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LEADER 00000cam a2200589Ka 4500 
001    ocn843882980 
003    OCoLC 
005    20160527040629.6 
006    m     o  d         
007    cr cnu---unuuu 
008    130521s1997    si a    ob    001 0 eng d 
020    9789812830258|q(electronic book) 
020    9812830251|q(electronic book) 
020    |z9810226322 
020    |z9789810226329 
035    (OCoLC)843882980 
040    N$T|beng|epn|cN$T|dE7B|dI9W|dOCLCF|dYDXCP|dOCLCQ 
049    RIDW 
050  4 QB721|b.K74 1997eb 
072  7 SCI|x004000|2bisacsh 
082 04 523.6|222 
084    US 8800|2rvk 
090    QB721|b.K74 1997eb 
100 1  Krishna Swamy, K. S.|0https://id.loc.gov/authorities/names
       /n85119519 
245 10 Physics of comets /|cK.S. Krishna Swamy. 
250    2nd ed. 
264  1 Singapore ;|aRiver Edge, N.J. :|bWorld Scientific,|c[1997]
264  4 |c©1997 
300    1 online resource (xiii, 380 pages) :|billustrations. 
336    text|btxt|2rdacontent 
337    computer|bc|2rdamedia 
338    online resource|bcr|2rdacarrier 
340    |gpolychrome|2rdacc 
347    text file|2rdaft 
490 1  World Scientific series in astronomy and astrophysics ;
       |vv. 2 
504    Includes bibliographical references and index. 
505 0  1. General introduction. 1.1. Historical perspective. 1.2.
       Encounter with comet Halley. 1.3. Discovery. 1.4. 
       Appearance. 1.5. Statistics. 1.6. Importance. 1.7. 
       Brightness. 1.8. Main characteristics. 1.9. An overall 
       view -- 2. Dynamics. 2.1. Orbital elements. 2.2. Orbit in 
       space -- 3. Physical aspects. 3.1. Black body radiation. 
       3.2. Perfect gas law. 3.3. Dissociative equilibrium. 3.4. 
       Doppler shift. 3.5. Spectroscopy. 3.6. Isotope effect. 
       3.7. Franck-Condon factors. 3.8. Intensity of emitted 
       lines. 3.9. Boltzmann distribution. 3.10. [symbol]-
       doubling. 3.11. Solar radiation. 3.12. Solar wind -- 4. 
       Spectra. 4.1. Main characteristics. 4.2. Forbidden 
       transitions. 4.3. Line-to-continuum ratio -- 5. Spectra of
       coma. 5.1. Fluorescence process. 5.2. Excitation 
       temperature. 5.3. Abundances of heavy elements. 5.4. 
       Isotopic abundances -- 6. Gas-production rates in coma. 
       6.1. Theoretical models. 6.2. Results. 6.3. Analysis of 
       hydrogen observations. 6.4. Gas-phase chemistry in the 
       coma. 6.5. Temperature and velocities of the coma gas. 
       6.6. Parent molecules. 6.7. Summary -- 7. Dust tail. 7.1. 
       Dynamics. 7.2. Anti-tail. 7.3. Dust features. 7.4. Icy-
       halo -- 8. Light scattering theory. 8.1. Mie scattering 
       theory. 8.2. Approximate expressions. 8.3. Computation of 
       cross sections. 8.4. Results. 8.5. Particles of other 
       types. 8.6. Optical constants -- 9. The nature of dust 
       particles. 9.1. Visible continuum. 9.2. Polarization. 9.3.
       Infrared measurements. 9.4. Spectral features. 9.5. 
       Properties derived from in situ measurements. 9.6. Albedo 
       of the particles. 9.7. Continuum emission in the radio 
       region. 9.8. Radiation-pressure effects. 9.9. Summary -- 
       10. Ion tails. 10.1. Evidence for the solar wind. 10.2. 
       Dynamical aberration. 10.3. Theoretical considerations. 
       10.4. Instabilities and waves. 10.5. Acceleration of 
       cometary ions. 10.6. Large scale structures -- 11. 
       Nucleus. 11.1. Theory of vaporization. 11.2. Outbursts. 
       11.3. Albedo and radius. 11.4. Rotation. 11.5. Density. 
       11.6. Chemical composition. 11.7. Mass loss. 11.8. 
       Structure. 11.9. Non-gravitational forces -- 12. Origin. 
       12.1. Evidence for the oort cloud. 12.2. Evolution and 
       properties of oort cloud. 12.3. Origin of the oort cloud -
       - 13. Relation to other solar system. 13.1. Asteroids. 
       13.2. Meteorites. 13.3. Meteor streams. 13.4. Particles 
       collected at high altitudes. 13.5. Primordial material. 
       13.6. Chemical evolution. 13.7. Overview -- 14. Problems 
       and prospects. 14.1. Epilogue. 14.2. Future studies. 14.3.
       Postscript. 
520    The study of Comet Halley in 1986 was a tremendous success
       for cometary science. In March of that year, six 
       spacecrafts passed through Comet Halley as close as 600 km
       from the nucleus and made the in situ measurements of 
       various kinds. These space missions to Comet Halley and 
       that of the ICE spacecraft to Comet Giacobini-Zinner 
       combined with studies, both ground-based and above the 
       atmosphere, have increased our knowledge of cometary 
       science in a dramatic way. This new edition of Physics of 
       Comets incorporates these new and exciting findings. The 
       emphasis of the book is on the physical processes 
       operating in a cometary environment. It discusses up-to-
       date observations, methods and results based on the study 
       of various comets. The subject is developed in a 
       systematic manner covering various aspects of cometary 
       phenomena. This book may serve as a text book for students,
       and as reference material for researchers. 
588 0  Print version record. 
590    eBooks on EBSCOhost|bEBSCO eBook Subscription Academic 
       Collection - North America 
650  0 Comets.|0https://id.loc.gov/authorities/subjects/
       sh85028854 
650  7 Comets.|2fast|0https://id.worldcat.org/fast/869108 
655  4 Electronic books. 
776 08 |iPrint version:|aKrishna Swamy, K.S.|tPhysics of comets.
       |b2nd ed.|dSingapore ; River Edge, N.J. : World Scientific,
       ©1997|z9810226322|w(DLC)   97007970|w(OCoLC)36477071 
830  0 World Scientific series in astronomy and astrophysics ;
       |0https://id.loc.gov/authorities/names/n95092807|vv. 2. 
856 40 |uhttps://rider.idm.oclc.org/login?url=http://
       search.ebscohost.com/login.aspx?direct=true&scope=site&
       db=nlebk&AN=564465|zOnline eBook. Access restricted to 
       current Rider University students, faculty, and staff. 
856 42 |3Instructions for reading/downloading this eBook|uhttp://
       guides.rider.edu/ebooks/ebsco 
901    MARCIVE 20231220 
948    |d20160607|cEBSCO|tebscoebooksacademic|lridw 
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