Saturday 30 January 2021

Block 1

AM

Block 2

PM

D2.2
Solar Probe and SolO
D2.2
Solar Probe and SolO
D2.2
Solar Probe and SolO
D2.2
Solar Probe and SolO
G0.2
Drop Tower Days
G0.2
Drop Tower Days
G0.2
Drop Tower Days
G0.2
Drop Tower Days
D1.1
Acceleration and Transport of Energetic Particlesin the Heliosphere and Beyond
D1.1
Acceleration and Transport of Energetic Particlesin the Heliosphere and Beyond
D1.1
Acceleration and Transport of Energetic Particlesin the Heliosphere and Beyond
D1.1
Acceleration and Transport of Energetic Particlesin the Heliosphere and Beyond
PPP.1
Planetary Protection Policy
PPP.1
Planetary Protection Policy
PPP.1
Planetary Protection Policy
PPP.1
Planetary Protection Policy
PSW.7
Hands-on Education in Space Weather
PSW.7
Hands-on Education in Space Weather
PSW.7
Hands-on Education in Space Weather
PSW.7
Hands-on Education in Space Weather
PRBEM.2
Development of Global Physical, Empirical, and Data Assimilative Models of the Radiation Belt Environment
PRBEM.3
Dedicated Tools for Radiation Belt Modeling and Data Processing: An Opportunity to Gather Efforts
PRBEM.2
Development of Global Physical, Empirical, and Data Assimilative Models of the Radiation Belt Environment
PRBEM.3
Dedicated Tools for Radiation Belt Modeling and Data Processing: An Opportunity to Gather Efforts
D2.1
Space Climate
D2.1
Space Climate
D2.1
Space Climate
D2.1
Space Climate
B0.1
Unifying planetary system formation out of elementary building blocks: from dust, gas and ice to our Solar System and exoplanets
B0.1
Unifying planetary system formation out of elementary building blocks: from dust, gas and ice to our Solar System and exoplanets
B0.1
Unifying planetary system formation out of elementary building blocks: from dust, gas and ice to our Solar System and exoplanets
B0.1
Unifying planetary system formation out of elementary building blocks: from dust, gas and ice to our Solar System and exoplanets
B0.4
Technologies for Planetary Research
B0.4
Technologies for Planetary Research
B1.1
Small Body Exploration Science in the New Decade
B1.1
Small Body Exploration Science in the New Decade
B1.1
Small Body Exploration Science in the New Decade
B1.1
Small Body Exploration Science in the New Decade
B4.1
Mars Science Results
B4.1
Mars Science Results
B4.1
Mars Science Results
B4.1
Mars Science Results
B5.2
Gas Giant Planet Systems
B5.2
Gas Giant Planet Systems
B5.2
Gas Giant Planet Systems
B5.2
Gas Giant Planet Systems
PE.1
Teacher Training Workshop
PE.1
Teacher Training Workshop
E1.5
Accretion on All Scales
E1.5
Accretion on All Scales
E1.5
Accretion on All Scales
E1.5
Accretion on All Scales
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
E1.4
Black Hole Astrophysics: Observational Evidence and Theoretical Models
E1.16
Origin of Cosmic Rays
E1.16
Origin of Cosmic Rays
E1.16
Origin of Cosmic Rays
E1.16
Origin of Cosmic Rays
E1.6
X- and Gamma-ray Counterparts of New Transients in the Multimessenger Era
E1.6
X- and Gamma-ray Counterparts of New Transients in the Multimessenger Era
E1.6
X- and Gamma-ray Counterparts of New Transients in the Multimessenger Era
E1.6
X- and Gamma-ray Counterparts of New Transients in the Multimessenger Era
E1.13
High-energy Processes at the Galactic Center
E1.19
Scientific Opportunities from Multi-wavelength Follow-up of Largearea X-ray Surveys
E1.13
High-energy Processes at the Galactic Center
E1.19
Scientific Opportunities from Multi-wavelength Follow-up of Largearea X-ray Surveys
E1.1
Rapidly-rotating Neutron Stars
E1.1
Rapidly-rotating Neutron Stars
E1.1
Rapidly-rotating Neutron Stars
E1.1
Rapidly-rotating Neutron Stars
E2.2
Magnetic Structures of Solar Filaments
E2.2
Magnetic Structures of Solar Filaments
C4.2
Development of Models Related to the COSPAR International Reference Atmosphere and to ISO Standards for the Atmosphere
C4.2
Development of Models Related to the COSPAR International Reference Atmosphere and to ISO Standards for the Atmosphere
C4.2
Development of Models Related to the COSPAR International Reference Atmosphere and to ISO Standards for the Atmosphere
C4.2
Development of Models Related to the COSPAR International Reference Atmosphere and to ISO Standards for the Atmosphere
C1.4
CSES and Swarm Data Analysis of the Ionosphere Dynamics at Different Temporal and Spatial Scales
C1.3
Conditions for Enhanced Risk in Ionospheric Weather
C1.3
Conditions for Enhanced Risk in Ionospheric Weather
C2.2
Wave Coupling Processes and Consequences in the Whole Atmosphere and Ionosphere
C2.2
Wave Coupling Processes and Consequences in the Whole Atmosphere and Ionosphere
C2.2
Wave Coupling Processes and Consequences in the Whole Atmosphere and Ionosphere
C2.2
Wave Coupling Processes and Consequences in the Whole Atmosphere and Ionosphere
C1.2
The Coupled Solar Wind-Magnetosphere-Ionosphere-Thermosphere System and the Impact of Solar and Geomagnetic Storms on Geospace
C1.2
The Coupled Solar Wind-Magnetosphere-Ionosphere-Thermosphere System and the Impact of Solar and Geomagnetic Storms on Geospace
C1.2
The Coupled Solar Wind-Magnetosphere-Ionosphere-Thermosphere System and the Impact of Solar and Geomagnetic Storms on Geospace
C1.2
The Coupled Solar Wind-Magnetosphere-Ionosphere-Thermosphere System and the Impact of Solar and Geomagnetic Storms on Geospace
PSW.6
Global Coordination in Space Weather. Interfacing with User Groups
PSW.6
Global Coordination in Space Weather. Interfacing with User Groups
PSW.6
Global Coordination in Space Weather. Interfacing with User Groups
PSW.6
Global Coordination in Space Weather. Interfacing with User Groups
A0.3
Observing the Anthropocene from Space
A0.3
Observing the Anthropocene from Space
A0.3
Observing the Anthropocene from Space
A0.3
Observing the Anthropocene from Space
A2.1
Science and applications enabled by oceanographic satellite measurements
A2.1
Science and applications enabled by oceanographic satellite measurements
A2.1
Science and applications enabled by oceanographic satellite measurements
A2.1
Science and applications enabled by oceanographic satellite measurements
PSD.1
Satellite Dynamics - new Developments and Challenges for Earth and Solar System Sciences
PSD.1
Satellite Dynamics - new Developments and Challenges for Earth and Solar System Sciences
PSD.1
Satellite Dynamics - new Developments and Challenges for Earth and Solar System Sciences
PSD.1
Satellite Dynamics - new Developments and Challenges for Earth and Solar System Sciences
F0.1
Scientific Commission F Overview Talks
F0.1
Scientific Commission F Overview Talks
F0.1
Scientific Commission F Overview Talks
F0.1
Scientific Commission F Overview Talks

Sponsors

Hosted by

Anchor Partner

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