Search engine for discovering works of Art, research articles, and books related to Art and Culture
ShareThis
Javascript must be enabled to continue!

Search for Martian Schumann Resonances

View through CrossRef
On Earth, electric discharges in thunderstorms produce ELF waves in the Earth-ionosphere waveguide that circles the globe. These waves give rise to Schumann resonances in the waveguide resonant cavity. These waves are also expected to occur at Venus, produced by strong lightning in the Venus atmosphere and at Mars produced by active dust devils or dust storms, during southern hemisphere summer, when the planet is near periapsis. Within dust storms, dust particles undergo triboelectric charging. The charge transfer leads to charge separation. A lightning discharge is expected to occur when the charge exceeds the breakdown strength of the media present. The transient electric discharge emits electromagnetic waves in the VLF/ELF range of frequency, leading to Schumann Resonance in the surface-ionospheric cavity. In a heterogeneous cavity, Schumann resonance modes are observable using an in-situ instrument. Recently has it been possible to search for these electromagnetic waves from the Mars surface using the UCLA-provided InSight fluxgate magnetometer. The weakness of the vertical component of ULF waves at Mars suggests that the subsurface is electrically conducting, allowing trapping of electromagnetic energy between the sub-surface and the ionosphere. The fundamental mode of Schumann resonance carries higher energy compared to there are more chances of observing the fundamental mode. Various values of the first mode are predicted in the literature for Mars like 13-14 Hz or between 9-14 Hz and 17.5 Hz. Even if the fundamental mode is above 10 Hz, the 20 Hz sampling rate will allow detection of an aliased signal. We examine the data obtained during Martian sandstorms for the possible existence of such waves. A large dust storm was detected on Mars beginning on InSight sols 40 to 50, and ending during sols 50 to 90. Examining the 20 Hz InSight magnetometer data during this period reveals no clearly identifiable Schumann Resonance signals within the bandwidth of the magnetometer.
Title: Search for Martian Schumann Resonances
Description:
On Earth, electric discharges in thunderstorms produce ELF waves in the Earth-ionosphere waveguide that circles the globe.
These waves give rise to Schumann resonances in the waveguide resonant cavity.
These waves are also expected to occur at Venus, produced by strong lightning in the Venus atmosphere and at Mars produced by active dust devils or dust storms, during southern hemisphere summer, when the planet is near periapsis.
Within dust storms, dust particles undergo triboelectric charging.
The charge transfer leads to charge separation.
A lightning discharge is expected to occur when the charge exceeds the breakdown strength of the media present.
The transient electric discharge emits electromagnetic waves in the VLF/ELF range of frequency, leading to Schumann Resonance in the surface-ionospheric cavity.
In a heterogeneous cavity, Schumann resonance modes are observable using an in-situ instrument.
Recently has it been possible to search for these electromagnetic waves from the Mars surface using the UCLA-provided InSight fluxgate magnetometer.
The weakness of the vertical component of ULF waves at Mars suggests that the subsurface is electrically conducting, allowing trapping of electromagnetic energy between the sub-surface and the ionosphere.
The fundamental mode of Schumann resonance carries higher energy compared to there are more chances of observing the fundamental mode.
Various values of the first mode are predicted in the literature for Mars like 13-14 Hz or between 9-14 Hz and 17.
5 Hz.
Even if the fundamental mode is above 10 Hz, the 20 Hz sampling rate will allow detection of an aliased signal.
We examine the data obtained during Martian sandstorms for the possible existence of such waves.
A large dust storm was detected on Mars beginning on InSight sols 40 to 50, and ending during sols 50 to 90.
Examining the 20 Hz InSight magnetometer data during this period reveals no clearly identifiable Schumann Resonance signals within the bandwidth of the magnetometer.

Related Results

Extreme planetary resonances: Study of high eccentricity and high inclination resonances in exoplanet systems
Extreme planetary resonances: Study of high eccentricity and high inclination resonances in exoplanet systems
Over the past 30 years, the number of confirmed exoplanetary systems has increased enormously, with nearly a thousand systems hosting multiple planets. The orbital architectures of...
A catalogue of Martian sound
A catalogue of Martian sound
IntroductionThe two microphones onboard the Perseverance rover have now been operating for more than three years on the surface of Mars. They have provided the first sound recordin...
Three-dimensional Morphological Analysis of Martian Rocks Using Zhurong Rover NaTeCam Images
Three-dimensional Morphological Analysis of Martian Rocks Using Zhurong Rover NaTeCam Images
This research delves into the three-dimensional (3D) morphological characteristics of Martian rocks, utilizing high-resolution images captured by the NaTeCam of China's Zhurong rov...
Evaluating the Science to Inform the Physical Activity Guidelines for Americans Midcourse Report
Evaluating the Science to Inform the Physical Activity Guidelines for Americans Midcourse Report
Abstract The Physical Activity Guidelines for Americans (Guidelines) advises older adults to be as active as possible. Yet, despite the well documented benefits of physical a...
Interannual variations of CO2 deposit in Martian caps from the HEND/Odyssey data.
Interannual variations of CO2 deposit in Martian caps from the HEND/Odyssey data.
<p>It is known that growing and sublimation of Martian snow caps is seen as seasonal variations of neutron flux above Martian polar regions. The surficial CO<s...
Vertical plasma drifts in magnetically controlled ionosphere of Mars 
Vertical plasma drifts in magnetically controlled ionosphere of Mars 
<p>Our focus in this paper is to explain the electron density (N<sub>e</sub>) profiles measured over the Martian high-latitude region by t...
New constraint of the Martian dynamo from surface magnetic survey by Zhurong rover
New constraint of the Martian dynamo from surface magnetic survey by Zhurong rover
The timing of the martian dynamo has always been an outstanding scientific issue in the evolution of Mars, as it provides the key implications for the evolution of the Martian core...
Acoustic Propagation in the Near‐Surface Martian Atmosphere
Acoustic Propagation in the Near‐Surface Martian Atmosphere
AbstractThis work introduces a comprehensive model of sound propagation on Mars, in light of the recent operation of several microphones on the Martian surface. The main outcome of...

Back to Top