The meeting will be held at the ESACPE Tennis Hall at ESTEC. 

 

     

Monday 23 Sept 2019

Title

Author

14:00

Intro

 

14:20

The Anhur region: pristine exposure of volatiles

Fornasier

14:40

Multi-instrument analysis of FUV emissions during solar events at comet 67P

Stephenson

15:00

The inner dust and gas comae of comet 67P from a multi-instrument modelling perspective.

Marschall

15:20

Discussion

 

15:30

Coffee

 

16:00

A duck with HiPS - Towards a 67P basemap as Hierarchical Progressive Survey

Grieger

16:20

Light scattering and thermal emission modelling of dust in 67P

Markkanen

16:40

The outgassing morphology of comet 67P from MIRO maps

Biver

17:00

Review of rotating non-spherical dust modelling calibrated with Rosetta/GIADA measurements: simulations with multi-instrument Rosetta data.

Ivanovski

17:20

Discussion

 

17:30

End

 

18:00

ICE BREAKER

 
     

Tuesday 24 Sept 2019

   

09:30

Characterization of a two-electron temperature plasma in the ionosphere of the comet 67P/Churyumov-Gerasimenko with the mutual impedance experiment (RPC-MIP) of Rosetta

GILET

09:50

Dynamic field line draping at comet 67P/CG during the Rosetta dayside excursion

Volwerk

10:10

'The infant bow shock - where and when does it exist?'

Götz

10:30

Discussion

 

10:45

Coffee

 

11:30

Polarisation of a small scale cometary plasma environment: Particle in Cell simulations

Gunell

11:50

Steepening of Magnetosonic Waves in the Inner Coma of 67P/Churyumov-Gerasimenko

Ostaszewski

12:10

Kinetic simulations of the interaction between the solar wind and a comet and feedback to Rosetta observations

Henri

12:30

Discussion

 

13:00

Lunch

 

14:00

The whole mission in your workspace: RPC-ICA moment data and what we can learn

Nilsson

14:20

Mechanical Properties of 67P/Churyumov–Gerasimenko surface material

Auster

14:40

Dust Particle Tracking at Comet 67P/Churyumov–Gerasimenko

Pfeifer

15:00

Bulk composition of volatiles versus early mission data from ROSINA

Fernandez-Valenzuela

15:20

Discussion

 

15:30

Coffee

 

16:00

Characterization of the refractory organic matter present in the dust particles of 67P/Churyumov-Gerasimenko.

Fray

16:20

Post-rendezvous radar properties of comet 67P/CG from the Rosetta Mission: Understanding future Earth-based radar observations and the dynamical evolution of comets

Heggy

16:40

Dust-to-gas and refractory-to-ice mass ratios of comet 67P/Churyumov-Gerasimenko from Rosetta observations

Choukroun

17:00

How Comets Work

Fulle

17:20

Discussion

 

17:30

End

 
     

Wednesday 25 Sept 2019

   

10:00

SWT

 

11:00

Coffee

 

11:30

SWT

 

13:00

Lunch

 

14:00

SWT

 

15:30

Coffee

 

16:00

SWT

 

17:00

END

 

18:00

Dinner

 
     

Thursday 26 Sept 2019

   

09:30

The CoPhyLab

Gundlach

09:50

Anomalous oxygen isotopes in O2 and SO/SO2

Altwegg

10:10

Analysis of the present state of the dusty gas coma modelling

Zakharov

10:30

Discussion

 

10:45

Coffee

 

11:30

3D viewer of comet 67P/Churyumov-Gerasimenko

Semon

11:50

Metal depletions in 67P’s dust: a new insight into primitive dust composition?

Baklouti

12:10

What glycine distributed source in 67P could tell us about the formation of organic matter in comets ?

Cottin

12:30

Discussion

 

13:00

Lunch

 

14:00

Short-term outbursts on 67P/ Churyumov-Gerasimenko and 2060 Chiron (95P/Chiron)

Buratti

14:20

The subunit size distributions of dust of comet 67P at the nanometre range

Mannel

14:40

The D/H Ratio Measured in the Dust of Comet 67P/ Churyumov-Gerasimenko Using Rosetta/COSIMA

Paquette

15:00

CN/HCN Ratio Seen with DFMS/ROSINA in the Inner Coma of Comet 67P/Churyumov-Gerasimenko

Haenni

15:20

Discussion

 

15:30

Coffee

 

16:00

Ingredients for Solar-like Systems: protostar IRAS 16293-2422 B versus comet 67P/Churyumov–Gerasimenko

Drozdovskaya

16:20

Quantification of Li abundance in the dust particles of 67P/Churyumov-Gerasimenko and its context in the relation between volatility and abundance in other elements

Stenzel

16:40

LICIACube mission overview and modelling dust dynamics of the plume evolution in support of the mission scientific objectives.

Ivanovski

17:00

A large chunk in temporary orbit around comet 67P

Kueppers

17:20

Discussion

 

17:30

End

 
     

Friday 27 Sept 2019

   

09:30

Sources of volatiles and dust on 67P: a cross instrument comparison

Kramer

09:50

From large interstellar organics to comets and prebiotic delivery

Foing

10:10

Bulk composition of volatiles versus early mission data from Rosina

Rubin

10:30

Discussion

 

10:45

Coffee

 

11:30

Open questions in cometary plasma physics

Götz

11:50

Predicted activity of a dynamically new comet – application for the proposed mission Comet Interceptor

Kossacki

12:10

Comet Interceptor - current status

Snodgrass

12:30

Discussion + wrap up + end

 

 

POSTERS-

Posters boards are provided in the main meeting area and will be up all week.

Due to the number of posters we will not have a dedicated poster session, but instead utilise the ice breaker and coffee breaks etc for poster interactions.

 

Lemos -      Global distribution and dynamics of dust near comet 67P/Churyumov-Gerasimenko

Odelstad-    Plasma waves near the diamagnetic cavity of 67P

Bucciantini- RPCMIP/RPCLAP CROSS-CALIBRATED DENSITY DATASET

Myllys-        Electric field measurements at plasma frequency and their solar wind drivers at comet 67P

Schroeder-  A comparison between the two lobes of comet 67P / Churyumov-Gerasimenko based on D/H ratios in H2O measured with the Rosetta / ROSINA DFMS 

 

 

 

SWT Schedule - 

 

SWT #52 - Wednesday 25 September 2019

 

Start 10:00


Introduction and update (including actions) – Matt
Mission Status – Patrick
NASA overview/summary - Bonnie/Art/Mathieu


Archiving update –
PSA overview & status - Dave
SPICE related presentation  - Bjorn
Rosetta archive presentation - Larry
PDS4 presentation - Anne Raugh
PDS SBN presentation - Tilden/Ludmilla 

Communications - a final word - Markus Bauer/Emily Baldwin/ Claudia Mignone
 

SWT summary presentations –     

PIs and IDSs are invited to present a summary of the mission from their perspective or simply report in their normal way – it is up to you, it is the last one after all.

 

End 17:00