Results 101 to 110 of about 3,254 (234)
Heater‐induced ionization inferred from spectrometric airglow measurements
Spectrographic airglow measurements were made during an ionospheric modification experiment at High Frequency Active Auroral Research Program on 12 March 2013. Artificial airglow enhancements at 427.8, 557.7, 630.0, 777.4, and 844.6 nm were observed.
Bernhardt, P. A. +17 more
core +1 more source
Resolving thermospheric vertical wind ambiguities and energy processes
This study applies a generalized vertical coordinate system approach alongside thermodynamic control volume analysis to explore the nuanced interpretations of energy transfer processes associated with vertical motion in the thermosphere.
Jeffrey P. Thayer +2 more
doaj +1 more source
Nightside Detection of a Large‐Scale Thermospheric Wave Generated by a Solar Eclipse
The generation of a large‐scale wave in the upper atmosphere caused by a solar eclipse was first predicted in the 1970s, but the experimental evidence remains sparse and comprises mostly indirect observations. This study presents observations of the wind
B. J. Harding +3 more
doaj +1 more source
Impact of lower atmospheric scattering on ground-based optical thermospheric wind observations with spatially uneven airglow [PDF]
Scattered airglow emissions in the lower atmosphere can bias ground-based interferometer observations of thermospheric winds, particularly when airglow brightness becomes spatially uneven due to auroras. During two geomagnetic storms with visible auroras
X. Wei +19 more
doaj +1 more source
Simultaneous measurements of high-frequency pump-enhanced airglow and ionospheric temperatures at auroral latitudes [PDF]
P(論文)Simultaneous measurements of enhanced airglow at 6300 A and plasma temperatures from transmitting a powerful high frequency electromagnetic pump wave from the EISCAT-Heating facility into the ionospheric F region at auroral latitudes are reported ...
Brändström, B. +13 more
core +1 more source
Characterizing both the CO2 distribution and wind dynamics in the Martian mesosphere and lower thermosphere is vital for planetary atmospheric science and mission planning. In this work, we propose a novel dual-channel passive limb-viewing imaging system
Yanqiang Wang +6 more
doaj +1 more source
Disentangling Stellar and Airglow Emission Lines from HST-COS Spectra
H I Ly$\alpha$ (1215.67 \r{A}) and the O I triplet (1302.17, 1304.86, and 1306.03 \r{A}) are bright far-ultraviolet (FUV) emission lines that trace the stellar chromosphere.
France, Kevin +3 more
core
Airglow observations from ELOISE
In August and September 2015, the Defence Science and Technology Group (DST Group) undertook the Elevation-scanned Oblique Incidence Sounder Experiment (ELOISE): a unique campaign to observe and characterise mid-latitude ionospheric disturbances across ...
Pederick, L. +4 more
core
Spectroscopy of a mesospheric ghost reveals iron emissions. [PDF]
Passas-Varo M +8 more
europepmc +1 more source
Airglow monitoring by one-pixel detector
International audienceThe night time airglow is a dynamic phenomenon that acts as a background for the detection of the extensive air shower (EAS) fluorescence. It is a mandatory task to monitor this background for the ground-based telescopes and for the
Gorodetzky, P. +5 more
core +1 more source

