- Asteroid Visiting Earth’s Neighborhood Brings its Own Face Mask 23 Apr, 2020
- REU Students’ Research & Presentations01 Apr, 2020
- Transforming the Arecibo Observatory into a Classroom31 Mar, 2020
- Arecibo Observatory re-enters VLBI network with 21st-century backend31 Mar, 2020
- JWST Workshop 31 Mar, 2020
- Management Update (COVID-19, Eartquakes, Transmitters)27 Mar, 2020
- NANOGrav Meeting Hosted at UCF27 Mar, 2020
- AO Colloquium: Dr. Michael Denton 27 Mar, 2020
- AO Colloquium: Dr. Alain Herique27 Mar, 2020
- REU Student Mishaal Jan Publishes Summer Research Study about Massive Star Forming Region26 Mar, 2020
- AO helps detect Magnetar in the Cow26 Mar, 2020
- Pulsar Astronomy and Physics at the Arecibo Observatory with Dr. Joanna Rankin26 Mar, 2020
- AO Science at AAS, AOGS26 Mar, 2020
- GBO/AO Single Dish and Observer Training Workshops (May 11-20, 2020)05 Feb, 2020
- Arecibo Observatory update after recent earthquakes09 Jan, 2020
- The Arecibo Observatory Congratulates Dr. Martha P. Haynes, Recipient of 2019 Bruce Gold Medal11 Dec, 2019
Radio-frequency (RF) auroras, like the beautiful example shown in Figure 1 and the movie (link here), are often dancing across the night skies of Puerto Rico. Unlike their high-latitude cousins, however, these tropical phantasms do not generate optical emission and are not associated with solar activity. These are mid-latitude RF echoes observed with coherent radar and displaying radio signatures similar to those detected from the northern lights.
The Arecibo Observatory has been key to understanding the nature of these mid-latitude RF auroras. This unique cluster of diverse and highly sensitive equipment includes both radar and optical instruments. The ionized particles are observed with Arecibo’s incoherent scatter radar (ISR) and show billowy behavior as well as unexplained changes in the density and temperature distributions. At the same time, the neutral particles are observed with Arecibo’s lidars, which also show the billowy behavior and temperature changes. An example of the neutral billows using the sodium resonance lidar is shown in Figure 2. The background ionospheric medium is observed simultaneously with Arecibo’s imagers and ionosondes.
RF auroras appear to result from the interaction between neutral particles in the thermosphere and charged particles in the ionosphere. Neutral winds produce a shear that generates Kelvin-Helmholtz rolls. Current work suggests that RF auroras are produced by neutral particles that drag ions and result in coherent echoes. This finding is motivating a new area of research that focuses on the study of ion behavior to infer neutral winds. Recent work reported convective instabilities and other neutral dynamics during the daytime, opening up new possibilities to expand our understanding of ion-neutral coupling in the lower ionosphere and adding to our understanding of RF auroras.
Figure 1. Mid-latitude RF auroras observed on the night of September 30, 2008, with a coherent scatter radar located on St. Croix and looking perpendicular to the earth's magnetic field line over the Arecibo Observatory at an altitude close to 105 km. The contour corresponds to the island of Puerto Rican and the “X” to the location of the Arecibo Observatory. The color scale indicates variations in Doppler, intensity, and spectral width.
Animation related to Figure 1 Arecibo Observatory: Mid-latitude Radio-Frequency Auroras. By Eliana Nossa, Shikha Raizada, and David Hysell
Figure 2. Altitudinal and temporal distribution of Na atoms obtained using a resonance lidar over Arecibo. The main layer between 80-100 km has been saturated to reveal the structures between 101-110 km. Sarkhel et al. (2012) found atmospheric conditions to be dynamically unstable and conducive a Kelvin-Helmholtz instability during this event.Paper Title: Dynamic instability in the lower thermosphere inferred from irregular sporadic E layers
Paper Authors: D.L. Hysell, E. Nossa, M.F. Larsen, J. Munro, S. Smith, M.P. Sulzer, and S.A. González
Paper Reference: J. Geophys. Res., (2012), 117, A08305, doi:10.1029/2012JA017910.
Keywords: Ionosphere, Auroras, Aeronomy, Nossa, Hysell, Raizada, MLT Region, Mesosphere, Thermosphere, E Region, Radio Propagation, Space, Atmosphere, Earth