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WINTER 2013 - Volume 60, Number 4 the Air Force Historical Foundation Founded on May 27, 1953 by Gen Carl A
WINTER 2013 - Volume 60, Number 4 WWW.AFHISTORICALFOUNDATION.ORG The Air Force Historical Foundation Founded on May 27, 1953 by Gen Carl A. “Tooey” Spaatz MEMBERSHIP BENEFITS and other air power pioneers, the Air Force Historical All members receive our exciting and informative Foundation (AFHF) is a nonprofi t tax exempt organization. Air Power History Journal, either electronically or It is dedicated to the preservation, perpetuation and on paper, covering: all aspects of aerospace history appropriate publication of the history and traditions of American aviation, with emphasis on the U.S. Air Force, its • Chronicles the great campaigns and predecessor organizations, and the men and women whose the great leaders lives and dreams were devoted to fl ight. The Foundation • Eyewitness accounts and historical articles serves all components of the United States Air Force— Active, Reserve and Air National Guard. • In depth resources to museums and activities, to keep members connected to the latest and AFHF strives to make available to the public and greatest events. today’s government planners and decision makers information that is relevant and informative about Preserve the legacy, stay connected: all aspects of air and space power. By doing so, the • Membership helps preserve the legacy of current Foundation hopes to assure the nation profi ts from past and future US air force personnel. experiences as it helps keep the U.S. Air Force the most modern and effective military force in the world. • Provides reliable and accurate accounts of historical events. The Foundation’s four primary activities include a quarterly journal Air Power History, a book program, a • Establish connections between generations. -
The Beckman Center for the History of Chemistry
THE BECKMAN CENTER FOR THE HISTORY OF CHEMISTRY GERHARD HERZBERG Transcript of an Interview Conducted by M. Christine King at The National Research Council of Canada on 5 May 1986 This interview has been designated as Free Access. One may view, quote from, cite, or reproduce the oral history with the permission of CHF. Please note: Users citing this interview for purposes of publication are obliged under the terms of the Chemical Heritage Foundation Oral History Program to credit CHF using the format below: Gerhard Herzberg, interview by M. Christine King at The National Research Council of Canada, Ottawa, Canada, 5 May 1986 (Philadelphia: Chemical Heritage Foundation, Oral History Transcript # 0023). Chemical Heritage Foundation Oral History Program 315 Chestnut Street Philadelphia, Pennsylvania 19106 The Chemical Heritage Foundation (CHF) serves the community of the chemical and molecular sciences, and the wider public, by treasuring the past, educating the present, and inspiring the future. CHF maintains a world-class collection of materials that document the history and heritage of the chemical and molecular sciences, technologies, and industries; encourages research in CHF collections; and carries out a program of outreach and interpretation in order to advance an understanding of the role of the chemical and molecular sciences, technologies, and industries in shaping society. GERHARD HERZBERG 1904 Born in Hamburg, Germany on 25 December Education 1928 Dr. Ing., Darmstadt Technische Universität Professional Experience 1928-1929 Post-doctoral -
New 78 Covers
NATIONAL ACADEMY OF SCIENCES ROBERT SANDERSON MULLIKEN 1896–1986 A Biographical Memoir by R. STEPHEN BERRY Biographical Memoirs, VOLUME 78 PUBLISHED 2000 BY THE NATIONAL ACADEMY PRESS WASHINGTON, D.C. Photo credit: Photo by Harris & Ewing, Washington, D.C. ROBERT SANDERSON MULLIKEN June 7, 1896-October 31, 1986 BY R. STEPHEN BERRY OBERT S. MULLIKEN WAS a quiet, soft-spoken man, yet so R single-minded and determined in his devotion to under- standing molecules that he came to be called “Mr. Molecule.” If any single person’s ideas and teachings dominated the development of our understanding of molecular structure and spectra, it surely was Robert Mulliken. From the begin- ning of his career as an independent scientist in the mid- 1920s until he published his last scientific papers in the early 1980s, he guided an entire field through his penetrat- ing solutions of outstanding puzzles, his identification (or discovery) and analysis of the new major problems ripe for study, and his creation of a school—the Laboratory of Molecular Structure and Spectroscopy or LMSS at the University of Chicago, during its existence the most impor- tant center in the world for the study of molecules. Robert’s background led him naturally into academic sci- ence. He was born in Newburyport, Massachusetts, in a house built by his great-grandfather in about 1798. His father, Samuel Parsons Mulliken, was a professor of chemistry at MIT, which made him a daily commuter between Newburyport and Boston. Samuel Mulliken and his child- hood friend and later MIT colleague Arthur A. Noyes were 3 4 BIOGRAPHICAL MEMOIRS strong influences stirring Robert’s interests in science. -
Henry Taube Papers SC0731SC0731
http://oac.cdlib.org/findaid/ark:/13030/kt329035mg No online items Guide to the Henry Taube Papers SC0731SC0731 Stanford University Archives staff Department of Special Collections and University Archives October 2010 Green Library 557 Escondido Mall Stanford 94305-6064 [email protected] URL: http://library.stanford.edu/spc Note This encoded finding aid is compliant with Stanford EAD Best Practice Guidelines, Version 1.0. Guide to the Henry Taube Papers SC073117755 1 SC0731SC0731 Language of Material: English Contributing Institution: Department of Special Collections and University Archives Title: Henry Taube papers Creator: Taube, Henry Identifier/Call Number: SC0731 Identifier/Call Number: 17755 Physical Description: 65.25 Linear Feet(56 boxes) Date (inclusive): 1941-2003 Abstract: Collection pertains to his teaching and research, primarily while at Stanford University, and includes grant files, articles and papers, reprints, class files, correspondence, travel records, and biographical materials. Information about Access This collection is open for research; materials must be requested at least 48 hours in advance of intended use. Ownership & Copyright All requests to reproduce, publish, quote from, or otherwise use collection materials must be submitted in writing to the Head of Special Collections and University Archives, Stanford University Libraries, Stanford, California 94304-6064. Consent is given on behalf of Special Collections as the owner of the physical items and is not intended to include or imply permission from the copyright owner. Such permission must be obtained from the copyright owner, heir(s) or assigns. See: http://library.stanford.edu/depts/spc/pubserv/permissions.html. Restrictions also apply to digital representations of the original materials. -
Messenger Extreme Exploration
MESSENGERMESSENGER EEXTREMEXTREME EEXPLORATIONXPLORATION — Deborah Domingue, MESSENGER Deputy Project Scientist, Johns Hopkins University Applied Physics Laboratory The first half of 2004 has been an exciting time for planetary exploration with the successful encounter and sampling of Comet Wild 2 by Stardust, the landing of two Mars rovers, orbital operations at Mars by three spacecraft, and the arrival of Cassini at Saturn. This month we wished “Bon Voyage” to the MESSENGER spacecraft, which successfully launched from Cape Canaveral on August 3, 2004, and began its journey to the innermost planet of our solar system, Mercury. MESSENGER is a MEcury Surface, Space ENvironment, GEochemistry, and Ranging mission that will orbit Mercury for one Earth year (beginning in March 2011) following three flybys (in January and Septem- ber 2008 and October 2009) of the planet. It will be our first return to Mercury in over 30 years! The Mariner 10 spacecraft flew past Mer- cury three times in 1974 and 1975 and collected information on less than half the planet. MESSENGER will provide the first global map of Mercury, in addition to detailed information on the composition and structure of Mercury’s crust, its geologic history, the nature of Mercury’s thin exosphere and dynamic magnetosphere, and the makeup of its core and polar materials. MERCURY:A PLACE OF EXTREMES Mercury, the planet closest to the Sun, has a highly elliptical orbit such that its distance from the Sun ranges from 46 million kilometers (29 million miles) to 70 million kilometers (43 million miles). Because of its slow rotation, Mercury’s day (sunrise to sunrise) actually lasts two Mercury years (88 Earth days of dark and 88 Earth days of daylight). -
Copyright by Paul Harold Rubinson 2008
Copyright by Paul Harold Rubinson 2008 The Dissertation Committee for Paul Harold Rubinson certifies that this is the approved version of the following dissertation: Containing Science: The U.S. National Security State and Scientists’ Challenge to Nuclear Weapons during the Cold War Committee: —————————————————— Mark A. Lawrence, Supervisor —————————————————— Francis J. Gavin —————————————————— Bruce J. Hunt —————————————————— David M. Oshinsky —————————————————— Michael B. Stoff Containing Science: The U.S. National Security State and Scientists’ Challenge to Nuclear Weapons during the Cold War by Paul Harold Rubinson, B.A.; M.A. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2008 Acknowledgements Thanks first and foremost to Mark Lawrence for his guidance, support, and enthusiasm throughout this project. It would be impossible to overstate how essential his insight and mentoring have been to this dissertation and my career in general. Just as important has been his camaraderie, which made the researching and writing of this dissertation infinitely more rewarding. Thanks as well to Bruce Hunt for his support. Especially helpful was his incisive feedback, which both encouraged me to think through my ideas more thoroughly, and reined me in when my writing overshot my argument. I offer my sincerest gratitude to the Smith Richardson Foundation and Yale University International Security Studies for the Predoctoral Fellowship that allowed me to do the bulk of the writing of this dissertation. Thanks also to the Brady-Johnson Program in Grand Strategy at Yale University, and John Gaddis and the incomparable Ann Carter-Drier at ISS. -
A Brief History of Magnetospheric Physics Before the Spaceflight Era
A BRIEF HISTORY OF MAGNETOSPHERIC PHYSICS BEFORE THE SPACEFLIGHT ERA David P. Stern Laboratoryfor ExtraterrestrialPhysics NASAGoddard Space Flight Center Greenbelt,Maryland Abstract.This review traces early resea/ch on the Earth's aurora, plasma cloud particles required some way of magneticenvironment, covering the period when only penetratingthe "Chapman-Ferrarocavity": Alfv•n (1939) ground:based0bservationswerepossible. Observations of invoked an eleCtric field, but his ideas met resistance. The magneticstorms (1724) and of perturbationsassociated picture grew more complicated with observationsof with the aurora (1741) suggestedthat those phenomena comets(1943, 1951) which suggesteda fast "solarwind" originatedoutside the Earth; correlationof the solarcycle emanatingfrom the Sun's coronaat all times. This flow (1851)with magnetic activity (1852) pointed to theSun's was explainedby Parker's theory (1958), and the perma- involvement.The discovei-yof •solarflares (1859) and nent cavity which it producedaround the Earth was later growingevidence for their associationwith large storms named the "magnetosphere"(1959). As early as 1905, led Birkeland (1900) to proposesolar electronstreams as Birkeland had proposedthat the large magneticperturba- thecause. Though laboratory experiments provided some tions of the polar aurora refleCteda "polar" type of support;the idea ran into theoreticaldifficulties and was magneticstorm whose electric currents descended into the replacedby Chapmanand Ferraro's notion of solarplasma upper atmosphere;that idea, however, was resisted for clouds (1930). Magnetic storms were first attributed more than 50 years. By the time of the International (1911)to a "ringcurrent" of high-energyparticles circling GeophysicalYear (1957-1958), when the first artificial the Earth, but later work (1957) reCOgnizedthat low- satelliteswere launched, most of the importantfeatures of energy particlesundergoing guiding center drifts could the magnetospherehad been glimpsed, but detailed have the same effect. -
The CCNY Physics Department Newsletter Volume 12 Fall 2019 - Spring 2021
CCNY PHYSICS The CCNY Physics Department Newsletter Volume 12 Fall 2019 - Spring 2021 Features CCNY Physics Club Wins Awards Quantum Computing and CCNY Physics Planetariums in a Pandemic 2 CCNY Physics Department Newsletter Welcome to the 2019-2021 CCNY Physics Department Newsletter. It has been quite a year, but our department has re- mained strong and devoted to both our students and our research programs. We’ve had a newsletter for a number of years, but this year we decided to spruce it up a bit and give all these hardworking faculty, staff, and students a nice record of the past year’s accom- plishements. Going foward, we will be releasing the newsletter in the fall of each year. So, enjoy this issue, and look forward to another in a few months. PHYSICS CLUB REMAINS VIBRANT, WINS AWARDS The CCNY Physics Club bustles with activity whether students are meeting face-to-face on campus, or associat- ing virtually abiding COVID-19 guidelines, and garners awards for their exemplary education and outreach activi- ties. First, the awards! Awards The 2020 Physics Club Execitives: Prof. Franco (Advisor), Michael Gaziani, Jireh Garcia, The Physics Club has recently garnered two major Lisa Chan, Matthew Kubikowski national awards. The Club, a chapter of the Society of is lauded for its vigorous STEM outreach program for un- Physics Students (SPS) received an Outstanding Chap- derprivileged elementary and middle school students. The ter Award from the SPS National Office for 2020. The Chapter runs this outreach program in partnership with designation, given to fewer than 15 percent of all SPS inner city schools and community groups, such as, Ham- chapters at colleges and universities in the United States ilton Grange Middle School, PS 325 Elementary School, and internationally, recognizes the CCNY chapter’s suc- America Scores, the New York Math Academy, the Bridge cessful “Physics Month” activities between October and Golf Foundation and the Eagle Academy of Harlem. -
Robert Mulliken
NATIONAL ACADEMY OF SCIENCES ROBERT SANDERSON MULLIKEN 1896–1986 A Biographical Memoir by R. STEPHEN BERRY Biographical Memoirs, VOLUME 78 PUBLISHED 2000 BY THE NATIONAL ACADEMY PRESS WASHINGTON, D.C. Photo credit: Photo by Harris & Ewing, Washington, D.C. ROBERT SANDERSON MULLIKEN June 7, 1896-October 31, 1986 BY R. STEPHEN BERRY OBERT S. MULLIKEN WAS a quiet, soft-spoken man, yet so R single-minded and determined in his devotion to under- standing molecules that he came to be called “Mr. Molecule.” If any single person’s ideas and teachings dominated the development of our understanding of molecular structure and spectra, it surely was Robert Mulliken. From the begin- ning of his career as an independent scientist in the mid- 1920s until he published his last scientific papers in the early 1980s, he guided an entire field through his penetrat- ing solutions of outstanding puzzles, his identification (or discovery) and analysis of the new major problems ripe for study, and his creation of a school—the Laboratory of Molecular Structure and Spectroscopy or LMSS at the University of Chicago, during its existence the most impor- tant center in the world for the study of molecules. Robert’s background led him naturally into academic sci- ence. He was born in Newburyport, Massachusetts, in a house built by his great-grandfather in about 1798. His father, Samuel Parsons Mulliken, was a professor of chemistry at MIT, which made him a daily commuter between Newburyport and Boston. Samuel Mulliken and his child- hood friend and later MIT colleague Arthur A. Noyes were 3 4 BIOGRAPHICAL MEMOIRS strong influences stirring Robert’s interests in science. -
Lecture 17: the Solar Wind O Topics to Be Covered
Lecture 17: The solar wind o Topics to be covered: o Solar wind o Inteplanetary magnetic field The solar wind o Biermann (1951) noticed that many comets showed excess ionization and abrupt changes in the outflow of material in their tails - is this due to a solar wind? o Assumed comet orbit perpendicular to line-of-sight (vperp) and tail at angle ! => tan! = vperp/vr o From observations, tan ! ~ 0.074 o But vperp is a projection of vorbit -1 => vperp = vorbit sin ! ~ 33 km s -1 o From 600 comets, vr ~ 450 km s . o See Uni. New Hampshire course (Physics 954) for further details: http://www-ssg.sr.unh.edu/Physics954/Syllabus.html The solar wind o STEREO satellite image sequences of comet tail buffeting and disconnection. Parker’s solar wind o Parker (1958) assumed that the outflow from the Sun is steady, spherically symmetric and isothermal. o As PSun>>PISM => must drive a flow. o Chapman (1957) considered corona to be in hydrostatic equibrium: dP = −ρg dr dP GMS ρ + 2 = 0 Eqn. 1 dr r o If first term >> than second €=> produces an outflow: € dP GM ρ dv + S + ρ = 0 Eqn. 2 dr r2 dt o This is the equation for a steadily expanding solar/stellar wind. € Parker’s solar wind (cont.) dv dv dr dv dP GM ρ dv o As, = = v => + S + ρv = 0 dt dr dt dr dr r2 dr dv 1 dP GM or v + + S = 0 Eqn. 3 dr ρ dr r2 € € o Called the momentum equation. € o Eqn. 3 describes acceleration (1st term) of the gas due to a pressure gradient (2nd term) and gravity (3rd term). -
Reversed out (White) Reversed
Berkeley rev.( white) Berkeley rev.( FALL 2014 reversed out (white) reversed IN THIS ISSUE Berkeley’s Space Sciences Laboratory Tabletop Physics Bringing More Women into Physics ALUMNI NEWS AND MORE! Cover: The MAVEN satellite mission uses instrumentation developed at UC Berkeley's Space Sciences Laboratory to explore the physics behind the loss of the Martian atmosphere. It’s a continuation of Berkeley astrophysicist Robert Lin’s pioneering work in solar physics. See p 7. photo credit: Lockheed Martin Physics at Berkeley 2014 Published annually by the Department of Physics Steven Boggs: Chair Anil More: Director of Administration Maria Hjelm: Director of Development, College of Letters and Science Devi Mathieu: Editor, Principal Writer Meg Coughlin: Design Additional assistance provided by Sarah Wittmer, Sylvie Mehner and Susan Houghton Department of Physics 366 LeConte Hall #7300 University of California, Berkeley Berkeley, CA 94720-7300 Copyright 2014 by The Regents of the University of California FEATURES 4 12 18 Berkeley’s Space Tabletop Physics Bringing More Women Sciences Laboratory BERKELEY THEORISTS INVENT into Physics NEW WAYS TO SEARCH FOR GOING ON SIX DECADES UC BERKELEY HOSTS THE 2014 NEW PHYSICS OF EDUCATION AND SPACE WEST COAST CONFERENCE EXPLORATION Berkeley theoretical physicists Ashvin FOR UNDERGRADUATE WOMEN Vishwanath and Surjeet Rajendran IN PHYSICS Since the Space Lab’s inception are developing new, small-scale in 1959, Berkeley physicists have Women physics students from low-energy approaches to questions played important roles in many California, Oregon, Washington, usually associated with large-scale of the nation’s space-based scientific Alaska, and Hawaii gathered on high-energy particle experiments. -
Henry Taube by J
Chemical Education Today Nobel Centennial Essays A Century of Chemical Dynamics Traced through the Nobel Prizes W 1983: Henry Taube by J. Van Houten Nobel Prize in Chemistry 1983 Photo by Rudy Baum Henry Taube (1915– ) for his work on the mechanisms of electron transfer Henry Taube, shown on reactions, especially in metal complexes the cover of C&E News. This is the eighth in a series of essays (1) written in com- Reprinted with permis- memoration of the centennial of the Nobel Prize, examin- sion from Chemical & ing the history of chemical dynamics in the 20th century.W Engineering News, May 21, 1984. © As his Nobel citation (2) states, Henry Taube studied elec- Copyright 1984 Ameri- tron transfer reactions of transition metal complexes. The can Chemical Society. Nobel Prize to Taube came exactly seventy years after it was awarded to Alfred Werner (3) for developing the structural chemistry of inorganic transition metal complexes. During the entire 20th century, Taube and Werner are the only in- to Werner’s. His early mechanistic studies relied heavily on organic transition metal chemists to win a Nobel Prize.1 In isotope tracer techniques developed by George de Hevesy, the fact, many of the complexes that Taube studied were first 1943 Nobel Laureate (1d). The second of the 100 references prepared or characterized by Werner. in Taube’s Nobel lecture (6) is to a 1920 paper where de Taube’s citation (2) concludes with the statement: “There Hevesy used naturally occurring lead isotopes to follow the is no doubt that Henry Taube is one of the most creative exchange reaction between Pb2+ and Pb4+ (7).