Gravity Wave Activity in the Stratosphere and Mesosphere at the South Pole (2024)

    Collins, R. L. / Gardner, C. S. / Committee on Space Research; Scientific Commission C

    • Neue Suche nach: Collins, R. L.
    • Neue Suche nach: Gardner, C. S.
    • Neue Suche nach: Committee on Space Research; Scientific Commission C
    • Neue Suche nach: Collins, R. L.
    • Neue Suche nach: Gardner, C. S.
    • Neue Suche nach: Hernandez, G.
    • Neue Suche nach: Smith, R. W.
    • Neue Suche nach: Committee on Space Research; Scientific Commission C

    In: Southern hemisphere upper atmosphere and ionosphere 5 ; 81-90 ; 1995

    • ISBN:

      0080426255

    • ISSN:

      0273-1177

    • Aufsatz (Konferenz) / Print

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    • Titel:

      Gravity Wave Activity in the Stratosphere and Mesosphere at the South Pole

    • Beteiligte:

      Collins, R. L. ( Autor:in ) / Gardner, C. S. ( Autor:in ) / Hernandez, G. / Smith, R. W. / Committee on Space Research; Scientific Commission C

    • Kongress:

      Meeting C.3; 30th Scientific assembly, Southern hemisphere upper atmosphere and ionosphere ; 1994 ; Hamburg; Germany

    • Erschienen in:

      Southern hemisphere upper atmosphere and ionosphere , 5 ; 81-90

      ADVANCES IN SPACE RESEARCH -OXFORD- ; 16, 5 ; 81-90

    • Verlag:

      Pergamon

      • Neue Suche nach: Pergamon
    • Erscheinungsdatum:

      01.01.1995

    • Format / Umfang:

      10 pages

    • ISBN:

      0080426255

    • ISSN:

      0273-1177

    • Medientyp:

      Aufsatz (Konferenz)

    • Format:

      Print

    • Sprache:

      Englisch

    • Schlagwörter:

      COSPAR , southern hemisphere , upper atmosphere , ionosphere

    • Datenquelle:

      British Library Conference Proceedings

    © Metadata Copyright the British Library Board and other contributors. All rights reserved.

    Inhaltsverzeichnis Konferenzband

    Die Inhaltsverzeichnisse werden automatisch erzeugt und basieren auf den im Index des TIB-Portals verfügbaren Einzelnachweisen der enthaltenen Beiträge. Die Anzeige der Inhaltsverzeichnisse kann daher unvollständig oder lückenhaft sein.

    3

    Thermospheric Dynamics in the Southern Polar Region

    Rees, D. / Hernandez, G. / Smith, R. W. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    17

    Optical Interferometric Observations of 630-nm Intensities, Thermospheric Winds and Temperatures Near the Geomagnetic Equator

    Meriwether, J. W. / Biondi, M. A. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    27

    Observations of Thermospheric Neutral Winds and Temperatures at Cachoeira Paulista (23S, 45W) During a Geomagnetic Storm

    fa*gundes, P. R. / Sahai, Y. / Bittencourt, J. A. / Takahashi, H. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    31

    Upper Thermospheric Temperatures at South Pole

    Smith, R. W. / Hernandez, G. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    41

    Thermospheric Horizontal Winds Above Mawson, Antarctica

    Conde, M. / Dyson, P. L. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    53

    Southern Hemisphere Dynamics Observed by WINDII: The Wind Imaging Interferometer on the UARS Mission

    Shepherd, G. G. / McLandress, C. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    61

    What Can Be Learned from Rotational Temperatures Derived from Ground-Based Airglow Observations about the Aeronomy of the Southern Hemisphere

    Scheer, J. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    71

    Antarctic High-latitude Mesospheric Dynamics

    Hernandez, G. / Smith, R. W. / Fraser, G. J. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    81

    Gravity Wave Activity in the Stratosphere and Mesosphere at the South Pole

    Collins, R. L. / Gardner, C. S. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    91

    Ground Based Radar Investigation of the Antarctic Mesosphere

    Von Biel, H. A. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    99

    Modelling Studies of North-South Differences in the Ionosphere at Mid Latitudes

    Balan, N. / Bailey, G. J. / Titheridge, J. E. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    103

    Radio Studies of the Southern Hemisphere High-latitude Ionosphere

    Dyson, P. L. / Parkinson, M. L. / Quach, A. D. / Smith, P. R. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    113

    Observations of Gravity Waves Associated with Mid-Latitude Spread-F

    Dyson, P. L. / Johnston, D. L. / Scali, J. L. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    117

    Relationship Between Geneation of Equatorial F-Region Plasma Bubbles and Thermospheric Dynamics

    fa*gundes, P. R. / Sahai, Y. / Bittencourt, I. A. / Takahashi, H. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    121

    Geomagnetic Pulsations in the Ionosphere

    Menk, F. W. / Marshall, R. A. / Waters, C. L. / Dunlop, I. S. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    131

    Global Electrodynamics from Superpressure Balloons

    Holzworth, R. H. / Hu, H. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    141

    Upper Atmosphere Research at INPE

    Clemesha, B. R. / Takahashi, H. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    151

    Australian Antarctic Middle and Upper Atmospheric Physics - A New Direction

    Morris, R. J. / Monselesan, D. P. / Klekociuk, A. R. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

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    Gravity Wave Activity in the Stratosphere and Mesosphere at the South Pole (2024)

    FAQs

    What is the gravity wave in the atmosphere? ›

    In a gravity wave, the upward moving region is the most favorable region for cloud development and the sinking region favorable for clear skies. That is why you may see rows of clouds and clear areas between the rows of clouds. A gravity wave is nothing more than a wave moving through a stable layer of the atmosphere.

    What are internal gravity waves in the atmosphere? ›

    Internal gravity waves are waves occurring in the interior of a stratified fluid, with buoyancy providing the restoring force which opposes vertical displacements.

    What causes gravity wave clouds? ›

    They form when air is forced upward by hills or mountains into a layer of stable air in the atmosphere. Gravity causes the air to fall back down, and it begins to oscillate, creating a ripple effect. Wind flowing over the Rocky Mountains, for example, can create gravity waves that are felt as turbulence on an airplane.

    How do gravity waves affect us? ›

    From even the distance of the nearest star, gravitational waves would pass through us almost completely unnoticed. Although these ripples in spacetime carry more energy than any other cataclysmic event, the interactions are so weak that they barely affect us.

    Has there ever been a gravity wave? ›

    In 2015, scientists detected gravitational waves for the very first time. They used a very sensitive instrument called LIGO (Laser Interferometer Gravitational-Wave Observatory). These first gravitational waves happened when two black holes crashed into one another.

    Do humans emit gravitational waves? ›

    Technically speaking, every physical object that accelerates produces gravitational waves. This includes humans, cars, airplanes etc.

    What emits gravitational waves? ›

    The strongest gravitational waves are produced by cataclysmic events such as colliding black holes, supernovae (massive stars exploding at the end of their lifetimes), and colliding neutron stars.

    Can you hear gravitational waves in space? ›

    Astronomers have been able to “hear” the celestial hum of powerful gravitational waves, created by collisions between black holes, echoing across the universe for the first time.

    How fast do gravity waves move? ›

    Gravitational waves travel at the speed of light (186,000 miles per second or 299,000 kilometers per second), squeezing and stretching anything in their path.

    What is the difference between a gravity wave and a ripple? ›

    Gravity waves, or gravitational waves, are essentially ripples in the fabric of space-time caused by accelerating masses. To put it simply, when an object with mass accelerates, the resulting gravitational force travels across space and time, creating waves of gravity that reach out infinitely at the speed of light.

    Did Einstein predict gravitational waves? ›

    About a hundred years ago, Einstein predicted the existence of gravitational waves, but until now, they were undetectable.

    How do you explain gravity waves? ›

    “Gravitational waves are ripples in spacetime. When objects move, the curvature of spacetime changes and these changes move outwards (like ripples on a pond) as gravitational waves. A gravitational wave is a stretch and squash of space and so can be found by measuring the change in length between two objects.”

    What is the gravity in the atmosphere? ›

    What are gravity waves called? ›

    Gravitational waves are sometimes called gravity waves, but gravity waves typically refer to displacement waves in fluids. In 1916 Albert Einstein demonstrated that gravitational waves result from his general theory of relativity as ripples in spacetime.

    What is the difference between a capillary wave and a gravity wave? ›

    The term 'gravity wave' is typically applied to wind-generated, periodic displacements of the sea surface, though nominally tsunamis are also gravity waves. A capillary wave is a wave travelling along the interface between two fluids, whose dynamics are dominated by the effects of surface tension.

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