Theoretical study of the low- and midlatitude ionospheric electron density enhancement during the October 2003 superstorm: Relative importance of the neutral wind and the electric field

By Chien-Hung Lin, Arthur D. Richmond, R. Heelis, G. Bailey, G. Lu, Jann‐Yenq Liu, H. Yeh, Shin-Yi Su. 2005

202 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/7d2cdc76145de65c9e50dbcceff2650549e3e0b9

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Aerospace Engineering

1. K. Shiokawa
2. Yuichi Otsuka
3. Huijun Le
4. N. Balan
5. Libo Liu
6. C. Liu
7. R. Akmaev
8. Takuya Tsugawa

In Astronomy and Astrophysics

1. T. Immel
2. C. Liu
3. Jann‐Yenq Liu
4. C. Hsiao
5. Larry J. Paxton
6. Chien-Hung Lin
7. Yuichi Otsuka
8. M. E. Hagan

In Geophysics

1. K. Shiokawa
2. Yuichi Otsuka
3. M. E. Hagan
4. N. Balan
5. Jann‐Yenq Liu
6. T. Immel
7. Libo Liu
8. C. Liu

Citations in the corpus

• Plausible effect of atmospheric tides on the equatorial ionosphere observed by the FORMOSAT‐3/COSMIC: Three‐dimensional electron density structures (2007, background): “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].”
• Low‐latitude ionosphere response to super geomagnetic storm of 17/18 March 2015: Results from a chain of ground‐based observations over Indian sector (2015, background): “However, positive ionospheric storms are produced by additional production of density at lower altitudes due to photoionization as existing density goes to higher altitudes due to higher upward drifts [Lin et al., 2005; Sastri et al., 2000].”
• Longitudinal structure of the equatorial ionosphere: Time evolution of the four-peaked EIA structure (2007, background): “These two effects are considered theoretically by Lin et al. [2005] , and they concluded that a stronger plasma fountain effect is indeed the major driver for producing a stronger and poleward extended EIA.”
• Unusual early morning development of the equatorial anomaly in the Brazilian sector during the Halloween magnetic storm (2006, unknown): “According to their model, the meridional wind can show a very disturbed pattern at low latitudes during the first hours following the magnetic storm onset, in such a way that rapid reversals from northward to southward can occur in time intervals shorter that two hours, and strong transequatorial wi”
• A brief review of equatorial ionization anomaly and ionospheric irregularities (2018, methodology): “The strong EIA was explained in terms of the combined effects of strong eastward PPEF and fast storm-time equatorward winds (e.g., Lin et al., 2005; Balan et al., 2010, 2011; Lu et al., 2012).”
• Super plasma fountain and equatorial ionization anomaly during penetration electric field (2009, background): “Lin et al. [2005] and Lei et al. [2008] showed that in addition to penetration electric field, neutral wind is important in producing positive storms in Nmax and TEC.”
• A physical mechanism of positive ionospheric storms at low latitudes and midlatitudes (2010, background): “Werner et al. [1999], Lin et al. [2005] , and Lei et al.[2008] showed that, in addition to PPEF, equatorward wind is important in producing positive storms in Nmax and TEC.”
• 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].”