Javascript must be enabled to continue!
Nightside Neutral Density Disturbances Collocated With Equatorial Plasma Irregularities Above 450 km: GRACE and GRACE‐FO Observations in 2002–2022
View through CrossRef
AbstractWe investigate the climatology of Neutral Density Disturbances (NDDs) collocated with Equatorial Plasma Irregularities (EPIs) at altitudes above 450 km by using 20 years of data from the Gravity Recovery and Climate Experiment (GRACE) and GRACE‐FO satellites. Electron density data are used to detect EPIs, and thermospheric neutral density measured onboard the same spacecraft serves to identify EPI‐related NDDs. A detailed analysis focused on the morphological similarity between electron and neutral densities. To examine the relationship between EPI and NDD, statistical dependences of EPIs and NDDs on season/longitude (S/L), Magnetic Latitude (MLAT), Magnetic Local Time (MLT), and solar activity have been checked. As a first step, we confirmed that the EPI climatology in GRACE satellite data is consistent with previous reports. Then, it is found that the lower the neutral density in the background upper thermosphere, the higher the probability that EPI can accompany NDDs. We suggest that the vertical plasma advection surrounding EPI can result in neutral density disturbance, of which the efficiency depends on the background neutral scale height or temperature. The colder the thermosphere, the shorter its vertical scale height (or the lower the background neutral density), which can make the plasma advection leave measurable imprints on the neutral density.
American Geophysical Union (AGU)
Title: Nightside Neutral Density Disturbances Collocated With Equatorial Plasma Irregularities Above 450 km: GRACE and GRACE‐FO Observations in 2002–2022
Description:
AbstractWe investigate the climatology of Neutral Density Disturbances (NDDs) collocated with Equatorial Plasma Irregularities (EPIs) at altitudes above 450 km by using 20 years of data from the Gravity Recovery and Climate Experiment (GRACE) and GRACE‐FO satellites.
Electron density data are used to detect EPIs, and thermospheric neutral density measured onboard the same spacecraft serves to identify EPI‐related NDDs.
A detailed analysis focused on the morphological similarity between electron and neutral densities.
To examine the relationship between EPI and NDD, statistical dependences of EPIs and NDDs on season/longitude (S/L), Magnetic Latitude (MLAT), Magnetic Local Time (MLT), and solar activity have been checked.
As a first step, we confirmed that the EPI climatology in GRACE satellite data is consistent with previous reports.
Then, it is found that the lower the neutral density in the background upper thermosphere, the higher the probability that EPI can accompany NDDs.
We suggest that the vertical plasma advection surrounding EPI can result in neutral density disturbance, of which the efficiency depends on the background neutral scale height or temperature.
The colder the thermosphere, the shorter its vertical scale height (or the lower the background neutral density), which can make the plasma advection leave measurable imprints on the neutral density.
Related Results
The terminator and nightside ionosphere of Mars as seen by Mars Express MaRS radio science
The terminator and nightside ionosphere of Mars as seen by Mars Express MaRS radio science
Fig. 1:. 7 MaRS terminator/nightside electron density profiles observed between August and September 2005. All profiles have an offset of 3·1010 m−3 to the neighbouring profiles. T...
The spatial distribution of dust in the inner comae of comets: Evidence for and modelling of nightside emission
The spatial distribution of dust in the inner comae of comets: Evidence for and modelling of nightside emission
<p>Spacecraft imaging of the inner comae of 1P/Halley (Giotto/HMC) and 19P/Borrelly (DS1/MICAS) indicated unexpectedly low ratios for the dust brightness above the da...
Magnetohydrodynamics enhanced radio blackout mitigation system for spacecraft during planetary entries
Magnetohydrodynamics enhanced radio blackout mitigation system for spacecraft during planetary entries
(English) Spacecraft entering planetary atmospheres are enveloped by a plasma layer with high levels of ionization, caused by the extreme temperatures in the shock layer. The charg...
Venus nightside radiances data analysis and model comparison in view of upcoming Venus missions
Venus nightside radiances data analysis and model comparison in view of upcoming Venus missions
The 2030s will see the arrival of several spacecrafts, with multiple spectrometers designed to measure the atmosphere or surface using the transparency windows through the clouds o...
Linking White‐Tailed Deer Density, Nutrition, and Vegetation in a Stochastic Environment
Linking White‐Tailed Deer Density, Nutrition, and Vegetation in a Stochastic Environment
ABSTRACT
Density‐dependent behavior underpins white‐tailed deer (
Odocoileus virginianus
) theory and...
Ionospheric Plasma Irregularities During Intense geomagnetic storms of Solar Cycle 25
Ionospheric Plasma Irregularities During Intense geomagnetic storms of Solar Cycle 25
Abstract. This study aims to characterize several key aspects of the ionosphere during intense geomagnetic storms that occurred on March 23–25, 2023, April 23–25, 2023, November 4–...
What drives Mars’ nightside Ionosphere? Insights from in situ and remote sensing
What drives Mars’ nightside Ionosphere? Insights from in situ and remote sensing
Mars’ nightside ionosphere is highly variable and poorly understood, with several internal, external, and local factors affecting multiple sources of ionospheric plasma, all combin...
Convectively Coupled Equatorial Waves in High-Resolution Hadley Centre Climate Models
Convectively Coupled Equatorial Waves in High-Resolution Hadley Centre Climate Models
Abstract
A methodology for diagnosing convectively coupled equatorial waves is applied to output from two high-resolution versions of atmospheric models, the Hadley ...

