@article{Walsh:2020:0004-6361/201936894,
author = {Walsh, AP and Horbury, TS and Maksimovic, M and Owen, CJ and Rodriguez-Pacheco, J and Wimmer-Schweingruber, RF and Zouganelis, I and Anekallu, C and Bonnin, X and Bruno, R and Carrasco, Blazquez I and Cernuda, I and Chust, T and De, Groof A and Espinosa, Lara F and Fazakerley, AN and Gilbert, HR and Gomez-Herrero, R and Ho, GC and Krucker, S and Lepri, ST and Lewis, GR and Livi, S and Louarn, P and Mueller, D and Nieves-Chinchilla, T and O'Brien, H and Osuna, P and Plasson, P and Raines, JM and Rouillard, AP and St, Cyr OC and Sanchez, L and Soucek, J and Varsani, A and Verscharen, D and Watson, CJ and Watson, G and Williams, DR},
doi = {0004-6361/201936894},
journal = {Astronomy and Astrophysics: a European journal},
pages = {1--7},
title = {Coordination of the in situ payload of Solar Orbiter},
url = {http://dx.doi.org/10.1051/0004-6361/201936894},
volume = {642},
year = {2020}
}

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TY  - JOUR
AB  - Solar Orbiter’s in situ coordination working group met frequently during the development of the mission with the goal of ensuring that its in situ payload has the necessary level of coordination to maximise science return. Here we present the results of that work, namely how the design of each of the in situ instruments (EPD, MAG, RPW, SWA) was guided by the need for coordination, the importance of time synchronisation, and how science operations will be conducted in a coordinated way. We discuss the mechanisms by which instrument sampling schemes are aligned such that complementary measurements will be made simultaneously by different instruments, and how burst modes are scheduled to allow a maximum overlap of burst intervals between the four instruments (telemetry constraints mean different instruments can spend different amounts of time in burst mode). We also explain how onboard autonomy, inter-instrument communication, and selective data downlink will be used to maximise the number of transient events that will be studied using high-resolution modes of all the instruments. Finally, we briefly address coordination between Solar Orbiter’s in situ payload and other missions.
AU  - Walsh,AP
AU  - Horbury,TS
AU  - Maksimovic,M
AU  - Owen,CJ
AU  - Rodriguez-Pacheco,J
AU  - Wimmer-Schweingruber,RF
AU  - Zouganelis,I
AU  - Anekallu,C
AU  - Bonnin,X
AU  - Bruno,R
AU  - Carrasco,Blazquez I
AU  - Cernuda,I
AU  - Chust,T
AU  - De,Groof A
AU  - Espinosa,Lara F
AU  - Fazakerley,AN
AU  - Gilbert,HR
AU  - Gomez-Herrero,R
AU  - Ho,GC
AU  - Krucker,S
AU  - Lepri,ST
AU  - Lewis,GR
AU  - Livi,S
AU  - Louarn,P
AU  - Mueller,D
AU  - Nieves-Chinchilla,T
AU  - O'Brien,H
AU  - Osuna,P
AU  - Plasson,P
AU  - Raines,JM
AU  - Rouillard,AP
AU  - St,Cyr OC
AU  - Sanchez,L
AU  - Soucek,J
AU  - Varsani,A
AU  - Verscharen,D
AU  - Watson,CJ
AU  - Watson,G
AU  - Williams,DR
DO  - 0004-6361/201936894
EP  - 7
PY  - 2020///
SN  - 0004-6361
SP  - 1
TI  - Coordination of the in situ payload of Solar Orbiter
T2  - Astronomy and Astrophysics: a European journal
UR  - http://dx.doi.org/10.1051/0004-6361/201936894
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000577099700005&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - https://www.aanda.org/articles/aa/abs/2020/10/aa36894-19/aa36894-19.html
UR  - http://hdl.handle.net/10044/1/83848
VL  - 642
ER  - 

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