Outstanding problems in the equatorial ionosphere–thermosphere electrodynamics relevant to spread F

By M. Abdu. 2001

344 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/aa1197003d48e7e93a0f26f064b0b92250484446

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In Astronomy and Astrophysics

1. T. Immel
2. C. Hsiao
3. Jann‐Yenq Liu
4. M. E. Hagan
5. C. Liu
6. H. Frey
7. Larry J. Paxton
8. S. Mende

In Molecular Biology

1. C. Hsiao
2. Jann‐Yenq Liu
3. C. Liu
4. M. E. Hagan
5. Akinori Saito
6. Takuya Tsugawa
7. T. Immel
8. S. Mende

Citations in the corpus

• Gravity wave initiation of equatorial spread F/plasma bubble irregularities based on observational data from the SpreadFEx campaign (2009, result): “Observational evidence of a possible association between gravity waves and ESF has been suggested in statistical data comparisons by several authors (see for example Rottger, 1981; McClure et al., 1998; Abdu, 2001).”
• Longitudinal structure of the equatorial ionosphere: Time evolution of the four-peaked EIA structure (2007, background): “The two basic processes that affect the EIA formation significantly are the strength of the equatorial plasma fountain and thermospheric neutral winds [Balan and Bailey, 1995; Balan et al., 1997; Rishbeth, 2000; Abdu, 2001; Lin et al., 2005].”
• Plausible effect of atmospheric tides on the equatorial ionosphere observed by the FORMOSAT‐3/COSMIC: Three‐dimensional electron density structures (2007, background): “The two basic processes that affect the EIA formation significantly are the equatorial zonal electric field and thermospheric neutral winds [Balan and Bailey, 1995; Balan et al., 1997; Rishbeth, 2000; Abdu, 2001; Lin et al., 2005].”
• Occurrence characteristics of plasma bubble derived from global ground‐based GPS receiver networks (2007, background): “[2] There have been many studies on the occurrence characteristics of plasma bubbles using observational data such as ionosondes [e.g., Rastogi, 1980; Abdu, 2001 ], topside sounders [e.g., Maruyama and Matsuura, 1984], radio scintillations [e.g., Basu and Basu, 1985; Paulson, 1981; Aarons, 1993] an”
• Longitudinal structure of the equatorial anomaly in the nighttime ionosphere observed by IMAGE/FUV (2005, background): “However, these parameters can show a very complex behavior [Rishbeth, 2000; Abdu, 2001 ] and also are difficult to measure in comparison with the EA itself.”
• Motions of the equatorial ionization anomaly crests imaged by FORMOSAT‐3/COSMIC (2007, background): “[9] The two basic processes that affect the EIA formation significantly are the strength of the equatorial plasma fountain and thermospheric neutral winds [Balan and Bailey, 1995; Balan et al., 1997; Su et al., 1997; Rishbeth, 2000; Abdu, 2001; Lin et al., 2005].”