On seeding equatorial spread F during solstices
Interpretation of the morphology of equatorial spread F (ESF) is usually given in terms of factors that modulate the growth rate of the Rayleigh‐Taylor instability. That interpretation is, however, incomplete because only one means for growth‐rate enhancement has been included; that is, the strength...
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| Published in: | Geophysical research letters Vol. 37; no. 5 |
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| Format: | Journal Article |
| Language: | English |
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Blackwell Publishing Ltd
01-03-2010
American Geophysical Union John Wiley & Sons, Inc |
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| Abstract | Interpretation of the morphology of equatorial spread F (ESF) is usually given in terms of factors that modulate the growth rate of the Rayleigh‐Taylor instability. That interpretation is, however, incomplete because only one means for growth‐rate enhancement has been included; that is, the strength of the post‐sunset rise of the F layer could become enhanced, when the solar terminator aligns with geomagnetic field lines. Maxima in ESF occurrence observed near equinoxes seem accountable by this means, but maxima observed near solstices require another source of enhancement. Seasonal migration and latitudinal alignment of the inter‐tropical convergence zone (ITCZ) with the magnetic dip equator is suggested as the missing source, and shown able to fill that void. |
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| AbstractList | Interpretation of the morphology of equatorial spread F (ESF) is usually given in terms of factors that modulate the growth rate of the Rayleigh‐Taylor instability. That interpretation is, however, incomplete because only one means for growth‐rate enhancement has been included; that is, the strength of the post‐sunset rise of the F layer could become enhanced, when the solar terminator aligns with geomagnetic field lines. Maxima in ESF occurrence observed near equinoxes seem accountable by this means, but maxima observed near solstices require another source of enhancement. Seasonal migration and latitudinal alignment of the inter‐tropical convergence zone (ITCZ) with the magnetic dip equator is suggested as the missing source, and shown able to fill that void. Interpretation of the morphology of equatorial spread F (ESF) is usually given in terms of factors that modulate the growth rate of the Rayleigh‐Taylor instability. That interpretation is, however, incomplete because only one means for growth‐rate enhancement has been included; that is, the strength of the post‐sunset rise of the F layer could become enhanced, when the solar terminator aligns with geomagnetic field lines. Maxima in ESF occurrence observed near equinoxes seem accountable by this means, but maxima observed near solstices require another source of enhancement. Seasonal migration and latitudinal alignment of the inter‐tropical convergence zone (ITCZ) with the magnetic dip equator is suggested as the missing source, and shown able to fill that void. |
| Author | Tsunoda, Roland T. |
| Author_xml | – sequence: 1 givenname: Roland T. surname: Tsunoda fullname: Tsunoda, Roland T. email: tsunoda@sri.com organization: Center for Geospace Studies, SRI International, California, Menlo Park, USA |
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| Cites_doi | 10.1175/1520‐0469(1966)023<0812:ESFATT>2.0.CO;2 10.1029/JA085iA02p00722 10.1175/1520‐0442(1993)006<2162:ASDCOT>2.0.CO;2 10.1029/JA090iA01p00447 10.1029/2008GL035706 10.1016/0021‐9169(77)90007‐1 10.1029/2008GL036221 10.1029/2006GL027465 10.1029/93JA00762 10.1029/95JA02211 10.1029/JA076i016p03777 10.1029/98JA02749 10.1029/2006JA011845 10.1029/2009GL039887 10.1029/92GL01935 10.1029/JA089iA12p10903 10.1016/0021‐9169(85)90052‐2 10.1016/j.asr.2009.08.019 10.1016/0021‐9169(81)90108‐2 10.1029/2005GL022512 |
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| Keywords | Field line growth rates morphology strength dip geomagnetic field Seeding Sunset Alignment interpretation Solar terminator Rayleigh Taylor instability migration Spread F Intertropical convergence zone |
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| Snippet | Interpretation of the morphology of equatorial spread F (ESF) is usually given in terms of factors that modulate the growth rate of the Rayleigh‐Taylor... Interpretation of the morphology of equatorial spread F (ESF) is usually given in terms of factors that modulate the growth rate of the Rayleigh‐Taylor... Interpretation of the morphology of equatorial spread F (ESF) is usually given in terms of factors that modulate the growth rate of the Rayleigh-Taylor... |
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| SubjectTerms | Alignment Atmospheric sciences Convergence Dipping Earth sciences Earth, ocean, space Equator equatorial spread F Exact sciences and technology Geomagnetic field Maxima Migration Nucleation Solstices Spread F |
| Title | On seeding equatorial spread F during solstices |
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