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Record W2346531044 · doi:10.11728/cjss2002.02.136

神舟2号大气密度探测器的探测结果(I)日照和阴影区域热层大气密度变化

2002· article· zh· W2346531044 on OpenAlexvenueno aff
秦国泰, 邱时彦

Bibliographic record

VenueCanadian Journal of Soil Science · 2002
Typearticle
Languagezh
FieldEngineering
TopicInertial Sensor and Navigation
Canadian institutionsnot available
Fundersnot available
KeywordsThermosphereEnvironmental scienceAtmospheric temperatureOrbiterEarth's magnetic fieldAtmospheric sciencesCircular orbitAltitude (triangle)Density of airAtmospheric soundingPhysicsOrbit (dynamics)MeteorologyIonosphereAstronomyGeometryMathematics

Abstract

fetched live from OpenAlex

Solar radiation is the main source for heating of thermosphere. The change of its intensity can result in the change of Earth's upper atmospheric density. With the same reasons, the difference between the sunshine and shaded area is one of the main reasons for the difference of upper atmospheric density at the same altitude. For Low Earth Orbit (LEO) orbiter, when running around Earth, it will pass the sunshine area and shaded area each orbit even the orbit is circular or quasi-circular.The consequent change of atmospheric density directly influence orbiter's motions and the precision of prognostication of orbit. On the other hand, change of atmospheric density resulted from sunshining and shaded area has something to do with different factors of solar-terrestrial prsacs, some discussions are needed, takeing into about these related phenomena.Although data of American earlier balloon detection had already been applied to the discussion of diurnal-change of upper atmospheric density, due to limitation of the conditions at that time, detailed description of the change could not obtained. And the later AE, DE satellite etc. all run at elliptical orbits, could not provide data for the discussion of the phenomena above mentioned. In this article, we applied the data from SZ-2 Atmospheric Density Detector, which are the direct measurement results at quasi-circular orbit and very helpful for the discussion of atmospheric density change in sunshine and shaded area. We separate the results and primary analysis into 2 parts: Characteristics of Change and Response to Solar and Geomagnetic Activity, and will describe them seperately. This paper is mainly concentrated on the first part. SZ-2 Atmospheric Density Detector started orbitting around the earth on January 18, 2001. The orbital inclination was 410, and the flew altitude was,410 km. During the period of half a year, a lot of data of the upper atmospheric density have been obtained. In this paper, data of thermosphere density from Febru- ary to April, 2001 collected by SZ-2 Atmospheric Density Detector are used to study the change of the thermosphere density in the sunshining and shaded area.The results show that the ratio of the changes can be up to 2-3 in the vicinity of 410 km, and the magnitude of this change decreases as the geomagnetic activ-ities increases. The peak value of the density in sunshining area increases as the solar activities increases and locates at the Local Time 14-15 h. The density in shaded area bear a relation to the geomagnetic activates, and increases as Ap value increases. The minimum value of the density in shaded area locates at the Local Time 4-5 h. The latitude range of士100 in the shaded area often show a density peak.

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: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.464
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.001
Scholarly communication0.0000.001
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.015
GPT teacher head0.198
Teacher spread0.183 · 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 designSimulation or modeling
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

Citations0
Published2002
Admission routes1
Has abstractyes

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