{"id":521,"date":"2015-03-06T10:34:35","date_gmt":"2015-03-06T10:34:35","guid":{"rendered":"http:\/\/www.radio-science.eu\/?page_id=521"},"modified":"2023-11-10T10:15:25","modified_gmt":"2023-11-10T10:15:25","slug":"chef","status":"publish","type":"page","link":"https:\/\/fip-koeln.de\/en_us\/team\/chef\/","title":{"rendered":"Martin"},"content":{"rendered":"
\"Placeholder<\/figure>\n\n\n\n

PD Dr. Martin P\u00e4tzold<\/p>\n\n\n\n

Position<\/span>:
Director of the department Planetary Science of the Rhenish Institute for Environmental Research (RIU-PF)
Principal Investigator (PI) of the Radio Science Experiments on Mars Express (MaRS), Rosetta (RSI) and Co-PI of the Radio Science Experiment VeRa on Venus Express.
Tel.: +49 221 277 81 81-0<\/p>\n\n\n\n

About me<\/summary>\nPersonal Information:<\/b><\/span>\n
    \n \t
  • Date of birth:                        16 January 1960<\/li>\n \t
  • Place of birth:                      Gladbeck, Westfalia, Federal Republic of Germany<\/li>\n<\/ul>\nEducation:<\/b><\/span>\n
      \n \t
    • November 1998       Habilitation and Venia Legendi in Geophysics, Universit\u00e4t zu K\u00f6ln, Cologne, Germany\nThesis: \u201cRadiosondierung solarer und kometarer Atmosph\u00e4ren mit interplanetaren Raumsonden (Radiosounding of cometary and solar atmospheres using interplanetary spacecraft)\u201d<\/li>\n \t
    • June 1990 Ph.D. (Dr. rer.nat.) in Astronomy, 1990, Radioastronomisches Institut, Universit\u00e4t Bonn, Bonn, Federal Republic of Germany\nThesis: \u201cThe Dynamics of the Giotto Spacecraft in the Inner Dust Coma of Comet P\/Halley as Determined From the Giotto Radio-Science Experiment\u201d<\/li>\n \t
    • May 1986 Diploma in Physics, 1986, Radioastronomisches Institut, Universit\u00e4t Bonn, Bonn, Federal Republic of Germany\nThesis: \u201cDas mittlere koronale Magnetfeld: Eine Analyse mit Helios Faraday Rotations Daten (The Mean Coronal Magnetic Field: An Analysis using Helios Faraday Rotation Data).\u201d<\/li>\n \t
    • Oct. 1979 \u2013 June 1990 study of Physics and Astronomy, Oct 1979 – June 1990, Universit\u00e4t Bonn, Bonn, Federal Republic of Germany<\/li>\n<\/ul>\nPositions:<\/b><\/span>\n
        \n \t
      • since May 2010 Vice-Director of the Rheinische Institut f\u00fcr Umweltforschung an der Universit\u00e4t zu K\u00f6ln e.V., Cologne, Germany<\/li>\n \t
      • Since April 2007 Director of the Department Planetary Research at the Rheinisches Institut f\u00fcr Umweltforschung at the University Cologne, Cologne, Germany<\/li>\n \t
      • November 2008 position 3 on the list of candidates for the W3 professorship in Spacecraft Engineering at the Universit\u00e4t der Bundeswehr M\u00fcnchen (UniBw Munich)<\/li>\n \t
      • October 2003 \u2013 September 2005 acting C4 professor of Geophysics at the Institut f\u00fcr Geophysik und Meteorologie, Universit\u00e4t zu K\u00f6ln<\/li>\n \t
      • December 2002 position 2 on the list of candidates for the C3 professorship in Geophysics at the TU Braunschweig<\/li>\n \t
      • August 2001 \u2013 September 2001: Visiting Scientist at the Jet Propulsion Laboratory, Space Science Section, California Institute of Technology, Pasadena, California, USA<\/li>\n \t
      • April 1999 \u2013 March 2007 Hochschuldozent (University Lecturer), Institut f\u00fcr Geophysik und Meteorologie, Universit\u00e4t zu K\u00f6ln, K\u00f6ln, Germany\nHead of the Radio Science Group<\/li>\n \t
      • July 1997 – September 1997: Visiting Assistant Professor, Space Telecommunications  and Radio Science Laboratory (STARLab), Stanford University, Stanford, California, USA<\/li>\n \t
      • April 1997 \u2013 June 1997: Visiting Scientist at the Jet Propulsion Laboratory, Space Science Section, California Institute of Technology, Pasadena, California, USA<\/li>\n \t
      • Jan. 1993  – March 1999 Senior Research Scientist and \u201cWissenschaftlicher Assistent\u201d (Assistant Professor), Institut f\u00fcr Geophysik und Meteorologie, Universit\u00e4t zu K\u00f6ln (Cologne University), K\u00f6ln, Germany\nHead of the Radio Science and Georadar Group<\/li>\n \t
      • 1991 – 1992  Research Associate, Institut f\u00fcr Hochfrequenztechnik (Institute for High Frequency Technology), Deutsche Forschungsanstalt f\u00fcr Luft und Raumfahrt (DLR), (German Research Establishment for Air and Spaceflight), Oberpfaffenhofen, Germany<\/li>\n \t
      • July 1990 \u2013 Dec. 1990: Research Associate, Institut f\u00fcr Hoch- und H\u00f6chstfrequenztechnik, Ruhr-Universit\u00e4t Bochum, Bochum, Germany  position was located at the Radioastronomisches Institut Universit\u00e4t Bonn, Bonn, Germany<\/li>\n \t
      • 1987 \u2013 June 1990: Research Associate, Radioastronomisches Institut, Universit\u00e4t Bonn, Bonn, Federal Republic of Germany\n<\/b><\/li>\n<\/ul>\nESA and NASA Space Missions:<\/b><\/span>\n
          \n \t
        • Since 2014 Instrument Co-I on the radio science experiment REX for NASA\u00b4s New Horizons mission to Pluto<\/li>\n \t
        • Since 2013 Co-I on the 3GM experiment for the  ESA Jupiter JUICE mission<\/li>\n \t
        • Since 2010 Instrument Lead on the radio science experiment for the NASA Discovery proposal \u201cLucy\u201d led by C. Olkin, SwRI, CO, USA<\/li>\n \t
        • Since 2009 Instrument contact for the ESA mission studies \u201cEJSM Laplace\u201d and \u201cMarco Polo\u201d<\/li>\n \t
        • 2008 Co-I on the PRARE-L experiment for the national Moon orbiter LEO\nsince 2007 Corot operations for the search of extrasolar planets<\/li>\n \t
        • 2006-2008 Co-I on the radio science experiment for the Discovery proposal  \u201cThe Great Escape\u201d led by J. Burch<\/li>\n \t
        • 2005-2006 member of the ESA study team: Don Quijote<\/li>\n \t
        • Since 2005 mission and experiment operations in orbit with Venus Express<\/li>\n \t
        • Since 2004 mission and experiment operations in orbit with Mars Express and Rosetta<\/li>\n \t
        • 2002 member of the ESA study teams:\n
            \n \t
          • ISHTAR, asteroid orbiter (study lead Univ. Paris and Astrium)<\/li>\n \t
          • SIMONE, asteroid flybys (study lead Open University and Qinetiq)<\/li>\n \t
          •  APIES, satellite swarm to the asteroid belt (study lead Univ. Paris and Astrium)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n
              \n \t
            • Since May 2001 Co-PI of the radio science experiment VeRa of the Venus Express proposal study.<\/li>\n \t
            • Since January 2001 COROT Co-Investigator in cooperation with the German Lead-Co-I Dr. Heike Rauer (DLR Berlin-Adlershof): \u201cGravity and MHD-interactions of the central star and its planets (stellar-planetary relationship)\u201d; COROT is a french space telescope for the search for extrasolar planets; launch was in December 2006<\/li>\n \t
            • Since January 2001 Collaborator of the radio science experiment REX on the Pluto-Kuiper Belt Proposal \u201cNew Horizon\u201d (PI A.S. Stern, SwRI Boulder).<\/li>\n \t
            • 2000 Science Team Member of the F-Mission study MASTER, proposal study presented to ESA<\/li>\n \t
            • 2000 Co-Investigator \u201cPluto Kuiper Express Radio Science\u201d, Proposal submitted to NASA (proposal PI G.L. Tyler, Stanford University)<\/li>\n \t
            • since Feb. 1998 Principal Investigator \u201cMars Express Orbiter Radio Science\u201d, Mars Express Mission, selected by ESA\nCo-Investigator \u201cHigh Resolution Stereo Camera HRSC\u201d (PI G. Neukum, DLR Berlin) on Mars Express\nCo-Investigator \u201cNetlander NEIGE\u201d (PI J.-P. Barriot, CNES Toulouse)<\/li>\n \t
            • 1996-2004 Team Member \u201cRadio Science Experiment on Stardust\u201d (Mission Co-I J.D. Anderson, JPL)<\/li>\n \t
            • since Feb. 1996 Principal Investigator \u201cRosetta Radio Science Investigations (RSI)\u201d, International Rosetta Mission; selected by ESA<\/li>\n \t
            • 1993 – 1996 Team Member \u201cMars-96 High Resolution Stereo Camera-Surface Atmosphere interaction (HRSC-SAI)\u201d; appointment terminated due to loss of spacecraft<\/li>\n \t
            • since 1992 Team Member of the \u201cGalileo Radio Propagation Experiment-Solar Corona Experiment\u201d, appointed by NASA<\/li>\n \t
            • 1992 Co-Investigator \u201cGiotto Radio Science Experiment (GRE)\u201d at the P\/Grigg-Skjellerup Flyby; appointed by ESA<\/li>\n \t
            • since 1991 Co-Investigator \u201cUlysses Solar Corona Experiment (SCE)\u201d; appointed by ESA<\/li>\n<\/ul>\nPublications Dr. Martin P\u00e4tzold, 23.5.2014<\/b> <\/span>\n
                \n \t
              1. P\u00e4tzold, M. and H. Rauer, Where Are the Massive Close-in Extrasolar Planets?, Astrophys. J.<\/i>,568, L117-L120, doi:10.1086\/339794, 2002<\/li>\n \t
              2. P\u00e4tzold, M., L. Carone and H. Rauer, Tidal interactions of close-in extrasolar planets: The OGLE cases, Astron. & Astrophys.<\/i>, 427, 1075-1080, doi:10.1051\/0004-6361:20040258, 2004<\/li>\n \t
              3. P\u00e4tzold, M.; Tellmann, S.; H\u00e4usler, B.; Hinson, D.; Schaa, R.; Tyler, G. L., A\nSporadic Third Layer in the Ionosphere of Mars, Science, Volume 310, Issue\n5749, pp. 837-839, 2005.<\/li>\n \t
              4. P\u00e4tzold, M., B. H\u00e4usler, M.K. Bird, S. Tellmann, R. Mattei, S.W. Asmar, V.\nDehant, W. Eidel, T. Imamura, R.A. Simpson, G.L. Tyler, The structure of Venus middle atmosphere and ionosphere, Nature 450, 657, 2007.<\/li>\n \t
              5. P\u00e4tzold, M., S. Tellmann, B. H\u00e4usler, M.K. Bird, G.L. Tyler, A.A. Christou and P. Withers, A sporadic layer in the Venus lower ionosphere of meteoric origin,\nGeophys. Res. Vol. 35, doi: 10.1029\/2008GL035875, 2008.<\/li>\n \t
              6. P\u00e4tzold, M., T.P. Andert, B. H\u00e4usler, S. Tellmann, J.D. Anderson, S.W. Asmar, J.-P. Barriot, and M.K. Bird, Pre-Flyby estimates on the precision of the mass determination of Asteriod (21) Lutetia from Rosetta radio tracking, Astron. Astrophys. 518, L156, 2010.<\/li>\n \t
              7. P\u00e4tzold, M., T.P. Andert, S.W. Asmar, J.D. Anderson, J.-P. Barriot, M.K. Bird, B. H\u00e4usler, M. Hahn, S. Tellmann, H. Sierks, P. Lamy, B. Weiss, Asteroid (21)\nLutetia \u2013 low mass, high density, Science 334, 491, 2011.<\/li>\n \t
              8. P\u00e4tzold, M., M. Hahn, S. Tellmann, B. H\u00e4usler, M.K. Bird, G.L. Tyler, S.W.\nAsmar and B.T. Tsurutani, Coronal Density Structures and CMEs: Superior\nSolar Conjunctions of Mars Express, Venus Express and Rosetta: 2004, 2006, 2008, Solar Phys. 279, 127-152, 2012.<\/li>\n \t
              9. P\u00e4tzold, M., und 50 Co-Autoren, Transiting exoplanets from the CoRoT space mission. XXIII. CoRoT-21b: a doomed hot-Jupiter around a faint subgiant star, Astron. Astrophys. 545, A6, 2012.<\/li>\n \t
              10. P\u00e4tzold, M., T.P. Andert, G.L. Tyler, S.W. Asmar, B. H\u00e4usler, S. Tellmann, Phobos mass determination from the very close flby of Mars Express in 2010, Icarus 229, 92-98, 2014.<\/li>\n<\/ol>\n<\/details>","protected":false},"excerpt":{"rendered":"

                PD Dr. Martin P\u00e4tzold Position:Direktor der Abteilung Planetenforschung des Rheinischen Instituts f\u00fcr Umweltforschung (RIU-PF)Principal Investigator (PI) der Radio Science Experimente auf Mars Express (MaRS), Rosetta (RSI) und Co-PI des Radio Science Experimentes VeRa auf Venus Express.Tel.: +49 221 277 81 81-0<\/p>","protected":false},"author":1,"featured_media":0,"parent":15,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_uag_custom_page_level_css":"","site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"default","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","ast-disable-related-posts":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"footnotes":""},"class_list":["post-521","page","type-page","status-publish","hentry"],"yoast_head":"\nMartin - Radio Science<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/fip-koeln.de\/en_us\/team\/chef\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Martin - Radio Science\" \/>\n<meta property=\"og:description\" content=\"PD Dr. Martin P\u00e4tzold Position:Direktor der Abteilung Planetenforschung des Rheinischen Instituts f\u00fcr Umweltforschung (RIU-PF)Principal Investigator (PI) der Radio Science Experimente auf Mars Express (MaRS), Rosetta (RSI) und Co-PI des Radio Science Experimentes VeRa auf Venus Express.Tel.: +49 221 277 81 81-0\" \/>\n<meta property=\"og:url\" content=\"https:\/\/fip-koeln.de\/en_us\/team\/chef\/\" \/>\n<meta property=\"og:site_name\" content=\"Radio Science\" \/>\n<meta property=\"article:modified_time\" content=\"2023-11-10T10:15:25+00:00\" \/>\n<meta property=\"og:image\" content=\"https:\/\/fip-koeln.de\/wp-content\/uploads\/2023\/11\/PlaceholderPerson-240x300.webp\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Est. reading time\" \/>\n\t<meta name=\"twitter:data1\" content=\"7 minutes\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\"@context\":\"https:\\\/\\\/schema.org\",\"@graph\":[{\"@type\":\"WebPage\",\"@id\":\"https:\\\/\\\/fip-koeln.de\\\/team\\\/chef\\\/\",\"url\":\"https:\\\/\\\/fip-koeln.de\\\/team\\\/chef\\\/\",\"name\":\"Martin - 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