Tidal Signatures in the upper Atmosphere from the Equator to the Pole Chao Xiong 1, Hermann Lühr 1, Claudia Stolle 1, and Jorge Chau 2 1. Helmholtz Centre.

Slides:

Advertisements

Similar presentations

Chapter 10 Wind: Global Systems.

Advertisements

Space Weather dependence of the air drag as observed by CHAMP Hermann Lühr 1) and Huixin Liu 2) 1) GeoForschungsZentrum Potsdam, Germany 2) Dept. Earth.

The Unusual Northern Polar Summer of 2002 by Richard A. Goldberg (NASA GSFC) Artem G. Feofilov (CUA/GSFC) Alexander A. Kutepov (CUA/GSFC) W. Dean Pesnell.

Seismology Forum Meeting 2014：

Ionosphere Climate Studied by F3 / COSMIC Constellation C. H. Liu Academia Sinica In Collaboration with Tulasi Ram, C.H. Lin and S.Y. Su.

The primary mechanism through which energy and momentum are transferred from the lower atmosphere to the upper atmosphere and ionosphere is through the.

1 FIREBIRD Science Overview Marcello Ruffolo Nathan Hyatt Jordan Maxwell 2 August 2013FIREBIRD Science.

No. 1 Characteristics of field-aligned currents derived from the Swarm constellation Hermann Lühr, Jaeheung Park, Jan Rauberg, Ingo Michaelis, Guram Kervalishvili.

2011 SuperDARN Workshop, Hanover, NH 1 Solar cycle variability of atmospheric waves and tides as observed by SuperDARN Elsayed R. Talaat Johns Hopkins.

Spatio-temporal structures of equatorial F-region plasma irregularities & Geomagnetic Regular Daily Variations (Sq, Solar quiet) as seen in space and at.

Space Weather Workshop, Boulder, CO, April 2013 No. 1 Ionospheric plasma irregularities at high latitudes as observed by CHAMP Hermann Lühr and.

Abstract Since the ionosphere is the interface between the Earth and space environments and impacts radio, television and satellite communication, it is.

Oceans, Currents, and Weather Dynamics

Atmospheric Circulation

Summary: The coupling between the ionized layers of the upper atmosphere and the thermospheric neutral gas takes place via ion drag force and is mediated.

Abstract The non-dipolar portions of Earth's main magnetic field constitute substantial differences between the geomagnetic field configurations of both.

Julie A. Feldt CEDAR-GEM workshop June 26 th, 2011.

How do gravity waves determine the global distributions of winds, temperature, density and turbulence within a planetary atmosphere? What is the fundamental.

Meteorology Notes Part II

Antarctic Peninsula is a very suitable area for experimental investigations of troposphere-to-ionosphere energy transfer because this place characterized.

Chapter 17 Notes: The Atmosphere. What is the Atmosphere? The atmosphere can be defined as the portion of planet earth that contains gas. Weather can.

T SPP1788 “DynamicEarth“ Workshop, GFZ Potsdam, 3 July 2014 No. 1 Calibration/Validation of Swarm Data Products: German activities Hermann Lühr and Cal/Val.

Nighttime 4-peak Longitudinal Structure of Ionospheric Plasma Density at Mid-Low latitudes During High and Extreme.

Accomplishments of the Past Decade & Science Imperatives for Atmosphere-Ionosphere- Magnetosphere Interactions (AIMI) Research 1 What do they mean by “

How does the Sun drive the dynamics of Earth’s thermosphere and ionosphere Wenbin Wang, Alan Burns, Liying Qian and Stan Solomon High Altitude Observatory.

University of Colorado 1 ; Delft University of Technology 2 ; University of Alaska 3 ; Centre National d’Etudes Spatiales 4 ; National Center for Atmospheric.

Jeff Forbes (CU), Xiaoli Zhang (CU), Sean Bruinsma (CNES), Jens Oberheide (Clemson U), Jason Leonard (CU) 1 Coupling to the Lower Atmosphere, an Observation-Based.

Ionospheric Electrodynamics & Low-Earth Orbiting Satellites (LEOS) J-M Noël, A. Russell, D. Burrell & S. Thorsteinson Royal Military College of Canada.

Joint International GRACE Science Team Meeting and DFG SPP 1257 Symposium, Oct. 2007, GFZ Potsdam Folie 1 Retrieval of electron density profiles.

Coupling Between the Lower Atmosphere and Thermosphere as Revealed in GOCE and Swarm Accelerometer Measurements Jeffrey M. Forbes, Xiaoli Zhang and Jesse.

Neutral Winds in the Upper Atmosphere Qian Wu National Center for Atmospheric Research.

Scott M. Bailey, LWS Workshop March 24, 2004 The Observed Response of the Lower Thermosphere to Solar Energetic Inputs Scott M. Bailey, Erica M. Rodgers,

GP33A-06 / Fall AGU Meeting, San Francisco, December 2004 Magnetic signals generated by the ocean circulation and their variability. Manoj,

MESOSPHERE COUPLING THE ROLE OF WAVES AND TIDES. Spectra show that waves & tides of large amplitude dominate the MLT region A typical power spectrum of.

Use of GPS Radio Occultation Data for Climate Monitoring Y.-H. Kuo, C. Rocken, and R. A. Anthes University Corporation for Atmospheric Research.

Acoustic-gravity wave monitoring for global atmospheric studies Elisabeth Blanc 1 Alexis Le Pichon 1 Lars Ceranna 2 Thomas Farges 1 2- BGR / B3.11, Hannover,

1 Atmospheric Tides: Linking Deep Tropical Convection to Ionosphere-Thermosphere Variability Briefly discuss migrating vs. non-migrating tides. Demonstrate.

Rotation: Its effects 1.Day & Night. 2.Bulging of the Earth at the Equator and flattening at the poles. 3.The deflection of winds & ocean currents. 4.Tides.

NCAR Advanced Study Program (ASP) Seminar, February 13, Solar Semidiurnal Tide in the Atmosphere Jeff Forbes Department of Aerospace Engineering.

Composition/Characterstics of the Atmosphere 80% Nitrogen, 20% Oxygen- treated as a perfect gas Lower atmosphere extends up to  50 km. Lower atmosphere.

Heating of the Earth. Temperature Layers of the Atmosphere.

Image credit: NASA Response of the Earth’s environment to solar radiative forcing Ingrid Cnossen British Antarctic Survey.

Atmosphere. What makes up our atmosphere?  Nitrogen  Oxygen  Argon.

New Science Opportunities with a Mid-Latitude SuperDARN Radar Raymond A. Greenwald Johns Hopkins University Applied Physics Laboratory.

Study on the Impact of Combined Magnetic and Electric Field Analysis and of Ocean Circulation Effects on Swarm Mission Performance by S. Vennerstrom, E.

Earth in Space EARTH, THE SUN, AND THE SEASONS. Earth, the Sun, and the Seasons  Why is Earth colder in winter than in the summer?  Not because Earth.

The dynamics of planetary atmospheres

COSMIC Ionospheric measurements Jiuhou Lei NCAR ASP/HAO Research review, Boulder, March 8, 2007.

Space-based studies of low-latitude ionospheric forcing originating in the lower atmosphere Thomas J. Immel, Scott L. England Space Sciences Laboratory,

Effects of January 2010 stratospheric sudden warming in the low-latitude ionosphere L. Goncharenko, A. Coster, W. Rideout, MIT Haystack Observatory, USA.

Impacts of climate change in the troposphere, stratosphere, and mesosphere on the thermosphere and ionosphere Ingrid Cnossen GFZ German Research Centre.

Planetary waves in the equatorial mesosphere and ionosphere measurements Lourivaldo Mota Lima (UEPB) Luciana R. Araújo, Maxwelton F. Silva (UEPB) H. Takahashi,

The Atmosphere: Structure & Temperature. Atmosphere Characteristics Weather is constantly changing, and it refers to the state of the atmosphere at any.

Impact of midnight thermosphere dynamics on the equatorial ionospheric vertical drifts Tzu-Wei Fang 1,2 R. Akmaev 2, R. Stoneback 3, T. Fuller-Rowell 1,2,

Jaeheung Park1, Hermann Lühr1, Claudia Stolle1,

Using the Mars climate Database for aerobraking ( km)

The 3rd Swarm Science Meeting, June 2014, Copenhagen, Denmark

CEDAR Frontiers: Daytime Optical Aeronomy Duggirala Pallamraju and Supriya Chakrabarti Center for Space Physics, Boston University &

The Ionosphere and Thermosphere GEM 2013 Student Tutorial

Atmosphere-Ionosphere Wave Coupling as Revealed in Swarm Plasma Densities and Drifts Jeffrey M. Forbes Department of Aerospace Engineering Sciences, University.

High-latitude Neutral Density Maxima

The Source of Planetary Period Oscillations in Saturn’s magnetosphere

First validation of Level 2 CAT-2 products: FAC/IBI/TEC

Thermosphere-Ionosphere Issues for DASI - I:

The ionosphere is much more structured and variable than ever predicted. Solar Driven Model Since 2000, we have seen more, very clear evidence that the.

Ionosphere, Magnetosphere and Thermosphere Anthea Coster

SPP Colloquium, 16-Jun-2017, Bremen

Oerstedt+Champ+Swarm → Empirical models →New parameters/knowledge

Charles Lin1, Jia-Ting Lin1, Loren Chang2, Yang-Yi Sun2

Evaluation of IRI-2012 by comparison with JASON-1 TEC and incoherent scatter radar observations during the solar minimum period Eun-Young Ji,

Presentation transcript:

Tidal Signatures in the upper Atmosphere from the Equator to the Pole Chao Xiong 1, Hermann Lühr 1, Claudia Stolle 1, and Jorge Chau 2 1. Helmholtz Centre Potsdam, GFZ German Research Centre for Geosciences, Telegrafenberg, Potsdam, Germany. 2. Leibniz Institute of Atmospheric Physics, Kühlungsborn, Germany. DFG-SPP “1788 DynamicEarth” GFZ Potsdam, July, 2014

WN4 and WN3 as well as Midlatitude Summer Night Anomaly (MSNA) Equatorial region ? Northern hemi Southern hemi Weddell Sea Anomaly (WSA), first observed by an ionosode in the 1950s (Bellchambers and Piggott, 1958; Penndorf, 1965). Midlatitude Summer Night Anomaly (MSNA) observed by satellites observations (Lin et al., 2009; Thampi et al., 2010; Liu et al., 209). (Liu et al., 2010) (Lühr and Manoj., 2013) Equatorial Electrojet Electron density

Wave-1 and Wave-2 patterns of MSNA in the two hemispheres (Xiong and Lühr., 2014) Electron density Thermospheric mass density CHAMP -40°~-60° MLAT GRACE 40°~60° MLAT

Swarm Observations during solstice seasons Swarm-ASwarm-BSwarm-C Swarm-ASwarm-BSwarm-C Dec. S Southern hemisphere June. S Northern hemisphere

The opportunity Swarm provides us Pole Equator Ionosphere-Thermosphere (IT) Lower Atmosphere Mesopause 0 km 500 km Tides Atmosphere-Ionosphere Coupling by Tides & Planetary Waves plasma flow tidal penetra tion B E tidal dynam o tidal dissipation O3H2OO3H2O Tides Atmosphere-Space Interaction Region PWs E equator ial anomal y compositio n changes wind transpo rt The primary mechanism through which energy and momentum are transferred from the lower atmosphere to the upper atmosphere and ionosphere is through the generation and propagation of waves (Forbes et al., 2014). The Swarm constellation provides us good opportunity for better understanding the Atmosphere- Ionosphere (AI) coupling mechanisms at different latitude regions: 1. Analyzing the tidal signatures of ionospheric and thermosperic quantities. 2. Compare the tidal signatures at different altitudes. 3. Compare the Swarm in situ observations with groundbased measuremtns, to separate the different sources of the tides.