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  • Journal article
    Masters A, Thomsen MF, Badman SV, Arridge CS, Young DT, Coates AJ, Dougherty MKet al., 2011,

    Supercorotating return flow from reconnection in Saturn's magnetotail

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 38, ISSN: 0094-8276
  • Journal article
    Badman SV, Achilleos N, Baines KH, Brown RH, Bunce EJ, Dougherty MK, Melin H, Nichols JD, Stallard Tet al., 2011,

    Location of Saturn's northern infrared aurora determined from Cassini VIMS images

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 38, ISSN: 0094-8276
  • Report
    Haigh JD, 2011,

    Solar Influences on Climate

    , Grantham Institute for Climate Change Briefing Paper No 5, Publisher: Imperial College London
  • Journal article
    Wicks RT, Horbury TS, Chen CHK, Schekochihin AAet al., 2011,

    Anisotropy of Imbalanced Alfvenic Turbulence in Fast Solar Wind

    , Physical Review Letters, Vol: 106, Pages: 045001-045001, ISSN: 0031-9007
  • Journal article
    Voulgarakis A, Hadjinicolaou P, Pyle JA, 2011,

    Increases in global tropospheric ozone following an El Nino event: examining stratospheric ozone variability as a potential driver

    , ATMOSPHERIC SCIENCE LETTERS, Vol: 12, Pages: 228-232, ISSN: 1530-261X
  • Journal article
    Southwood DJ, 2011,

    Direct evidence of differences in magnetic rotation rate between Saturn’s northern andsouthern polar regions

    , J. Geophys. Res., Vol: 116

    The discovery of a difference in apparent rotation rate between Saturn kilometricradio emission from northern and southern hemispheres leads immediately to thequestion of whether there is a counterpart detectable in the Saturnian magnetic field. Wereport direct detection of a difference in the rotating magnetic signal measured by theCassini spacecraft magnetometer consistent with that seen in the radio signals.Theoretical consequences of the direct detection are discussed.
  • Conference paper
    Blackie D, Pickering JC, Rufus J, Thorne A, Stark G, Lyons J, Blackwell-Whitehead R, Smith PLet al., 2011,

    High resolution molecular spectroscopy with the imperial college UV FT spectrometer

    We report on a series of high resolution molecular spectroscopy measurements performed at Imperial College. We present: the first high resolution measurements of the absorption cross section of the <sup>x</sup>SO<inf>2</inf> (x = 32,33,34 and 36) isotopologues; and completion of a multitemperature study of the UV spectrum of SO<inf>2</inf>. © 2011 Optical Society of America.
  • Journal article
    Blackie D, Blackwell-Whitehead R, Stark G, Pickering JC, Smith PL, Rufus J, Thorne APet al., 2011,

    Erratum: High-resolution photoabsorption cross-section measurements of SO2 at 198 K from 213 to 325 nm (Journal of Geophysical Research E: Planets (2011) 116 (E03006) DOI: 10.1029/2010JE003707)

    , Journal of Geophysical Research Planets, Vol: 116, ISSN: 0148-0227
  • Journal article
    Fillingim MO, Eastwood JP, Parks GK, Angelopoulos V, Mann IR, Mende SB, Weatherwax ATet al., 2011,

    Polar UVI and THEMIS GMAG observations of the ionospheric response to a hot flow anomaly

    , JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, Vol: 73, Pages: 137-145, ISSN: 1364-6826
  • Journal article
    Thorne AP, Pickering JC, Semeniuk J, 2011,

    THE SPECTRUM AND TERM ANALYSIS OF V I

    , ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, Vol: 192, ISSN: 0067-0049
  • Journal article
    Blackwell-Whitehead R, Pavlenko YV, Nave G, Pickering JC, Jones HRA, Lyubchik Y, Nilsson Het al., 2011,

    Infrared Mn I laboratory oscillator strengths for the study of late type stars and ultracool dwarfs

    , ASTRONOMY & ASTROPHYSICS, Vol: 525, ISSN: 0004-6361
    • Cite
    • Citations: 12
  • Journal article
    Volwerk M, Berchem J, Bogdanova YV, Constantinescu OD, Dunlop MW, Eastwood JP, Escoubet P, Fazakerley AN, Frey H, Hasegawa H, Lavraud B, Panov EV, Shen C, Shi JK, Taylor MGGT, Wang J, Wild JA, Zhang QH, Amm O, Weygand JMet al., 2011,

    Interplanetary magnetic field rotations followed from L1 to the ground: the response of the Earth's magnetosphere as seen by multi-spacecraft and ground-based observations

    , ANNALES GEOPHYSICAE, Vol: 29, Pages: 1549-1569, ISSN: 0992-7689
  • Journal article
    Roy I, Haigh JD, 2011,

    The influence of solar variability and the quasi-biennial oscillation on lower atmospheric temperatures and sea level pressure

    , ATMOSPHERIC CHEMISTRY AND PHYSICS, Vol: 11, Pages: 11679-11687, ISSN: 1680-7316
  • Journal article
    Dhomse S, Chipperfield MP, Feng W, Haigh JDet al., 2011,

    Solar response in tropical stratospheric ozone: a 3-D chemical transport model study using ERA reanalyses

    , ATMOSPHERIC CHEMISTRY AND PHYSICS, Vol: 11, Pages: 12773-12786, ISSN: 1680-7316
  • Journal article
    Voulgarakis A, Telford PJ, Aghedo AM, Braesicke P, Faluvegi G, Abraham NL, Bowman KW, Pyle JA, Shindell DTet al., 2011,

    Global multi-year O<sub>3</sub>-CO correlation patterns from models and TES satellite observations

    , ATMOSPHERIC CHEMISTRY AND PHYSICS, Vol: 11, Pages: 5819-5838, ISSN: 1680-7316
  • Journal article
    Graven HD, Gruber N, 2011,

    Continental-scale enrichment of atmospheric <SUP>14</SUP>CO<sub>2</sub> from the nuclear power industry: potential impact on the estimation of fossil fuel-derived CO<sub>2</sub>

    , ATMOSPHERIC CHEMISTRY AND PHYSICS, Vol: 11, Pages: 12339-12349, ISSN: 1680-7316
  • Journal article
    Tinetti G, Cho JY-K, Griffith CA, Grasset O, Grenfell L, Guillot T, Koskinen TT, Moses JI, Pinfield D, Tennyson J, Tessenyi M, Wordsworth R, Aylward A, van Boekel R, Coradini A, Encrenaz T, Snellen I, Zapatero-Osorio MR, Bouwman J, du Foresto VC, Lopez-Morales M, Mueller-Wodarg I, Palle E, Selsis F, Sozzetti A, Beaulieu J-P, Henning T, Meyer M, Micela G, Ribas I, Stam D, Swain M, Krause O, Ollivier M, Pace E, Swinyard B, Ade PAR, Achilleos N, Adriani A, Agnor CB, Afonso C, Prieto CA, Bakos G, Barber RJ, Barlow M, Bernath P, Bezard B, Borde P, Brown LR, Cassan A, Cavarroc C, Ciaravella A, Cockell C, Coustenis A, Danielski C, Decin L, De Kok R, Demangeon O, Deroo P, Doel P, Drossart P, Fletcher LN, Focardi M, Forget F, Fossey S, Fouque P, Frith J, Galand M, Gaulme P, Hernandez JIG, Grassi D, Griffin MJ, Groezinger U, Guedel M, Guio P, Hainaut O, Hargreaves R, Hauschildt PH, Heng K, Heyrovsky D, Hueso R, Irwin P, Kaltenegger L, Kervella P, Kipping D, Kovacs G, La Barbera A, Lammar H, Lellouch E, Leto G, Morales ML, Valverde MAL, Lopez-Puertas M, Lovis C, Maggio A, Maillard J-P, Prado JM, Marquette J-B, Martin-Torres FJ, Maxted P, Miller S, Molinari S, Montes D, Moro-Martin A, Mousis O, Tuong NN, Nelson R, Orton GS, Pantin E, Pascale E, Pezzuto S, Poretti E, Prinja R, Prisinzano L, Reess J-M, Reiners A, Samuel B, Forcada JS, Sasselov D, Savini G, Sicardy B, Smith A, Stixrude L, Strazzulla G, Vasisht G, Vinatier S, Viti S, Waldmann I, White GJ, Widemann T, Yelle R, Yung Y, Yurchenko Set al., 2011,

    The science of EChO

    , ASTROPHYSICS OF PLANETARY SYSTEMS: FORMATION, STRUCTURE, AND DYNAMICAL EVOLUTION, Pages: 359-370, ISSN: 1743-9213
  • Conference paper
    Rodriguez-Martinez M, Blanco-Cano X, Russell CT, Leisner JS, Wilson RJ, Dougherty MK, Perez-Enriquez HRet al., 2011,

    WAVES AND INSTABILITIES IN THE MAGNETOSPHERIC PLASMA OF SATURN

    , 13th Latin American Regional Meeting of the International Astronomical Union, Publisher: UNIVERSIDAD NACIONAL AUTONOMA MEXICO INSTITUTO ASTRONOMIA, Pages: 295-295, ISSN: 1405-2059
  • Journal article
    Krasnoselskikh VV, de Wit TD, Bale SD, 2011,

    Determining the wavelength of Langmuir wave packets at the Earth's bow shock

    , ANNALES GEOPHYSICAE, Vol: 29, Pages: 613-617, ISSN: 0992-7689
  • Journal article
    Mushtaq S, Steers EBM, Pickering JC, Gusarova T, Smid P, Weinstein Vet al., 2011,

    Effects of traces of oxygen on Grimm-type glow discharges in argon

    , JOURNAL OF ANALYTICAL ATOMIC SPECTROMETRY, Vol: 26, Pages: 766-775, ISSN: 0267-9477
  • Report
    Orr PR, Twigger-Ross CL, Kashefi E, Rathouse K, Haigh JDet al., 2011,

    Evaluation of ‘Experiment Earth?’ Public Dialogue on Geoengineering. A report to the Natural Environment Research Council (NERC)

    , Publisher: Collingwood Environmental Planning Ltd, London
  • Book chapter
    Forster PM, DWJ T, Baldwin MP, Chipperfield M, Dameris M, Haigh JD, KAroly DJ, Kushner PJ, Randel WJ, Rosenlof KH, Seidel DJ, Solomon Cet al., 2011,

    Stratospheric Changes and Climate

    , Scientific Assessment of Ozone Depletion: 2010, Geneva, Publisher: World Meteorological Organisation
  • Journal article
    Gowen RA, Smith A, Fortes AD, Barber S, Brown P, Church P, Collinson G, Coates AJ, Collins G, Crawford IA, Dehant V, Chela-Flores J, Griffiths AD, Grindrod PM, Gurvitis LI, Hagermann A, Hussmann H, Jaumann R, Jones AP, Joy KH, Karatekin O, Miljkovic K, Palomba E, Pike WT, Prieto-Ballesteros O, Raulin F, Sephton MA, Sheridan S, Sims M, Storrie-Lombardi MC, Ambrosi R, Fielding J, Fraser G, Gao Y, Jones GH, Kargl G, Karl WJ, Macagnano A, Mukherjee A, Muller JP, Phipps A, Pullan D, Richter L, Sohl F, Snape J, Sykes J, Wells Net al., 2011,

    Penetrators for in situ subsurface investigations of Europa

    , ADV SPACE RES, Vol: 48, Pages: 725-742, ISSN: 0273-1177

    We present the scientific case for inclusion of penetrators into the Europan surface, and the candidate instruments which could significantly enhance the scientific return of the joint ESA/NASA Europa-Jupiter System Mission (EJSM). Moreover, a surface element would provide an exciting and inspirational mission highlight which would encourage public and political support for the mission.Whilst many of the EJSM science goals can be achieved from the proposed orbital platform, only surface elements can provide key exploration capabilities including direct chemical sampling and associated astrobiological material detection, and sensitive habitability determination. A targeted landing site of upwelled material could provide access to potential biological material originating from deep beneath the ice.Penetrators can also enable more capable geophysical investigations of Europa (and Ganymede) interior body structures, mineralogy, mechanical, magnetic, electrical and thermal properties. They would provide ground truth, not just for the orbital observations of Europa, but could also improve confidence of interpretation of observations of the other Jovian moons. Additionally, penetrators on both Europa and Ganymede, would allow valuable comparison of these worlds, and gather significant information relevant to future landed missions. The advocated low mass penetrators also offer a comparatively low cost method of achieving these important science goals.A payload of two penetrators is proposed to provide redundancy, and improve scientific return, including enhanced networked seismometer performance and diversity of sampled regions.We also describe the associated candidate instruments, penetrator system architecture, and technical challenges for such penetrators, and include their current status and future development plans.
  • Journal article
    Mushtaq S, Pickering JC, Steers EBM, Horvath P, Whitby JA, Michler Jet al., 2011,

    The role of oxygen in analytical glow discharges: GD-OES and GD-ToF-MS studies

    , JOURNAL OF ANALYTICAL ATOMIC SPECTROMETRY, Vol: 26, Pages: 1746-1755, ISSN: 0267-9477
  • Journal article
    Dunlop MW, Zhang Q-H, Bogdanova YV, Trattner KJ, Pu Z, Hasegawa H, Berchem J, Taylor MGGT, Volwerk M, Eastwood JP, Lavraud B, Shen C, Shi J-K, Wang J, Constantinescu D, Fazakerley AN, Frey H, Sibeck D, Escoubet P, Wild JA, Liu ZX, Carr Cet al., 2011,

    Magnetopause reconnection across wide local time

    , ANNALES GEOPHYSICAE, Vol: 29, Pages: 1683-1697, ISSN: 0992-7689
    • Cite
    • Citations: 60
  • Journal article
    Andrews DJ, Coates AJ, Cowley SWH, Dougherty MK, Lamy L, Provan G, Zarka Pet al., 2010,

    Magnetospheric period oscillations at Saturn: Comparison of equatorial and high-latitude magnetic field periods with north and south Saturn kilometric radiation periods

    , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380
  • Journal article
    Burton ME, Dougherty MK, Russell CT, 2010,

    Saturn's internal planetary magnetic field

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 37, ISSN: 0094-8276
  • Journal article
    Simpson IR, Blackburn M, Haigh JD, Sparrow SNet al., 2010,

    The Impact of the State of the Troposphere on the Response to Stratospheric Heating in a Simplified GCM

    , JOURNAL OF CLIMATE, Vol: 23, Pages: 6166-6185, ISSN: 0894-8755
  • Conference paper
    Magner T, Erd C, Pappalardo R, Blanc M, Bunce E, Clark K, Coustenis A, Dougherty M, Gavin T, Grasset O, Greeley R, Van Houten T, Lebreton JP, Prockter LM, Senske D, Sturm E, Titov Det al., 2010,

    The europa jupiter system mission (EJSM): Exploring the emergence of habitable worlds around gas giants

    , Pages: 10338-10350

    The Europa Jupiter System Mission (EJSM) would be an international mission with the overall theme of investigating the emergence of habitable worlds around gas giants. Its goals would be to (1) Explore Europa to investigate its habitability, (2) Characterize Ganymede as a planetary object including its potential habitability and (3) Explore the Jupiter system as an archetype for gas giants. NASA and ESA have concluded a detailed joint study of a mission to Europa, Ganymede, and the Jupiter system. The EJSM architecture consists of two primary elements operating in the Jovian system: the NASA-led Jupiter Europa Orbiter (JEO), and the ESA-led Jupiter Ganymede Orbiter (JGO). JEO and JGO would execute a choreographed exploration of the Jupiter System before settling into orbit around Europa and Ganymede, respectively. EJSM would directly address themes concerning the origin and evolution of icy satellite systems and water-rich environments therein. The potential habitability of the ocean-bearing moons Europa and Ganymede would be investigated, by characterizing the geophysical, compositional, geological, and external processes that affect these icy worlds. EJSM would also investigate Io and Callisto, small satellites and rings, Jupiter's atmosphere, and the Jovian magnetosphere. By better understanding the Jupiter system and unraveling its history, the formation and evolution of gas giant planets and their satellites would be better known. Most important, EJSM would shed new light on the potential for the emergence of life in our celestial neighborhood and beyond. The EJSM notional architecture provides opportunities for coordinated synergistic observations by JEO and JGO of the Jupiter and Ganymede magnetospheres, the volcanoes and torus of Io, the atmosphere of Jupiter, and comparative planetology of icy satellites. Each spacecraft would conduct both such synergistic dual-spacecraft investigations and also stand-alone measurements toward the overall mission theme and
  • Journal article
    Krasnoselskikh V, Vekstein G, Hudson HS, Bale SD, Abbett WPet al., 2010,

    GENERATION OF ELECTRIC CURRENTS IN THE CHROMOSPHERE VIA NEUTRAL-ION DRAG

    , ASTROPHYSICAL JOURNAL, Vol: 724, Pages: 1542-1550, ISSN: 0004-637X

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