Daniel J. Emmons
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View article: Reply on RC2
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View article: A comparison of modeled daytime E-regions from E-PROBED and PyIRI with ionosonde observations
A comparison of modeled daytime E-regions from E-PROBED and PyIRI with ionosonde observations Open
While the F-region is the primary focus of many ionospheric models because it contains the peak electron density, the E-region is an important region for ionospheric conductivities and high-frequency radio propagation. This study analyzes …
View article: Magnetic Field Variability as a Consistent Predictor of Solar Flares
Magnetic Field Variability as a Consistent Predictor of Solar Flares Open
Solar flares are intense bursts of electromagnetic radiation that occur due to a rapid destabilization and reconnection of the magnetic field. While preflare signatures and trends have been investigated from magnetic observations prior to …
View article: Magnetic Field Variability as a Consistent Predictor of Solar Flares
Magnetic Field Variability as a Consistent Predictor of Solar Flares Open
Solar flares are intense bursts of electromagnetic radiation, which occur due to a rapid destabilization and reconnection of the magnetic field. While pre-flare signatures and trends have been investigated from magnetic observations prior …
View article: Global Sporadic‐E Prediction and Climatology Using Deep Learning
Global Sporadic‐E Prediction and Climatology Using Deep Learning Open
Sporadic‐E is an ionospheric phenomenon defined by strong layers of plasma which may interfere with radio wave propagation. In this work, we develop deep learning models to improve the understanding of , including the presence, intensity a…
View article: Simultaneous observations of irregular sporadic E structures using the LWA and a DPS4D
Simultaneous observations of irregular sporadic E structures using the LWA and a DPS4D Open
Multi-instrument studies have recently shed new light on the morphology of sporadic E, especially intense sporadic E. Here we present simultaneous observations of dense sporadic E ( ) structures using the Long Wavelength Array (LWA) radio…
View article: Analyzing LF/VLF lightning waveforms to estimate D-region electron density profiles
Analyzing LF/VLF lightning waveforms to estimate D-region electron density profiles Open
View article: Corrigendum: Global empirical model of sporadic-E occurrence rates
Corrigendum: Global empirical model of sporadic-E occurrence rates Open
View article: HF Radar Observations and Modeling of the Impact of the 8 April 2024 Total Solar Eclipse on the Ionosphere‐Thermosphere System
HF Radar Observations and Modeling of the Impact of the 8 April 2024 Total Solar Eclipse on the Ionosphere‐Thermosphere System Open
The path of totality of the 8 April 2024 solar eclipse traversed the fields‐of‐view of four US SuperDARN radars. This rare scenario provided an excellent opportunity to monitor the large‐scale ionospheric response to the eclipse. In this s…
View article: Global Empirical Model of Sporadic-E Occurrence Rates
Global Empirical Model of Sporadic-E Occurrence Rates Open
Intense ionization enhancements in the Earth’s ionosphere, known as sporadic-E ( ), can degrade and severely disrupt the propagation of radio signals. Although many previous studies have analyzed the characteristics and morphologies of sp…
View article: Development of the Ionospheric E‐Region Prompt Radio Occultation Based Electron Density (E‐PROBED) Model
Development of the Ionospheric E‐Region Prompt Radio Occultation Based Electron Density (E‐PROBED) Model Open
This work reports the development of the first version of the E‐region Prompt Radio Occultation Based Electron Density (E‐PROBED) Model. This is an empirical model of E‐region electron density (Ne) between 90 and 120 km developed using rad…
View article: Analysis of modeled 3D solar magnetic field during 30 X/M-class solar flares
Analysis of modeled 3D solar magnetic field during 30 X/M-class solar flares Open
Using non-linear force free field (NLFFF) extrapolation, 3D magnetic fields were modeled from the 12-min cadence Solar Dynamics Observatory Helioseismic and Magnetic Imager (HMI) photospheric vector magnetograms, spanning a time period of …
View article: Editorial: Observations and simulations of layering phenomena in the middle/upper atmosphere and ionosphere
Editorial: Observations and simulations of layering phenomena in the middle/upper atmosphere and ionosphere Open
EDITORIAL article Front. Astron. Space Sci., 12 January 2024Sec. Space Physics Volume 10 - 2023 | https://doi.org/10.3389/fspas.2023.1361434
View article: Detection and Classification of Sporadic E Using Convolutional Neural Networks
Detection and Classification of Sporadic E Using Convolutional Neural Networks Open
In this work, convolutional neural networks (CNN) are developed to detect and characterize sporadic E ( E s ), demonstrating an improvement over current methods. This includes a binary classification model to determine if E s is present, f…
View article: Improved models for estimating sporadic-E intensity from GNSS radio occultation measurements
Improved models for estimating sporadic-E intensity from GNSS radio occultation measurements Open
Several models for estimating sporadic-E intensity from Global Navigation Satellite System (GNSS) radio occultation (RO) observation have previously been developed using a single perturbation or intensity parameter, such as phase-based tot…
View article: Impacts of Kelvin-Helmholtz billow formation on GNSS radio occultation measurements of sporadic-E
Impacts of Kelvin-Helmholtz billow formation on GNSS radio occultation measurements of sporadic-E Open
Global Navigation Satellite System (GNSS) Radio Occultation (RO) has shown great promise for monitoring sporadic-E layers. However, extracting sporadic-E information from RO signals remains a difficult task due to the many unknown paramete…
View article: Comparison of a Bottom-Up GNSS Radio Occultation Method to Measure D- and E-Region Electron Densities with Ionosondes and FIRI
Comparison of a Bottom-Up GNSS Radio Occultation Method to Measure D- and E-Region Electron Densities with Ionosondes and FIRI Open
High-frequency skywave propagation can be heavily impacted by D- and E-region dynamics requiring accurate global measurements to optimize performance. A standard measurement technique is to use ionosondes, but they are unable to measure be…
View article: Global Ionospheric Electron Density from GNSS-POD Limb Measurements
Global Ionospheric Electron Density from GNSS-POD Limb Measurements Open
GNSS-LEO radio links from Precise Orbital Determination (POD) and Radio Occultation (RO) antennas have been used increasingly in studying and monitoring the global ionospheric electron density (Nₑ). In this study we developed an optimal es…
View article: Optimal Estimation Inversion of Ionospheric Electron Density from GNSS-POD Limb Measurements: Part II-Validation and Comparison Using NmF2 and hmF2
Optimal Estimation Inversion of Ionospheric Electron Density from GNSS-POD Limb Measurements: Part II-Validation and Comparison Using NmF2 and hmF2 Open
A growing number of SmallSat/CubeSat constellations with high-rate (50–100 Hz) global navigation satellite system radio occultations (GNSS-RO) as well as low-rate (1 Hz) precise orbit determination (GNSS-POD) limb-viewing capabilities prov…
View article: Optimal Estimation Inversion of Ionospheric Electron Density from GNSS-POD Limb Measurements: Part I-Algorithm and Morphology
Optimal Estimation Inversion of Ionospheric Electron Density from GNSS-POD Limb Measurements: Part I-Algorithm and Morphology Open
GNSS-LEO radio links from Precise Orbital Determination (POD) and Radio Occultation (RO) antennas have been used increasingly in characterizing the global 3D distribution and variability of ionospheric electron density (Ne). In this study,…
View article: Evolution of coronal magnetic field parameters during X5.4 solar flare
Evolution of coronal magnetic field parameters during X5.4 solar flare Open
The coronal magnetic field over NOAA Active Region 11,429 during a X5.4 solar flare on 7 March 2012 is modeled using optimization based Non-Linear Force-Free Field extrapolation. Specifically, 3D magnetic fields were modeled for 11 timeste…
View article: Characterization of Intense Sporadic-E Through the Combination of Ionosonde Data and Amateur Radio Observations
Characterization of Intense Sporadic-E Through the Combination of Ionosonde Data and Amateur Radio Observations Open
View article: A Statistical Analysis of Sporadic-E Characteristics Associated with GNSS Radio Occultation Phase and Amplitude Scintillations
A Statistical Analysis of Sporadic-E Characteristics Associated with GNSS Radio Occultation Phase and Amplitude Scintillations Open
Statistical GNSS-RO measurements of phase and amplitude scintillation are analyzed at the mid-latitudes in the local summer for a 100 km altitude. These conditions are known to contain frequent sporadic-E, and the S4-σϕ trends provide insi…
View article: Global Sporadic‐E Occurrence Rate Climatology Using GPS Radio Occultation and Ionosonde Data
Global Sporadic‐E Occurrence Rate Climatology Using GPS Radio Occultation and Ionosonde Data Open
An updated global climatology of blanketing sporadic E (E s ) is developed from a combined data set of Global Positioning System (GPS) radio occultation (RO) and ground‐based ionosonde soundings over the period of September 2006–January 20…
View article: Long-distance propagation of 162 MHz shipping information links associated with sporadic E
Long-distance propagation of 162 MHz shipping information links associated with sporadic E Open
Sporadic E layers form in the daytime midlatitude ionosphere as a result of wind shears in the mesosphere–lower-thermosphere compressing metallic ions of meteoric origin into dense, narrow sheets extending over hundreds or thousands of kil…
View article: Comment on amt-2022-214
Comment on amt-2022-214 Open
Abstract. Sporadic E layers form in the daytime midlatitude ionosphere as a result of wind shears in the mesosphereâlower-thermosphere compressing metallic ions of meteoric origin into dense, narrow sheets extending over…
View article: Long Distance Propagation of 162-MHz Shipping Information Links Associated with Sporadic-E
Long Distance Propagation of 162-MHz Shipping Information Links Associated with Sporadic-E Open
Anomalous long distance reports of Automatic Identification System (AIS) shipping transmissions were received by a United States Coast Guard terrestrial monitoring network in the eastern United States and Puerto Rico. 6677 signals were ide…
View article: Reply on AC1
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Abstract. Sporadic E layers form in the daytime midlatitude ionosphere as a result of wind shears in the mesosphere–lower-thermosphere compressing metallic ions of meteoric origin into dense, narrow sheets extending over h…
View article: Comment on amt-2022-214
Comment on amt-2022-214 Open
Abstract. Sporadic E layers form in the daytime midlatitude ionosphere as a result of wind shears in the mesosphereâlower-thermosphere compressing metallic ions of meteoric origin into dense, narrow sheets extending over…