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Journal articles on the topic 'Giacobini-Zinner comet'

Author: Grafiati

Published: 4 June 2021

Last updated: 29 July 2025

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1

Cochran, Anita L., and Edwin S. Barker. "Comet Giacobini-Zinner - A normal comet?" Astronomical Journal 93 (January 1987): 239. http://dx.doi.org/10.1086/114304.

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2

BAME, S. J., R. C. ANDERSON, J. R. ASBRIDGE, et al. "Comet Giacobini-Zinner: Plasma Description." Science 232, no. 4748 (1986): 356–61. http://dx.doi.org/10.1126/science.232.4748.356.

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3

Shinnaka, Yoshiharu, Hideyo Kawakita, Hitomi Kobayashi, Reiko Furusho, and Jun-ichi Watanabe. "Optical Imaging Polarimetry of Comet 21P/Giacobini–Zinner during Its 2018 Apparition." Planetary Science Journal 4, no. 7 (2023): 125. http://dx.doi.org/10.3847/psj/acdf49.

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Abstract We conducted polarimetric observations of comet 21P/Giacobini–Zinner in the optical wavelength region using the polarimetric imager PICO equipped with the 50 cm telescope for Public Outreach at the Mitaka Campus of the National Astronomical Observatory of Japan on UT 2018 September 16, at a solar phase angle of 77° for the comet. We used Gunn’s i′-band filter to cover the wavelength region where sunlight reflected by dust grains dominates cometary spectra. The intensity map of comet 21P/Giacobini–Zinner showed an elongated coma structure along the east–west direction. The linear polar

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4

Fedder, Joel A., John G. Lyon, and John L. Guiliani. "Numerical simulations of comets: Predictions for comet Giacobini-Zinner." Eos, Transactions American Geophysical Union 67, no. 2 (1986): 17. http://dx.doi.org/10.1029/eo067i002p00017-01.

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5

Boice, D. C., W. F. Huebner, J. J. Keady, H. U. Schmidt, and R. Wegmann. "A model of comet P/Giacobini-Zinner." Geophysical Research Letters 13, no. 4 (1986): 381–84. http://dx.doi.org/10.1029/gl013i004p00381.

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6

Tsurutani, Bruce T., Richard M. Thorne, Edward J. Smith, J. T. Gosling, and Hiroshi Matsumoto. "Steepened magnetosonic waves at comet Giacobini-Zinner." Journal of Geophysical Research 92, A10 (1987): 11074. http://dx.doi.org/10.1029/ja092ia10p11074.

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7

Ogilvie, Keith W. "The plasma regime at comet Giacobini-Zinner." Advances in Space Research 5, no. 12 (1985): 27–35. http://dx.doi.org/10.1016/0273-1177(85)90064-x.

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8

Meyer-Vernet, N. "Comet Giacobini-Zinner diagnosis from radio measurements." Advances in Space Research 5, no. 12 (1985): 37–46. http://dx.doi.org/10.1016/0273-1177(85)90065-1.

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9

SCARF, F. L., F. V. CORONITI, C. F. KENNEL, D. A. GURNETT, W. H. IP, and E. J. SMITH. "Plasma Wave Observations at Comet Giacobini-Zinner." Science 232, no. 4748 (1986): 377–81. http://dx.doi.org/10.1126/science.232.4748.377.

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10

Tsurutani, Bruce T., and Edward J. Smith. "Strong hydromagnetic turbulence associated with comet Giacobini-Zinner." Geophysical Research Letters 13, no. 3 (1986): 259–62. http://dx.doi.org/10.1029/gl013i003p00259.

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11

Tsurutani, Bruce T., Edward J. Smith, Hiroshi Matsumoto, Armando L. Brinca, and Nojan Omidi. "Highly nonlinear magnetic pulses at comet Giacobini-Zinner." Geophysical Research Letters 17, no. 6 (1990): 757–60. http://dx.doi.org/10.1029/gl017i006p00757.

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12

Gary, S. Peter, and Dan Winske. "Linearly polarized magnetic fluctuations at comet Giacobini-Zinner." Journal of Geophysical Research 91, A12 (1986): 13699. http://dx.doi.org/10.1029/ja091ia12p13699.

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13

Tan, L. C., G. M. Mason, G. Gloeckler, F. M. Ipavich, and A. B. Galvin. "Energetic heavy ions observed near comet Giacobini-Zinner." Journal of Geophysical Research 95, A12 (1990): 20685. http://dx.doi.org/10.1029/ja095ia12p20685.

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14

Schleicher, D. G. "Spectrophotometric Spatial Mapping of Comet p/ Giacobini-Zinner." Publications of the Astronomical Society of the Pacific 97 (October 1985): 903. http://dx.doi.org/10.1086/131697.

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15

Hynds, R. J., S. W. H. Cowley, I. G. Richardson, et al. "Energetic ion observations during comet Giacobini-Zinner encounter." Advances in Space Research 5, no. 12 (1985): 17–25. http://dx.doi.org/10.1016/0273-1177(85)90063-8.

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16

Scarf, F. L. "Characteristics of the tail of comet Giacobini-Zinner." Advances in Space Research 6, no. 1 (1986): 329–36. http://dx.doi.org/10.1016/0273-1177(86)90048-7.

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17

Konno, I., and S. Wyckoff. "Atomic and molecular abundances in comet Giacobini-Zinner." Advances in Space Research 9, no. 3 (1989): 163–68. http://dx.doi.org/10.1016/0273-1177(89)90256-1.

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18

HYNDS, R. J., S. W. H. COWLEY, T. R. SANDERSON, K. P. WENZEL, and J. J. VAN ROOIJEN. "Observations of Energetic Ions from Comet Giacobini-Zinner." Science 232, no. 4748 (1986): 361–65. http://dx.doi.org/10.1126/science.232.4748.361.

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19

Ogilvie, K. W., M. A. Coplan, and L. A. McFadden. "Sodium near the Tail of Comet Giacobini–Zinner." Icarus 134, no. 2 (1998): 249–52. http://dx.doi.org/10.1006/icar.1998.5953.

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20

Królikowska, M., G. Sitarski, and S. Szutowicz. "Models of comets with strongly variable nongravitational effects." International Astronomical Union Colloquium 173 (1999): 381–87. http://dx.doi.org/10.1017/s0252921100031705.

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AbstractThe nongravitational motion of five “erratic” short-period comets is studied on the basis of published astrometric observations. We present the precession models which successfully link all the observed apparitions of the comets: 21P/Giacobini-Zinner, 31P/Schwassmann-Wachmann 2, 32P/Comas Solá, 37P/Forbes, and 43P/Wolf-Harrington. We used the Sekanina's forced precession model of the rotating cometary nucleus to include the nongravitational terms into equations of the comet's motion. Values of six basic parameters (four connected with the rotating comet nucleus and two describing the p

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21

Norris, R. P., J. R. Forster, and R. A. Duncan. "Detection of OH Maser Emission from Cornet Giacobini-Zinner." Publications of the Astronomical Society of Australia 6, no. 2 (1985): 180–81. http://dx.doi.org/10.1017/s132335800001804x.

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AbstractWe have detected OH maser radiation from the comet Giacobini-Zinner using the Parkes radio telescope. The emission was detected in two transitions of the ground state of OH, at an intensity consistent with the predicted OH molecular production rate. We also searched unsuccessfully for OH emission from comet Halley, from which we are able to place a significant upper limit on the intensity of OH emission.

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22

Huebner, W. F., D. C. Boice, H. U. Schmidt, and R. Wegmann. "Structure of the Coma: Chemistry and Solar Wind Interaction." International Astronomical Union Colloquium 116, no. 2 (1991): 907–36. http://dx.doi.org/10.1017/s025292110001277x.

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Much has been learned about the physics and chemistry of comets from the successful spacecraft encounters and intensive remote observing programs of Comets Halley and Giacobini-Zinner. Instead of being the panacea for our comet curiosity, these tantalizing “snapshots” have raised new questions, and many fundamental problems remain unsolved. To reap fuller benefits, extensive modeling is necessary to characterize the physical structure and chemical properties of the coma and to infer the composition and structure of the nucleus.

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23

Buti, B. "Chaotic Alfvén Waves in Solar and Cometary Plasmas: Summary." Symposium - International Astronomical Union 152 (1992): 297–98. http://dx.doi.org/10.1017/s0074180900091300.

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The recent observations, of energetic heavy ions in the vicinity of Comet Halley and Comet Giacobini-Zinner, are rather intriguing. Moreover the solar coronal heating is still not well understood and is somewhat puzzling. Since both these observations can not be properly explained by means of classical processes, we have to invoke anomalous heating and acceleration effects due to chaotic and turbulent plasma processes.

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24

Thomsen, M. F., S. J. Bame, W. C. Feldman, J. T. Gosling, D. J. McComas, and D. T. Young. "The comet/solar wind transition region at Giacobini-Zinner." Geophysical Research Letters 13, no. 4 (1986): 393–96. http://dx.doi.org/10.1029/gl013i004p00393.

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25

Telesco, C. M., R. Decher, C. Baugher, et al. "Thermal-infrared and visual imaging of comet Giacobini-Zinner." Astrophysical Journal 310 (November 1986): L61. http://dx.doi.org/10.1086/184782.

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26

von Rosenvinge, Tycho T., and John C. Brandt. "The International Cometary Explorer Mission to comet Giacobini-Zinner." Eos, Transactions American Geophysical Union 66, no. 36 (1985): 625. http://dx.doi.org/10.1029/eo066i036p00625.

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27

Tan, L. C., G. M. Mason, and B. T. Tsurutani. "Evidence for proton cyclotron waves near comet Giacobini-Zinner." Geophysical Research Letters 20, no. 3 (1993): 169–72. http://dx.doi.org/10.1029/93gl00069.

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28

Wallis, Max K., Nigel P. Meredith, and David Rees. "Gas coma of comet Giacobini-Zinner: Emission from grains." Advances in Space Research 9, no. 3 (1989): 213–16. http://dx.doi.org/10.1016/0273-1177(89)90262-7.

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29

VON ROSENVINGE, T. T., J. C. BRANDT, and R. W. FARQUHAR. "The International Cometary Explorer Mission to Comet Giacobini-Zinner." Science 232, no. 4748 (1986): 353–56. http://dx.doi.org/10.1126/science.232.4748.353.

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30

Chornaya, Ekaterina, Evgenij Zubko, Igor Luk'yanyk, et al. "Imaging polarimetry and photometry of comet 21P/Giacobini-Zinner." Icarus 337 (February 2020): 113471. http://dx.doi.org/10.1016/j.icarus.2019.113471.

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31

Schleicher, David G. "Comet 21P/Giacobini–Zinner: Narrowband Photometry of the Prototype of Carbon-chain Depleted Comets at Multiple Apparitions." Planetary Science Journal 3, no. 6 (2022): 143. http://dx.doi.org/10.3847/psj/ac6de2.

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Abstract We obtained extensive narrowband photoelectric photometry of Comet 21P/Giacobini–Zinner with observations spanning 33 yr. The original data from 1985 were re-reduced and are presented along with data from three additional apparitions, including 2018/19. The original conclusion regarding Giacobini–Zinner’s chemical composition remains unchanged, with it having a 4–6× depletion in the carbon-chain molecules C2 and C3 and in NH, as compared with both OH and CN. The comet continues to exhibit a large asymmetry in production rates as a function of time and heliocentric distance, with produ

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32

Brandt, J. C., R. W. Farquhar, S. P. Maran, M. B. Niedner, and T. von Rosenvinge. "The International Cometary Explorer (ICE) Mission to comet Giacobini-Zinner (G/Z)." International Astronomical Union Colloquium 83 (1985): 405–14. http://dx.doi.org/10.1017/s0252921100084098.

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AbstractThe ICE spacecraft will pass through the tail of P/Giacobini-Zinner on September 11, 1985, to make in situ measurements of particles, fields, and waves that will contribute significantly to the knowledge of plasma tails and other aspects of the cometary/solar wind interaction. By obtaining data on the downstream side of G/Z, the ICE will complement the later upstream measurements obtained by the Comet Halley probes.

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33

Sekanina, Z. "Precession model for the nucleus of periodic comet Giacobini-Zinner." Astronomical Journal 90 (May 1985): 827. http://dx.doi.org/10.1086/113793.

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34

Gosling, J. T., J. R. Asbridge, S. J. Bame, M. F. Thomsen, and R. D. Zwickl. "Large amplitude, low frequency plasma fluctuations at comet Giacobini-Zinner." Geophysical Research Letters 13, no. 3 (1986): 267–70. http://dx.doi.org/10.1029/gl013i003p00267.

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35

Baker, D. N., W. C. Feldman, S. P. Gary, D. J. McComas, and J. Middleditch. "Plasma fluctuations and large-scale mixing near comet Giacobini-Zinner." Geophysical Research Letters 13, no. 3 (1986): 271–74. http://dx.doi.org/10.1029/gl013i003p00271.

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36

Cravens, T. E. "Ion distribution functions in the vicinity of comet Giacobini-Zinner." Geophysical Research Letters 13, no. 3 (1986): 275–78. http://dx.doi.org/10.1029/gl013i003p00275.

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37

Blaauw, Rhiannon C., Robert M. Suggs, and William J. Cooke. "Dust production of comet 21P/Giacobini-Zinner using broadband photometry." Meteoritics & Planetary Science 49, no. 1 (2013): 45–51. http://dx.doi.org/10.1111/maps.12115.

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38

Kiselev, Nikolai N., Klaus Jockers, Vera K. Rosenbush, Fedor P. Velichko, Tanyu Bonev, and Nikolai Karpov. "Anomalous wavelength dependence of polarization of Comet 21P/Giacobini-Zinner." Planetary and Space Science 48, no. 10 (2000): 1005–9. http://dx.doi.org/10.1016/s0032-0633(00)00069-6.

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39

Pérez-de-Tejada, H., G. Zenteno, C. Firmani, J. Bohigas, J. Fierro, and G. F. Bisiacchi. "Spectroscopic observations of comet Giacobini-Zinner during the ice encounter." Advances in Space Research 5, no. 12 (1985): 293–96. http://dx.doi.org/10.1016/0273-1177(85)90100-0.

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40

McFadden, Lucy A., Michael F. A'Hearn, Paul D. Feldman, et al. "Ultraviolet spectrophotometry of comet Giacobini-Zinner during the ICE encounter." Icarus 69, no. 2 (1987): 329–37. http://dx.doi.org/10.1016/0019-1035(87)90109-6.

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41

Lara, L. M., J. Licandro, A. Oscoz, and V. Motta. "Behaviour of Comet 21P/Giacobini-Zinner during the 1998 perihelion." Astronomy & Astrophysics 399, no. 2 (2003): 763–72. http://dx.doi.org/10.1051/0004-6361:20021720.

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42

Staines, K., A. Balogh, S. W. H. Cowley, et al. "Bulk parameters of water group ions at comet Giacobini-Zinner." Advances in Space Research 12, no. 8 (1992): 327–30. http://dx.doi.org/10.1016/0273-1177(92)90406-n.

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43

IPAVICH, F. M., A. B. GALVIN, G. GLOECKLER, D. HOVESTADT, B. KLECKER, and M. SCHOLER. "Comet Giacobini-Zinner: In Situ Observations of Energetic Heavy Ions." Science 232, no. 4748 (1986): 366–69. http://dx.doi.org/10.1126/science.232.4748.366.

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44

Weaver, H. "An Infrared Investigation of Volatiles in Comet 21P/Giacobini–Zinner." Icarus 142, no. 2 (1999): 482–97. http://dx.doi.org/10.1006/icar.1999.6218.

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45

Weaver, H. A., G. Chin, D. Bockelée-Morvan, et al. "An Infrared Investigation of Volatiles in Comet 21P/Giacobini-Zinner." Icarus 144, no. 1 (2000): 203. http://dx.doi.org/10.1006/icar.2000.6351.

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46

Biver, N., D. Bockelée-Morvan, D. C. Lis, et al. "Molecular composition of short-period comets from millimetre-wave spectroscopy: 21P/Giacobini-Zinner, 38P/Stephan-Oterma, 41P/Tuttle-Giacobini-Kresák, and 64P/Swift-Gehrels." Astronomy & Astrophysics 651 (July 2021): A25. http://dx.doi.org/10.1051/0004-6361/202140765.

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We present the results of millimetre-wave spectroscopic observations and spectral surveys of the following short-period comets: 21P/Giacobini-Zinner in September 2018, 41P/Tuttle-Giacobini-Kresák in April 2017, and 64P/Swift-Gehrels and 38P/Stephan-Oterma in December 2018, carried out with the Institut de RadioAstronomie Millimétrique (IRAM) 30-m radio telescope at wavelengths between 1 and 3 mm. Comet 21P was also observed in November 1998 with the IRAM 30-m, James Clerk Maxwell Telescope, and the Caltech submillimeter Observatory radio telescopes at wavelengths from 0.8 to 3 mm. The abundanc

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47

Galt, J. "Observations of comet Giacobini-Zinner at the 1.667 GHz OH line." Astronomical Journal 94 (July 1987): 174. http://dx.doi.org/10.1086/114461.

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48

Jones, D. E., E. J. Smith, J. A. Slavin, B. T. Tsurutani, G. L. Siscoe, and D. A. Mendis. "The bow wave of comet Giacobini-Zinner: Ice magnetic field observations." Geophysical Research Letters 13, no. 3 (1986): 243–46. http://dx.doi.org/10.1029/gl013i003p00243.

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49

Richardson, I. G., S. W. H. Cowley, R. J. Hynds, T. R. Sanderson, K.-P. Wenzel, and P. W. Daly. "Three dimensional energetic ion bulk flows at comet P/Giacobini-Zinner." Geophysical Research Letters 13, no. 4 (1986): 415–18. http://dx.doi.org/10.1029/gl013i004p00415.

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50

Kennel, C. F., F. V. Coroniti, F. L. Scarf, et al. "Plasma waves in the shock interaction regions at comet Giacobini-Zinner." Geophysical Research Letters 13, no. 9 (1986): 921–24. http://dx.doi.org/10.1029/gl013i009p00921.

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