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

    Wie erhalte ich diesen Titel?

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

    FAQs

    What are gravity waves in the mesosphere? ›

    In the Earth's atmosphere, gravity waves are a mechanism that produce the transfer of momentum from the troposphere to the stratosphere and mesosphere. Gravity waves are generated in the troposphere by frontal systems or by airflow over mountains.

    What happens to the temperature from the stratosphere to the mesosphere? ›

    The ozone layer within the stratosphere also absorbs a lot of solar radiation and reemits it. So, the temperature does increase with altitude through the stratosphere, but begins to decrease again at the top of the stratopause and throughout the mesosphere above it.

    What is the difference between the stratosphere and the mesosphere? ›

    Above the stratosphere is the mesosphere. It extends upward to a height of about 85 km (53 miles) above our planet. Most meteors burn up in the mesosphere. Unlike the stratosphere, temperatures once again grow colder as you rise up through the mesosphere.

    What is the relationship between temperature and altitude in the troposphere, stratosphere, mesosphere, thermosphere, exosphere? ›

    Temperature increases as you gain altitude in the stratosphere and the thermosphere. Temperature decreases as you gain altitude in the troposphere and mesosphere. Air temperature varies in complicated ways with altitude.

    Is there gravity in the stratosphere? ›

    In the middle stratosphere (30–40 km), there is higher gravity wave activity near the equator in autumn in the middle stratosphere than in other seasons in 2020, and much less in 2021. The gravity wave activity is low (maximum 5 J kg1) compared to the lower stratosphere (maximum 10 J kg1).

    What are 3 things that happen in the mesosphere? ›

    Phenomena in mesosphere and near space
    • Airglow.
    • Atmospheric tides.
    • Ionosphere.
    • Meteors.
    • Noctilucent clouds.
    • Polar aurora.
    • Sprite (lightning)
    • Upper atmospheric lightning (Transient luminous event)

    What are 5 facts about the mesosphere? ›

    The mesosphere is directly above the stratosphere and below the thermosphere. It extends from about 50 to 85 km (31 to 53 miles) above our planet. Temperature decreases with height throughout the mesosphere. The coldest temperatures in Earth's atmosphere, about -90° C (-130° F), are found near the top of this layer.

    What will happen if there is no mesosphere? ›

    - Without the mesosphere, meteors would pass through the exosphere and thermosphere without much trouble. In summary, the mesosphere plays a crucial role in protecting life on Earth, regulating temperatures, and allowing meteor showers to light up our skies! ..

    What causes the temperature to increase in the stratosphere but decrease in the mesosphere? ›

    The temperature increases in the stratosphere due to the ozone layer being there that captures radiation. The temperature decreases in the next layer, the mesosphere, because there is no ozone layer there for protection + the amount of air in this layer decreases.

    What lies between the stratosphere and mesosphere? ›

    The stratopause lies between two layers of the atmosphere namely the stratosphere and mesosphere. It lies at an altitude of 50 km. Thus the correct answer is option C.

    Which is colder mesosphere or stratosphere? ›

    The top of the mesosphere is the coldest area of the Earth's atmosphere because temperature may locally decrease to as low as 100 K (-173°C).

    What are 5 facts about the stratosphere? ›

    Stratosphere – Interesting Facts
    • The stratosphere layer is 35 km thick.
    • Cold air is found at the bottom of the stratosphere.
    • Light air is found at the top of the stratosphere.
    • Heavy air is found at the bottom of the stratosphere.
    • Warm air is found at the top of the stratosphere.

    How the temperature changes in both the troposphere and the mesosphere? ›

    Answer and Explanation:

    In the mesosphere, the temperature decreases slowly with the height from 275 K to 195 K. (b) The altitude of the troposphere is about 18 km from the surface of the Earth. In the troposphere, the temperature decreases gradually as the altitude increase. The minimum temperature is about 215 K.

    What happens to temperature in the stratosphere as altitude or height increases? ›

    Temperature in the stratosphere rises with increasing altitude, because the ozone layer absorbs the greater part of the solar ultraviolet radiation.

    Why is the altitude temperature relationship direct in the stratosphere? ›

    One of the main reasons why the stratosphere increases in temperature as you rise is that it contains the ozone layer. The ozone absorbs the Sun's energy and protects the surface of the Earth from harmful radiation. Because the ozone layer is located here, the Sun's energy seems to heat this layer of the atmosphere.

    What are gravity waves in the atmosphere? ›

    A gravity wave is nothing more than a wave moving through a stable layer of the atmosphere. Thunderstorm updrafts will produce gravity waves as they try to punch into the tropopause. The tropopause represents a region of very stable air.

    What do gravity waves tell us? ›

    By tapping into this new source of information about the universe, gravitational wave astronomy might be able to solve some of the biggest puzzles in physics, including: how black holes form, how matter acts in extreme conditions, illuminating the nature of dark matter, and looking at the beginning of the universe long ...

    Where are gravity waves found? ›

    Compact binary inspiral gravitational waves are produced by orbiting pairs of massive and dense ("compact") objects like black holes and neutron stars. There are three subclasses of "compact binary" systems in this category: Binary Neutron Star (BNS) - two neutron stars orbiting each other.

    What is a gravitational wave in astronomy? ›

    Gravitational waves are 'ripples' in space-time caused by some of the most violent and energetic processes in the Universe. Albert Einstein predicted the existence of gravitational waves in 1916 in his general theory of relativity.

    References

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