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BibTex format

author = {Grün, E and Agarwal, J and Altobelli, N and Altwegg, K and Bentley, MS and Biver, N and Della, Corte V and Edberg, N and Feldman, PD and Galand, M and Geiger, B and Götz, C and Grieger, B and Güttler, C and Henri, P and Hofstadter, M and Horanyi, M and Jehin, E and Krüger, H and Lee, S and Mannel, T and Morales, E and Mousis, O and Müller, M and Opitom, C and Rotundi, A and Schmied, R and Schmidt, F and Sierks, H and Snodgrass, C and Soja, RH and Sommer, M and Srama, R and Tzou, C-Y and Vincent, J-B and Yanamandra-Fisher, P and A'Hearn, MF and Erikson, AI and Barbieri, C and Barucci, MA and Bertaux, J-L and Bertini, I and Burch, J and Colangeli, L and Cremonese, G and Da, Deppo V and Davidsson, B and Debei, S and De, Cecco M and Deller, J and Feaga, LM and Ferrari, M and Fornasier, S and Fulle, M and Gicquel, A and Gillon, M and Green, SF and Groussin, O and Gutiérrez, PJ and Hofmann, M and Hviid, SF and Ip, W-H and Ivanovski, S and Jorda, L and Keller, HU and Knight, MM and Knollenber},
doi = {mnras/stw2088},
journal = {Monthly Notices of the Royal Astronomical Society},
pages = {S220--S234},
title = {The 2016 Feb 19 outburst of comet 67P/CG: an ESA Rosetta multi-instrument study},
url = {},
volume = {462},
year = {2016}

RIS format (EndNote, RefMan)

AB - On 2016 Feb 19, nine Rosetta instruments serendipitously observed an outburst of gas and dust from the nucleus of comet 67P/Churyumov-Gerasimenko. Among these instruments were cameras and spectrometers ranging from UV over visible to microwave wavelengths, in situ gas, dust and plasma instruments, and one dust collector. At 09:40 a dust cloud developed at the edge of an image in the shadowed region of the nucleus. Over the next two hours the instruments recorded a signature of the outburst that significantly exceeded the background. The enhancement ranged from 50 per cent of the neutral gas density at Rosetta to factors >100 of the brightness of the coma near the nucleus. Dust related phenomena (dust counts or brightness due to illuminated dust) showed the strongest enhancements (factors >10). However, even the electron density at Rosetta increased by a factor 3 and consequently the spacecraft potential changed from ∼−16 V to −20 V during the outburst. A clear sequence of events was observed at the distance of Rosetta (34 km from the nucleus): within 15 min the Star Tracker camera detected fast particles (∼25 m s−1) while 100 μm radius particles were detected by the GIADA dust instrument ∼1 h later at a speed of 6 m s−1. The slowest were individual mm to cm sized grains observed by the OSIRIS cameras. Although the outburst originated just outside the FOV of the instruments, the source region and the magnitude of the outburst could be determined.
AU - Grün,E
AU - Agarwal,J
AU - Altobelli,N
AU - Altwegg,K
AU - Bentley,MS
AU - Biver,N
AU - Della,Corte V
AU - Edberg,N
AU - Feldman,PD
AU - Galand,M
AU - Geiger,B
AU - Götz,C
AU - Grieger,B
AU - Güttler,C
AU - Henri,P
AU - Hofstadter,M
AU - Horanyi,M
AU - Jehin,E
AU - Krüger,H
AU - Lee,S
AU - Mannel,T
AU - Morales,E
AU - Mousis,O
AU - Müller,M
AU - Opitom,C
AU - Rotundi,A
AU - Schmied,R
AU - Schmidt,F
AU - Sierks,H
AU - Snodgrass,C
AU - Soja,RH
AU - Sommer,M
AU - Srama,R
AU - Tzou,C-Y
AU - Vincent,J-B
AU - Yanamandra-Fisher,P
AU - A'Hearn,MF
AU - Erikson,AI
AU - Barbieri,C
AU - Barucci,MA
AU - Bertaux,J-L
AU - Bertini,I
AU - Burch,J
AU - Colangeli,L
AU - Cremonese,G
AU - Da,Deppo V
AU - Davidsson,B
AU - Debei,S
AU - De,Cecco M
AU - Deller,J
AU - Feaga,LM
AU - Ferrari,M
AU - Fornasier,S
AU - Fulle,M
AU - Gicquel,A
AU - Gillon,M
AU - Green,SF
AU - Groussin,O
AU - Gutiérrez,PJ
AU - Hofmann,M
AU - Hviid,SF
AU - Ip,W-H
AU - Ivanovski,S
AU - Jorda,L
AU - Keller,HU
AU - Knight,MM
AU - Knollenberg,J
AU - Koschny,D
AU - Kramm,J-R
AU - Kührt,E
AU - Küppers,M
AU - Lamy,PL
AU - Lara,LM
AU - Lazzarin,M
AU - Lòpez-Moreno,JJ
AU - Manfroid,J
AU - Epifani,EM
AU - Marzari,F
AU - Naletto,G
AU - Oklay,N
AU - Palumbo,P
AU - Parker,JW
AU - Rickman,H
AU - Rodrigo,R
AU - Rodrìguez,J
AU - Schindhelm,E
AU - Shi,X
AU - Sordini,R
AU - Steffl,AJ
AU - Stern,SA
AU - Thomas,N
AU - Tubiana,C
AU - Weaver,HA
AU - Weissman,P
AU - Zakharov,VV
AU - Taylor,MGGT
DO - mnras/stw2088
EP - 234
PY - 2016///
SN - 1365-2966
SP - 220
TI - The 2016 Feb 19 outburst of comet 67P/CG: an ESA Rosetta multi-instrument study
T2 - Monthly Notices of the Royal Astronomical Society
UR -
UR -
VL - 462
ER -