TY - JOUR
T1 - Overview of nighttime ionospheric instabilities at low- and mid-latitudes
T2 - Coupling aspects resulting in structuring at the mesoscale
AU - Makela, Jonathan J.
AU - Otsuka, Yuichi
N1 - Funding Information:
Acknowledgements JJM was supported by through the National Science Foundation grant ATM-09-40253. A part of the work done by YO was supported by Grant-in-Aid for Young Scientists A (20684021) of the Ministry of Education, Culture, Sports, Science and Technology of Japan. The authors thank the organizers of the International Space Science Institute workshop on “Coupling between Earth’s atmosphere and its plasma environment.”
PY - 2012/6
Y1 - 2012/6
N2 - We present a review of the current state of understanding regarding two classes of irregularities causing mesoscale structuring (hundreds of kilometers) in the nighttime ionosphere at low- and mid-latitudes. Additionally, current state of understanding of equatorial plasma bubbles at low latitudes, and medium-scale traveling ionospheric disturbances at mid latitudes and their relationship to possible seeding from lower altitudes are described. In each case, well-developed linear theories exist to explain the general properties of the irregularities. However, these linear theories have growth rates too low to explain the actual observations, giving rise to the need to invoke seeding mechanisms. We describe the observational databases that have been compiled over the decades and discuss possible coupling and seeding mechanisms that would overcome the low growth rate and explain the observed structuring at the mesoscale. Future research directions are also briefly discussed.
AB - We present a review of the current state of understanding regarding two classes of irregularities causing mesoscale structuring (hundreds of kilometers) in the nighttime ionosphere at low- and mid-latitudes. Additionally, current state of understanding of equatorial plasma bubbles at low latitudes, and medium-scale traveling ionospheric disturbances at mid latitudes and their relationship to possible seeding from lower altitudes are described. In each case, well-developed linear theories exist to explain the general properties of the irregularities. However, these linear theories have growth rates too low to explain the actual observations, giving rise to the need to invoke seeding mechanisms. We describe the observational databases that have been compiled over the decades and discuss possible coupling and seeding mechanisms that would overcome the low growth rate and explain the observed structuring at the mesoscale. Future research directions are also briefly discussed.
KW - Ionospheric irregularities
KW - Low-latitude ionosphere
KW - Mid-latitude ionosphere
KW - Perkins instability
KW - Rayleigh-Taylor instability
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U2 - 10.1007/s11214-011-9816-6
DO - 10.1007/s11214-011-9816-6
M3 - Article
AN - SCOPUS:84863565378
SN - 0038-6308
VL - 168
SP - 419
EP - 440
JO - Space Science Reviews
JF - Space Science Reviews
IS - 1-4
ER -