained from several solar system objects (Earth, Titan, and …
of EUV‐FUV observations obtained from several solar system objects (Earth, Titan, and …