Results 71 to 80 of about 4,644 (217)
The relatively unconstrained internal structure of Venus is a missing piece in our understanding of the formation and evolution of the Solar System. Detection of seismic waves generated by venusquakes is crucial to determine the seismic structure of ...
Raphael F. Garcia +17 more
doaj +1 more source
Statistics and variability of the altitude of elves
From June 2008 to January 2016 nearly 800 elves have been recorded by a low‐light camera in northeastern Spain. Elves occur in this region mainly over the lower topped cold air mass maritime thunderstorms, peaking from November to January.
Oscar A. van derVelde, Joan Montanyà
doaj +1 more source
Airglow Studies in India [PDF]
84-101 Airglow radiations in different portions of the eletromagnetic spectrum have been studied in many aspects at middle and high latitude stations, from ground-based observations, rockets and satellites.
Agashe, V V
core
OMTI Airglow Temperature Photometer (ATP) at Kototabang, Indonesia
Optical Mesosphere Thermosphere Imagers (OMTIs) Airglow Temperature Photometer (ATP) Data. The ATP measures airglow rotational temperature and airglow intensity in the mesopause region at 80-100km altitudes through the OH and O2 airglow emission lines.
Kazuo Shiokawa +2 more
core
Origin of [OI] 5577 in the airglow and the aurora
The distribution of 5577 zenith intensities at stations in the subauroral zone is found to be unimodal with no discontinuity at the visual threshold.
Roach, Franklin K. ; McCaulley, James W. ; Marovich, Edward
core +1 more source
Upper atmosphere research at the Instituto Nacional de Pesquisas Espaciais of Brazil [PDF]
Upper atmosphere research at the Instituto Nacional de Pesquisas Espaciais of Brazil is concentrated in the areas of photochemistry and dynamics of the mesopause and lower thermosphere, middle atmosphere climatology, and stratospheric aerosols.
D. M. Simonich +5 more
doaj
First observation of the Venus UV dayglow at limb from SPICAV/VEX
We present the first limb observations of the dayglow emissions by the UV channel of SPICAV aboard Venus Express between October and December 2011. The CO Cameron bands between 180–260 nm and CO2+ doublet at 289 nm are clearly identified for the first ...
Jean‐Yves Chaufray +2 more
doaj +1 more source
A rocket-borne airglow photometer [PDF]
The design of a rocket-borne photometer to measure the airglow emission of ionized molecular nitrogen in the 391.4 nm band is presented. This airglow is a well known and often observed phenomenon of auroras, where the principal source of ionization is ...
Paarmann, L. D., Smith, L. G.
core
Temporal and latitudinal 5577 Å airglow variations
From 32 000 [O1] 5577 Å airglow limb observations made between April 1971 and December 1972 from the ISIS-2 satellite, the major temporal and spatial night airglow features have been identified.
J. S. Murphree +2 more
core +1 more source
Previously unreported optical emissions generated during ionospheric heating [PDF]
Several radio-induced optical emissions were generated during an ionospheric heating experiment performed at the High Power Auroral Stimulation (HIPAS) facility near Two Rivers, Alaska.
Gustavsson, B. +5 more
core +1 more source

