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Record W1989268159 · doi:10.1029/2001jd001232

Climatological features of mesosphere and lower thermosphere stationary planetary waves within ±40° latitude

2002· article· en· W1989268159 on OpenAlexaff
J. M. Forbes, X. Zhang, W. E. Ward, E. R. Talaat

Bibliographic record

VenueJournal of Geophysical Research Atmospheres · 2002
Typearticle
Languageen
FieldPhysics and Astronomy
TopicIonosphere and magnetosphere dynamics
Canadian institutionsUniversity of New Brunswick
FundersNational Science Foundation
KeywordsThermosphereMesosphereNorthern HemisphereStratosphereAtmospheric sciencesMiddle latitudesGeologyZonal and meridionalSouthern HemisphereAmplitudeAtmosphere (unit)Gravity waveLatitudePolar nightClimatologyPhysicsGeodesyIonosphereGeophysicsMeteorologyAstrophysicsGravitational wave

Abstract

fetched live from OpenAlex

Zonal and meridional wind measurements from the High Resolution Doppler Imager (HRDI) and Wind Imaging Interferometer (WINDII) instruments on the Upper Atmosphere Research Satellite (UARS) are used to construct monthly average stationary planetary wave (SPW) structures from 15 km to 110 km over the period December 1991 to September 1994. Because of viewing constraints of the instruments, intercomparisons between Northern Hemisphere (NH) and Southern Hemisphere (SH) structures and seasonal evolutions are mainly confined to ±40° latitude. The largest zonal wave number s = 1 amplitudes (10–25 m s −1 ) in the stratosphere and mesosphere at ±40° exist in the zonal wind fields and occur during September–January in the NH and July–October in the SH. SPW s = 2 structures are much less prevalent, especially above 80 km because of more restrictive filtering effects due to the mean winds. Above about 70 km, s = 1 wave amplitudes (∼5–10 m s −1 ) are more uniform, extending over all nonsummer months in both hemispheres up to 80–90 km, with similar amplitudes existing throughout the year at higher altitudes. Our interpretation is that the SPW above about 80–90 km during summer owe their existence to ducting from the winter hemisphere, in agreement with numerical simulations by Pogoreltsev and Sukhanova [1993] . The origin of SPW above about 80 km during winter at midlatitudes is not possible to determine unambiguously. Phase structures undergo a transition from vertical propagation with long vertical wavelengths (hundreds of kilometers) below ∼80 km to either evanescent behavior or an extreme shortening of vertical scale at higher altitudes. This change in phase behavior may be connected with negative values in refractive index Q for quasi‐geostrophic wave propagation, which occur over a narrow height region near 80 km during almost every month. This interruption of normal phase progression makes it impossible to distinguish the origin of the planetary wave oscillations from (1) those that “tunnel” through the Q < 0 region and (2) those that might be excited in situ by zonally asymmetric momentum deposition from gravity waves which have undergone filtering by the stratospheric planetary wave wind field. In addition, quantitative estimates of aliasing due to the diurnal tide indicate that it may be of sufficient magnitude to contaminate retrieved SPW structures between 80–90 km and 100–110 km, where local time coverages are incomplete. Comparisons are made between the observed SPW structure and those from the horizontal wind model [ Hedin et al. , 1993 , 1996 ]. This model is found to provide a reasonable approximation to NH winter SPW s = 1 structures below 80 km, but severely underestimates the amplitudes of SPW in the SH.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.430
Threshold uncertainty score0.996

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.000
Science and technology studies0.0000.001
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0050.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.020
GPT teacher head0.282
Teacher spread0.262 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations44
Published2002
Admission routes1
Has abstractyes

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