Imperial College London

Dr Ravindra T. Desai

Faculty of Natural SciencesDepartment of Physics

Academic Visitor
 
 
 
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Contact

 

ravindra.desai Website

 
 
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Location

 

Blackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@unpublished{Rymer:2018,
author = {Rymer, A and Mandt, K and Hurley, D and Lisse, C and Izenberg, N and Smith, HT and Westlake, J and Bunce, E and Arridge, C and Masters, A and Hofstadter, M and Simon, A and Brandt, P and Clark, G and Cohen, I and Allen, R and Vine, S and Hansen, K and Hospodarsky, G and Kurth, W and Romani, P and Lamy, L and Zarka, P and Cao, H and Paty, C and Hedman, M and Roussos, E and Cruikshank, D and Farrell, W and Fieseler, P and Coates, A and Yelle, R and Parkinson, C and Militzer, B and Grodent, D and Kollmann, P and McNutt, R and André, N and Strange, N and Barnes, J and Dones, L and Denk, T and Rathbun, J and Lunine, J and Desai, R and Cochrane, C and Sayanagi, KM and Postberg, F and Ebert, R and Hill, T and Mueller-Wodarg, I and Regoli, L and Pontius, D and Stanley, S and Greathouse, T and Saur, J and Marouf, E and Bergman, J and Higgins, C and Johnson, R and Thomsen, M and Soderlund, K and Jia, X and Wilson, R and Englander, J and Burch, J and Nordheim, T and Grava, C and Baines, K and Qui},
title = {Solar System Ice Giants: Exoplanets in our Backyard},
url = {http://arxiv.org/abs/1804.03573v1},
year = {2018}
}

RIS format (EndNote, RefMan)

TY  - UNPB
AB - Future remote sensing of exoplanets will be enhanced by a thoroughinvestigation of our solar system Ice Giants (Neptune-size planets). What canthe configuration of the magnetic field tell us (remotely) about the interior,and what implications does that field have for the structure of themagnetosphere; energy input into the atmosphere, and surface geophysics (forexample surface weathering of satellites that might harbour sub-surfaceoceans). How can monitoring of auroral emission help inform future remoteobservations of emission from exoplanets? Our Solar System provides the onlylaboratory in which we can perform in-situ experiments to understand exoplanetformation, dynamos, systems and magnetospheres.
AU - Rymer,A
AU - Mandt,K
AU - Hurley,D
AU - Lisse,C
AU - Izenberg,N
AU - Smith,HT
AU - Westlake,J
AU - Bunce,E
AU - Arridge,C
AU - Masters,A
AU - Hofstadter,M
AU - Simon,A
AU - Brandt,P
AU - Clark,G
AU - Cohen,I
AU - Allen,R
AU - Vine,S
AU - Hansen,K
AU - Hospodarsky,G
AU - Kurth,W
AU - Romani,P
AU - Lamy,L
AU - Zarka,P
AU - Cao,H
AU - Paty,C
AU - Hedman,M
AU - Roussos,E
AU - Cruikshank,D
AU - Farrell,W
AU - Fieseler,P
AU - Coates,A
AU - Yelle,R
AU - Parkinson,C
AU - Militzer,B
AU - Grodent,D
AU - Kollmann,P
AU - McNutt,R
AU - André,N
AU - Strange,N
AU - Barnes,J
AU - Dones,L
AU - Denk,T
AU - Rathbun,J
AU - Lunine,J
AU - Desai,R
AU - Cochrane,C
AU - Sayanagi,KM
AU - Postberg,F
AU - Ebert,R
AU - Hill,T
AU - Mueller-Wodarg,I
AU - Regoli,L
AU - Pontius,D
AU - Stanley,S
AU - Greathouse,T
AU - Saur,J
AU - Marouf,E
AU - Bergman,J
AU - Higgins,C
AU - Johnson,R
AU - Thomsen,M
AU - Soderlund,K
AU - Jia,X
AU - Wilson,R
AU - Englander,J
AU - Burch,J
AU - Nordheim,T
AU - Grava,C
AU - Baines,K
AU - Quick,L
AU - Russell,C
AU - Cravens,T
AU - Cecconi,B
AU - Aslam,S
AU - Bray,V
AU - Garcia-Sage,K
AU - Richardson,J
AU - Clark,J
AU - Hsu,S
AU - Achterberg,R
AU - Sergis,N
AU - Paganelli,F
AU - Kempf,S
AU - Orton,G
AU - Portyankina,G
AU - Jones,G
AU - Economou,T
AU - Livengood,T
AU - Krimigi,S
AU - Szalay,J
AU - Jackman,C
AU - Valek,P
AU - Lecacheux,A
AU - Colwell,J
AU - Jasinski,J
AU - Tosi,F
AU - Sulaiman,A
AU - Galand,M
AU - Kotova,A
AU - Khurana,K
AU - Kivelson,M
AU - Strobel,D
AU - Radiota,A
AU - Estrada,P
AU - Livi,S
AU - Azari,A
AU - Yates,J
AU - Allegrini,F
AU - Vogt,M
AU - Felici,M
AU - Luhmann,J
AU - Filacchione,G
AU - Moore,L
PY - 2018///
TI - Solar System Ice Giants: Exoplanets in our Backyard
UR - http://arxiv.org/abs/1804.03573v1
UR - http://hdl.handle.net/10044/1/65724
ER -