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• Journal article
  Ryder CL, Highwood EJ, Rosenberg PD, Trembath J, Brooke JK, Bart M, Dean A, Crosier J, Dorsey J, Brindley H, Banks J, Marsham JH, McQuaid JB, Sodemann H, Washington Ret al., 2013,
  , ATMOSPHERIC CHEMISTRY AND PHYSICS, Vol: 13, Pages: 303-325, ISSN: 1680-7316
  • Cite
  • Citations: 154
• Journal article
  Shindell DT, Faluvegi G, Nazarenko L, Bowman K, Lamarque HF, Voulgarakis A, Schmidt GA, Pechony O, Ruedy Ret al., 2013,
  , Nature Climate Change, Vol: 3, Pages: 567-570
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• Journal article
  Archer MO, Horbury TS, 2013,
  , Ann. Geophys., Vol: 31, Pages: 319-331
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• Journal article
  See V, Cameron RF, Schwartz SJ, 2013,
  , ANNALES GEOPHYSICAE, Vol: 31, Pages: 639-646, ISSN: 0992-7689
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  • Citations: 20
• Journal article
  Khatiwala S, Tanhua T, Fletcher SM, Gerber M, Doney SC, Graven HD, Gruber N, McKinley GA, Murata A, Rios AF, Sabine CLet al., 2013,
  , BIOGEOSCIENCES, Vol: 10, Pages: 2169-2191, ISSN: 1726-4170
  • Cite
  • Citations: 389
• Journal article
  Wanninkhof R, Park G-H, Takahashi T, Sweeney C, Feely R, Nojiri Y, Gruber N, Doney SC, McKinley GA, Lenton A, Le Quere C, Heinze C, Schwinger J, Graven H, Khatiwala Set al., 2013,
  , BIOGEOSCIENCES, Vol: 10, Pages: 1983-2000, ISSN: 1726-4170
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  • Citations: 297
• Journal article
  Yver CE, Graven HD, Lucas DD, Cameron-Smith PJ, Keeling RF, Weiss RFet al., 2013,
  , ATMOSPHERIC CHEMISTRY AND PHYSICS, Vol: 13, Pages: 1837-1852, ISSN: 1680-7316
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  • Citations: 29
• Journal article
  Archer MO, Horbury TS, Eastwood JP, Weygand JM, Yeoman TKet al., 2013,
  , Journal of Geophysical Research, Vol: 118, Pages: 5454-5466

  Abstract. We present observations from the magnetopause to the ground during periods of large amplitude, transient dynamic pressure pulses in the magnetosheath. While individual magnetosheath pulses are sharp and impulsive, the magnetospheric response is much smoother with frequencies in the Pc5-6 range being excited in the compressional and poloidal components of the magnetic field. We show that the magnetopause acts like a low pass filter, suppressing timescales shorter than a few minutes. Further filtering appears to occur locally within the magnetosphere, which may be due to the unusual field line resonance frequency profile on this day. Ground magnetometer and radar data along with equivalent ionospheric currents show signatures of travelling convection vortices, similar to the response from pressure variations of solar wind origin. However, the signatures are associated with groups of magnetosheath pulses rather than individual ones due to the impulsive nature of the pressure variations. Thus the scale-dependent magnetospheric response to these transient pressure variations, results in coherent signatures on longer timescales than any individual pulse.

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• Journal article
  Turnbull J, Graven H, Miller J, Lehman Set al., 2013,
  , RADIOCARBON, Vol: 55, Pages: 1470-1474, ISSN: 0033-8222
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  • Citations: 2
• Journal article
  Miller J, Lehman S, Wolak C, Turnbull J, Dunn G, Graven H, Keeling R, Meijer HAJ, Aerts-Bijma AT, Palstra SWL, Smith AM, Allison C, Southon J, Xu X, Nakazawa T, Aoki S, Nakamura T, Guilderson T, LaFranchi B, Mukai H, Terao Y, Uchida M, Kondo Met al., 2013,
  , RADIOCARBON, Vol: 55, Pages: 1475-1483, ISSN: 0033-8222
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  • Citations: 13
• Journal article
  Stallard TS, Masters A, Miller S, Melin H, Bunce EJ, Arridge CS, Achilleos N, Dougherty MK, Cowley SWHet al., 2012,
  , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 117, ISSN: 2169-9380
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  • Citations: 20
• Conference paper
  Yoon S, Kim V, Yun J, Seon J, Jin H, Chae KS, Lee DH, Lin RP, Sample J, Immel T, Kim J, Horbury TS, Brown Pet al., 2012,

  Operations for two spacecraft of triple-cubesat mission trio-cinema with a single rf chain

  , Pages: 4240-4245, ISSN: 0074-1795

  TRiplet Ionospheric Observatory - Cubesat for Ion, Neutral, Electron and MAgnetic fields (TRIO-CINEMA) mission consists of three identical 3U cubesats for scientific observation. The TRIO-CINEMA mission will provide high sensitivity mapping and high cadence measurements of ring current Energetic Neutral Atom (ENA) in the range of 4 - 200 keV with 1 keV FWHM energy resolution in Low Earth Orbit (LEO). Each spacecraft is equipped with a Supra Thermal Electrons, Ions, Neutrals (STEIN) instrument and a MAGnetometer 911���պ��� College (MAGIC) instrument. STEIN instrument is improved from those in SupraThermal Electron (STE) instrument flown on NASA's Solar TERrestrial Relations Observatory (STEREO) spacecraft and is capable of identifying electrons, positive ions and neutrals through the application of an electric field in the entrance aperture. MAGIC is dual 3-axis magnetoresistive sensor for attitude control and scientific measurement. First spacecraft of TRIO-CINEMA is developed and will be operated by Space Science Laboratory of University of California, Berkeley (UCB). Another two spacecraft are developed by Kyung Hee University (KHU) in Republic of Korea. TRIO-CINEMA is expected to provide stereo imaging of ENAs and multi-point measurements of ions, electrons and Earth magnetic fields. It is also expected that the TRIO-CINEMA measurements will complement the measurements with NASA's Radiation Belt Storm Probes (RBSP) mission by stereo imaging of the ring current through ENA measurements at low altitudes. TRIO-CINEMA data will be transmitted at 1 Mbps via S-band, whereas a UHF receiver is used for uplink communication. UCB will operate the mission via Mission Operations Center (MOC) and Berkeley Ground Station (BGS) of Space Science Laboratory (SSL). KHU has constructed a new ground station with one UHF RF system for uplink. The two KHU's spacecraft will be initially contiguous with each other deployed from the same launcher. Because the ground S-band antenna can prov

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• Journal article
  Landi S, Matteini L, Pantellini F, 2012,
  , ASTROPHYSICAL JOURNAL, Vol: 760, ISSN: 0004-637X
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  • Citations: 57
• Journal article
  Scherrer SC, Ceppi P, Croci-Maspoli M, Appenzeller Cet al., 2012,
  , Theoretical and Applied Climatology, Vol: 110, Pages: 509-516, ISSN: 0177-798X

  We quantify the effect of the snow-albedo feedback on Swiss spring temperature trends using daily temperature and snow depth measurements from six station pairs for the period 1961–2011. We show that the daily mean 2-m temperature of a spring day without snow cover is on average 0.4 °C warmer than one with snow cover at the same location. This estimate is comparable with estimates from climate modelling studies. Caused by the decreases in snow pack, the snow-albedo feedback amplifies observed temperature trends in spring. The influence is small and confined to areas around the upward-moving snow line in spring and early summer. For the 1961–2011 period, the related temperature trend increases are in the order of 3–7 % of the total observed trend.

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• Journal article
  Hausmann U, Czaja A, 2012,
  , DEEP-SEA RESEARCH PART I-OCEANOGRAPHIC RESEARCH PAPERS, Vol: 70, Pages: 60-72, ISSN: 0967-0637
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  • Citations: 138
• Journal article
  Cui J, Yelle RV, Strobel DF, Mueller-Wodarg ICF, Snowden DS, Koskinen TT, Galand Met al., 2012,
  , JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, Vol: 117, ISSN: 2169-9097
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  • Citations: 45
• Journal article
  Shen C, Rong ZJ, Dunlop MW, Ma YH, Li X, Zeng G, Yan GQ, Wan WX, Liu ZX, Carr CM, Reme Het al., 2012,
  , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 117, ISSN: 2169-9380
  • Cite
  • Citations: 34
• Journal article
  Moore L, Fischer G, Mueller-Wodarg I, Galand M, Mendillo Met al., 2012,
  , ICARUS, Vol: 221, Pages: 508-516, ISSN: 0019-1035
  • Cite
  • Citations: 11
• Journal article
  Gryspeerdt E, Stier P, 2012,
  , GEOPHYSICAL RESEARCH LETTERS, Vol: 39, ISSN: 0094-8276
  • Cite
  • Citations: 78
• Journal article
  Cargill PJ, Vlahos L, Baumann G, Drake JF, Nordlund Aet al., 2012,
  , SPACE SCIENCE REVIEWS, Vol: 173, Pages: 223-245, ISSN: 0038-6308
  • Cite
  • Citations: 67
• Journal article
  Matteini L, Hellinger P, Landi S, Trávníček PM, Velli Met al., 2012,
  , Space Science Reviews, Vol: 172, Pages: 373-396, ISSN: 0038-6308
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• Journal article
  Balogh A, Bykov A, Lin R, Raymond J, Scholer Met al., 2012,
  , SPACE SCIENCE REVIEWS, Vol: 173, Pages: 1-4, ISSN: 0038-6308
  • Cite
  • Citations: 3
• Journal article
  Cargill PJ, Bradshaw SJ, Klimchuk JA, 2012,
  , ASTROPHYSICAL JOURNAL, Vol: 758, ISSN: 0004-637X
  • Cite
  • Citations: 64
• Journal article
  Moestl C, Farrugia CJ, Kilpua EKJ, Jian LK, Liu Y, Eastwood JP, Harrison RA, Webb DF, Temmer M, Odstrcil D, Davies JA, Rollett T, Luhmann JG, Nitta N, Mulligan T, Jensen EA, Forsyth R, Lavraud B, de Koning CA, Veronig AM, Galvin AB, Zhang TL, Anderson BJet al., 2012,
  , ASTROPHYSICAL JOURNAL, Vol: 758, ISSN: 0004-637X
  • Cite
  • Citations: 105
• Journal article
  Chen CHK, Mallet A, Schekochihin AA, Horbury TS, Wicks RT, Bale SDet al., 2012,
  , The Astrophysical Journal, Vol: 758, Pages: 120-120

  We present a measurement of the scale-dependent, three-dimensional structureof the magnetic field fluctuations in inertial range solar wind turbulence withrespect to a local, physically motivated coordinate system. The Alfvenicfluctuations are three-dimensionally anisotropic, with the sense of thisanisotropy varying from large to small scales. At the outer scale, the magneticfield correlations are longest in the local fluctuation direction, consistentwith Alfven waves. At the proton gyroscale, they are longest along the localmean field direction and shortest in the direction perpendicular to the localmean field and the local field fluctuation. The compressive fluctuations arehighly elongated along the local mean field direction, although axiallysymmetric perpendicular to it. Their large anisotropy may explain why they arenot heavily damped in the solar wind.

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• Journal article
  Ceppi P, Hwang Y-T, Frierson DMW, Hartmann DLet al., 2012,
  , Geophysical Research Letters, Vol: 39, Pages: 1-5, ISSN: 0094-8276

  [1] Substantial biases in shortwave cloud forcing (SWCF) of up to ±30 W m−2are found in the midlatitudes of the Southern Hemisphere in the historical simulations of 34 CMIP5 coupled general circulation models. The SWCF biases are shown to induce surface temperature anomalies localized in the midlatitudes, and are significantly correlated with the mean latitude of the eddy‐driven jet, with a negative SWCF bias corresponding to an equatorward jet latitude bias. Aquaplanet model experiments are performed to demonstrate that the jet latitude biases are primarily induced by the midlatitude SWCF anomalies, such that the jet moves toward (away from) regions of enhanced (reduced) temperature gradients. The results underline the necessity of accurately representing cloud radiative forcings in state‐of‐the‐art coupled models.

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• Journal article
  Graven HD, Gruber N, Key R, Khatiwala S, Giraud Xet al., 2012,
  , JOURNAL OF GEOPHYSICAL RESEARCH-OCEANS, Vol: 117, ISSN: 2169-9275
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  • Citations: 104
• Journal article
  Christophe B, Spilker LJ, Anderson JD, André N, Asmar SW, Aurnou J, Banfield D, Barucci A, Bertolami O, Bingham R, Brown P, Cecconi B, Courty J-M, Dittus H, Fletcher LN, Foulon B, Francisco F, Gil PJS, Glassmeier KH, Grundy W, Hansen C, Helbert J, Helled R, Hussmann H, Lamine B, Lämmerzahl C, Lamy L, Lehoucq R, Lenoir B, Levy A, Orton G, Páramos J, Poncy J, Postberg F, Progrebenko SV, Reh KR, Reynaud S, Robert C, Samain E, Saur J, Sayanagi KM, Schmitz N, Selig H, Sohl F, Spilker TR, Srama R, Stephan K, Touboul P, Wolf Pet al., 2012,
  , Experimental Astronomy, Vol: 34, Pages: 203-242, ISSN: 0922-6435
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• Journal article
  Tinetti G, Beaulieu JP, Henning T, Meyer M, Micela G, Ribas I, Stam D, Swain M, Krause O, Ollivier M, Pace E, Swinyard B, Aylward A, van Boekel R, Coradini A, Encrenaz T, Snellen I, Zapatero-Osorio MR, Bouwman J, Cho JY-K, du Foresto VC, Guillot T, Lopez-Morales M, Mueller-Wodarg I, Palle E, Selsis F, Sozzetti A, Ade PAR, Achilleos N, Adriani A, Agnor CB, Afonso C, Allende Prieto C, Bakos G, Barber RJ, Barlow M, Batista V, 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, Gonzalez Hernandez JI, Grasset O, Grassi D, Grenfell JL, Griffin MJ, Griffith CA, 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, Koskinen TT, Kovacs G, La Barbera A, Lammer H, Lellouch E, Leto G, Lopez Valverde MA, Lopez-Puertas M, Lovis C, Maggio A, Maillard JP, Maldonado Prado J, Marquette JB, Martin-Torres FJ, Maxted P, Miller S, Molinari S, Montes D, Moro-Martin A, Moses JI, Mousis O, Nguyen Tuong N, Nelson R, Orton GS, Pantin E, Pascale E, Pezzuto S, Pinfield D, Poretti E, Prinja R, Prisinzano L, Rees JM, Reiners A, Samuel B, Sanchez-Lavega A, Sanz Forcada J, Sasselov D, Savini G, Sicardy B, Smith A, Stixrude L, Strazzulla G, Tennyson J, Tessenyi M, Vasisht G, Vinatier S, Viti S, Waldmann I, White GJ, Widemann T, Wordsworth R, Yelle R, Yung Y, Yurchenko SNet al., 2012,
  , EXPERIMENTAL ASTRONOMY, Vol: 34, Pages: 311-353, ISSN: 0922-6435
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  • Citations: 108
• Journal article
  Orr A, Bracegirdle TJ, Hosking JS, Jung T, Haigh JD, Phillips T, Feng Wet al., 2012,
  , JOURNAL OF THE ATMOSPHERIC SCIENCES, Vol: 69, Pages: 2917-2932, ISSN: 0022-4928
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  • Citations: 28

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