Monday 1 February 2021

Block 1

AM

Block 2

PM

D1.2
Large-Scale Heliospheric Structure: Theory, Modelling, and Data
D1.2
Large-Scale Heliospheric Structure: Theory, Modelling, and Data
D2.3
Thermal and Dynamic Plasma Instabilities on Multiscales: From Laboratories to Planets, the Sun/Stars, Galaxies, and Beyond
D2.3
Thermal and Dynamic Plasma Instabilities on Multiscales: From Laboratories to Planets, the Sun/Stars, Galaxies, and Beyond
D3.1
Highlights of Magnetospheric Plasma Physics
D0.1
Overview Talks
D0.1
Overview Talks
PPP.3
Planetary Protection Research and Development
PPP.3
Planetary Protection Research and Development
PPP.3
Planetary Protection Research and Development
PPP.2
Planetary Protection Mission Implementation and Status
PPP.2
Planetary Protection Mission Implementation and Status
D3.5
Particle Acceleration and Loss in the Earth and Planetary Magnetospheres
D3.5
Particle Acceleration and Loss in the Earth and Planetary Magnetospheres
D2.4
Sun-Heliosphere Connection Events: Origin, Propagation, Impact and Prediction
D2.4
Sun-Heliosphere Connection Events: Origin, Propagation, Impact and Prediction
B0.2
Human and Robotic Exploration of Moon, Mars, and Asteroids
B0.2
Human and Robotic Exploration of Moon, Mars, and Asteroids
B0.2
Human and Robotic Exploration of Moon, Mars, and Asteroids
B0.2
Human and Robotic Exploration of Moon, Mars, and Asteroids
B0.6
Planetary Instruments
B0.6
Planetary Instruments
B0.6
Planetary Instruments
B1.1
Small Body Exploration Science in the New Decade
B1.2
Asteroids, Friends Or Foe: Planetary Defense and Resources
B1.2
Asteroids, Friends Or Foe: Planetary Defense and Resources
B1.2
Asteroids, Friends Or Foe: Planetary Defense and Resources
B4.3
Mars Sample Return
B4.3
Mars Sample Return
B4.4
Venus Science and Exploration
B4.4
Venus Science and Exploration
B5.3
Ocean Worlds
B5.4
Ice Giant Systems
PE.2
Current Trends, Initiatives and Research in Education and Outreach for Space Sciences
B3.1
Lunar Science and Exploration
B3.1
Lunar Science and Exploration
E1.10
Accretion and Ejection in Galactic Compact Objects
E1.10
Accretion and Ejection in Galactic Compact Objects
E1.10
Accretion and Ejection in Galactic Compact Objects
E1.10
Accretion and Ejection in Galactic Compact Objects
E1.4
Black Hole Astrophysics: Observational Evidence and Theoretical Models
E1.4
Black Hole Astrophysics: Observational Evidence and Theoretical Models
E1.4
Black Hole Astrophysics: Observational Evidence and Theoretical Models
E1.8
Evolution of Disk and Corona in X-ray Binaries: Intersection of Observations and Modeling
E1.16
Origin of Cosmic Rays
E1.16
Origin of Cosmic Rays
E1.16
Origin of Cosmic Rays
E1.16
Origin of Cosmic Rays
E1.20
Science with Cubesats, Small Satellites, and Constellations
E1.20
Science with Cubesats, Small Satellites, and Constellations
E1.20
Science with Cubesats, Small Satellites, and Constellations
E1.20
Science with Cubesats, Small Satellites, and Constellations
E1.2
The Remnants of Supernova Explosions
E1.2
The Remnants of Supernova Explosions
E1.2
The Remnants of Supernova Explosions
E1.2
The Remnants of Supernova Explosions
E1.18
Probing Energy Extraction from Supermassive Black Holes
E1.18
Probing Energy Extraction from Supermassive Black Holes
E1.18
Probing Energy Extraction from Supermassive Black Holes
E1.18
Probing Energy Extraction from Supermassive Black Holes
E2.1
Magnetic Flux Ropes in Solar and Stellar Environments
E2.1
Magnetic Flux Ropes in Solar and Stellar Environments
E2.1
Magnetic Flux Ropes in Solar and Stellar Environments
E2.1
Magnetic Flux Ropes in Solar and Stellar Environments
C5.2
Dust Detection and Observation in Space and Laboratory Experiments
C5.2
Dust Detection and Observation in Space and Laboratory Experiments
C0.3
Variabilities of Radio Wave Propagation Characteristics in Lower Ionosphere
C0.3
Variabilities of Radio Wave Propagation Characteristics in Lower Ionosphere
C2.1
The Physics and Dynamics of the Middle Atmosphere from Mid to High Latitudes
C2.1
The Physics and Dynamics of the Middle Atmosphere from Mid to High Latitudes
C3.1
Planetary Atmospheres
C3.1
Planetary Atmospheres
C1.1
Recent Advances in Equatorial, Low- and Mid-Latitude Mesosphere, Thermosphere and Ionosphere Studies
C1.1
Recent Advances in Equatorial, Low- and Mid-Latitude Mesosphere, Thermosphere and Ionosphere Studies
C1.1
Recent Advances in Equatorial, Low- and Mid-Latitude Mesosphere, Thermosphere and Ionosphere Studies
C1.1
Recent Advances in Equatorial, Low- and Mid-Latitude Mesosphere, Thermosphere and Ionosphere Studies
PSW.5
International Space Weather Action Team - a Global Network of Research Teams Targeting Improvements of Resilience to Space Weather
PSW.5
International Space Weather Action Team - a Global Network of Research Teams Targeting Improvements of Resilience to Space Weather
PSW.5
International Space Weather Action Team - a Global Network of Research Teams Targeting Improvements of Resilience to Space Weather
PSW.5
International Space Weather Action Team - a Global Network of Research Teams Targeting Improvements of Resilience to Space Weather
A0.5
CubeSats for Scientific and Civil-use Studies of the Earth
A0.5
CubeSats for Scientific and Civil-use Studies of the Earth
A0.5
CubeSats for Scientific and Civil-use Studies of the Earth
A0.5
CubeSats for Scientific and Civil-use Studies of the Earth
A1.1
Space-based and Sub-orbital Observations of Atmospheric Physics and Chemistry
A1.1
Space-based and Sub-orbital Observations of Atmospheric Physics and Chemistry
A1.1
Space-based and Sub-orbital Observations of Atmospheric Physics and Chemistry
F3.5
Pre-biotic and Complex Molecules in the Universe: Observational, Laboratory, and Computational Perspectives on the Evolution of Molecular Complexity
F3.5
Pre-biotic and Complex Molecules in the Universe: Observational, Laboratory, and Computational Perspectives on the Evolution of Molecular Complexity
F3.1
Chemical Evolution and Origin of Life
F3.1
Chemical Evolution and Origin of Life
F4.5
Space Food and Nutrition
F4.5
Space Food and Nutrition
PSB.1
Scientific Ballooning: Recent Developments in Technology and Instrumentation
H0.1
Commission H Highlight Talks
H0.1
Commission H Highlight Talks
H0.3
Space Missions for Fundamental Physics
H0.3
Space Missions for Fundamental Physics
F2.2
Space Radiation Risk, Quality of Radiation and Countermeasures: Physical and Biophysical Mechanisms, Modelling and Simulations
F2.4
Genetic, Epigenetic and Metabolic Changes in Spaceflight and Simulated Spaceflight Environment
F2.4
Genetic, Epigenetic and Metabolic Changes in Spaceflight and Simulated Spaceflight Environment
F2.2
Space Radiation Risk, Quality of Radiation and Countermeasures: Physical and Biophysical Mechanisms, Modelling and Simulations

Sponsors

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Major Supporters

Sponsors

Exhibitors

Fast Facts

The Help Desk was the most visited chat space with 48,540 posts and 8,848 unique viewers. Lockheed Martin’s workshop had a total of 103 posts and 118 unique viewers. The Climate Change topic was well above average with a total of 5,833 clicks followed by the Opening & Awards Ceremony with a total of 3,656 clicks.

Total registrants that attended was 11,410 and user total was 67,650.

  • Peak time was during the PM shift (Europe & Asia Pacific)

Most popular Spaces:

  1. Lobby with 29,957
  2. Full program with 26,960
  3. Scientific program with 16,201
  4. Lounge 1 – Genesis with 14,309
  5. Resources with 16,832 – peak time in the AM shift (Americas)

Top Documents:

  1. Cospar program posters 2021 with 491
  2. About COSPAR2022 with 450
  3. COSPAR Program Timetable 2021 with 424
  4. 2021 In Need of Space with 399
  5. Lockheed Martin Workshops with 373

Top Companies:

  1. Lockheed Martin
  2. CSIRO
  3. North-West University
  4. Jet Propulsion Laboratory
  5. UNSW

Post Congress Information

The Covid-19 pandemic forced deferral of the Sydney Assembly from August 2020 to January 2021 and redesign of the presentation mode from 100% in-person to either 100% virtual presentation or a mix of virtual and in-person presentations (COSPAR-2021-Hybrid).

During the events of the week, we all engaged with an extremely high quality COSPAR scientific program. There were 615 sessions, each delivered twice; over 2,000 scientific presentations; and three excellent workshops led by our anchor sponsor Lockheed Martin. Over 2,000 delegates were active on the platform each day. From the app, there have been over 2,000 downloads, more than 117 thousand page hits, and the number keeps rising. The assembly website has had over unique 11,000 users accessing content.

Testimonials

© COSPAR 2021