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Journal articles on the topic 'Meteor shower'

Author: Grafiati

Published: 4 June 2021

Last updated: 8 June 2024

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1

Nayana, T., MH Mallikarjun, BV Roopasree, and J. Rajashekar. "Meteor shower." Indian Journal of Ophthalmology - Case Reports 4, no. 2 (2024): 585. http://dx.doi.org/10.4103/ijo.ijo_3018_23.

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2

Yang, Hong-Jin, Changbom Park, and Myeong-Gu Park. "Analysis of Historical Meteor and Meteor shower Records: Korea, China and Japan." Proceedings of the International Astronomical Union 10, H16 (2012): 150–51. http://dx.doi.org/10.1017/s1743921314005079.

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AbstractWe have compiled and analyzed historical meter and meteor shower records in Korean, Chinese, and Japanese chronicles. We have confirmed the peaks of Perseids and an excess due to the mixture of Orionids, north-Taurids, or Leonids through the Monte-Carlo test from the Korean records. The peaks persist for almost one thousand years. We have also analyzed seasonal variation of sporadic meteors from Korean records. Major features in Chinese meteor shower records are quite consistent with those of Korean records, particularly for the last millennium. Japanese records also show Perseids feat

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3

Pendarvis, Edwina. "Meteor Shower: (Summer, 1994)." Appalachian Heritage 30, no. 2 (2002): 19. http://dx.doi.org/10.1353/aph.2002.0049.

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4

Beall, Abigail. "Watch a meteor shower." New Scientist 244, no. 3256 (2019): 51. http://dx.doi.org/10.1016/s0262-4079(19)32170-0.

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5

Hughes, David W. "The Perseid meteor shower." Earth, Moon, and Planets 68, no. 1-3 (1995): 31–70. http://dx.doi.org/10.1007/bf00671498.

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6

Andrews, Brian. "The Leonid Meteor Shower." Ballarat Naturalist (1998:Dec) (December 1998): 6. http://dx.doi.org/10.5962/p.384491.

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7

Williams, I. P., and Z. Wu. "The current Perseid meteor shower." Monthly Notices of the Royal Astronomical Society 269, no. 2 (1994): 524–28. http://dx.doi.org/10.1093/mnras/269.2.524.

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8

McBeath, A. "Meteor, not shower, over Bala." Astronomy & Geophysics 47, no. 6 (2006): 6.8—a—6.8. http://dx.doi.org/10.1093/astrog/47.6.6.8-a.

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9

Ryabova, G. O., and J. Rendtel. "Increasing Geminid meteor shower activity." Monthly Notices of the Royal Astronomical Society: Letters 475, no. 1 (2018): L77—L80. http://dx.doi.org/10.1093/mnrasl/slx205.

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10

Attia, G. F., A. M. Abdelaziz, and I. N. Hassan. "Video Observation of Perseids meteor shower 2016 from Egypt." Applied Mathematics and Nonlinear Sciences 2, no. 1 (2017): 151–56. http://dx.doi.org/10.21042/amns.2017.1.00012.

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AbstractThe results of single television observations of Perseid meteor shower in 2016 are presented. The Perseid shower occurs from 17 July to 24 August, peaking on or around August 12 every year. In 2016, the peak of the Perseids was Night of Aug 11 to the morning of Aug 12. The meteor video observations in Egypt are carried out at The National Researcher Institute of Astronomy and Geophysics (NRIAG). The system consists of TV - cameras Watec -902H Ultimate with the lens DV10x8SA-1 (8-80 mm (10x)) capable of recording the rapid motion of meteors entering the Earth atmosphere.

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11

BASURAH, HASSAN. "The Recorded Meteors and Meteor Shower in the Islamic History." Journal of King Abdulaziz University-Science 16, no. 1 (2004): 3–17. http://dx.doi.org/10.4197/sci.16-1.12.

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12

Cowen, Ron. "Meteor Shower Promises Quite a Show." Science News 160, no. 19 (2001): 293. http://dx.doi.org/10.2307/4012938.

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13

Vaubaillon, J., R. Arlt, S. Shanov, S. Dubrovski, and M. Sato. "The 2004 June Bootid meteor shower." Monthly Notices of the Royal Astronomical Society 362, no. 4 (2005): 1463–71. http://dx.doi.org/10.1111/j.1365-2966.2005.09421.x.

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14

Jenniskens, Peter. "The IAU Meteor Shower Nomenclature Rules." Earth, Moon, and Planets 102, no. 1-4 (2007): 5–9. http://dx.doi.org/10.1007/s11038-007-9155-5.

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15

Cevolani, G., V. Porubčan, A. Hajduk, M. F. Gabucci, G. Grassi, and G. Trivellone. "Radio Geminid meteor shower of 1994." Il Nuovo Cimento C 19, no. 3 (1996): 451–54. http://dx.doi.org/10.1007/bf02509302.

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16

Banzhaf, William H. "Commentary: A Meteor Shower of Activities." Journal of Forestry 93, no. 10 (1995): 3. http://dx.doi.org/10.1093/jof/93.10.3.

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17

Asher, David J. "The dynamical structure of meteor streams and meteor shower predictions." Proceedings of the International Astronomical Union 2004, IAUC197 (2004): 375–82. http://dx.doi.org/10.1017/s1743921304008877.

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18

Campbell-Brown, M. D., R. Blaauw, and A. Kingery. "Optical fluxes and meteor properties of the camelopardalid meteor shower." Icarus 277 (October 2016): 141–53. http://dx.doi.org/10.1016/j.icarus.2016.05.001.

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19

Dunker, T., U. P. Hoppe, G. Stober, and M. Rapp. "Development of the mesospheric Na layer at 69° N during the Geminids meteor shower 2010." Annales Geophysicae 31, no. 1 (2013): 61–73. http://dx.doi.org/10.5194/angeo-31-61-2013.

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Abstract. The ECOMA sounding rocket campaign in 2010 was performed to investigate the charge state and number density of meteoric smoke particles during the Geminids meteor shower in December 2010. The ALOMAR Na lidar contributed to the campaign with measurements of sodium number density, temperature and line-of-sight wind between 80 and 110 km altitude over Andøya in northern Norway. This paper investigates a possible connection between the Geminids meteor shower and the mesospheric sodium layer. We compare with data from a meteor radar and from a rocket-borne in situ particle instrument on t

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20

Ishizaki, Masaharu, Jun-ichi Watanabe, and Mikiya Sato. "Meteor shower activity derived from meteor watching public campaign in Japan." Planetary and Space Science 143 (September 2017): 99–103. http://dx.doi.org/10.1016/j.pss.2017.01.006.

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21

Kozlovsky, Alexander, Renata Lukianova, Sergey Shalimov, and Mark Lester. "Mesospheric temperature estimation from meteor decay times during Geminids meteor shower." Journal of Geophysical Research: Space Physics 121, no. 2 (2016): 1669–79. http://dx.doi.org/10.1002/2015ja022222.

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22

DELAPENA, S., S. AVERY, and J. AVERY. "Observations of the 2001 Leonid meteor shower using VHF meteor radar." Icarus 196, no. 1 (2008): 164–70. http://dx.doi.org/10.1016/j.icarus.2008.02.019.

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23

Moorhead, Althea V., Auriane Egal, Peter G. Brown, Danielle E. Moser, and William J. Cooke. "Meteor Shower Forecasting in Near-Earth Space." Journal of Spacecraft and Rockets 56, no. 5 (2019): 1531–45. http://dx.doi.org/10.2514/1.a34416.

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24

Gater, Will. "New Arid meteor shower delights star gazers." New Scientist 252, no. 3357 (2021): 12. http://dx.doi.org/10.1016/s0262-4079(21)01868-6.

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25

Wiegert, Paul A., Peter G. Brown, Robert J. Weryk, and Daniel K. Wong. "THE RETURN OF THE ANDROMEDIDS METEOR SHOWER." Astronomical Journal 145, no. 3 (2013): 70. http://dx.doi.org/10.1088/0004-6256/145/3/70.

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26

Mallama, Anthony, and Fred Espenak. "Automated Meteor Detection and the Leonid Shower." Publications of the Astronomical Society of the Pacific 111, no. 757 (1999): 359–63. http://dx.doi.org/10.1086/316333.

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27

Hunten, D. M., R. W. H. Kozlowski, and A. L. Sprague. "A possible meteor shower on the Moon." Geophysical Research Letters 18, no. 11 (1991): 2101–4. http://dx.doi.org/10.1029/91gl02543.

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28

Sugar, Glenn, Althea Moorhead, Peter Brown, and William Cooke. "Meteor shower detection with density-based clustering." Meteoritics & Planetary Science 52, no. 6 (2017): 1048–59. http://dx.doi.org/10.1111/maps.12856.

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29

Kumar, Devulapalli Venkata Phani, Kammadhanam Chenna Reddy, and Ganji Yellaiah. "Radar Observations of Leonid Meteor Shower 2003." Astrophysics and Space Science 306, no. 4 (2006): 235–39. http://dx.doi.org/10.1007/s10509-006-9267-9.

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30

Hughes, David W. "The world's most famous meteor shower picture." Earth, Moon, and Planets 68, no. 1-3 (1995): 311–22. http://dx.doi.org/10.1007/bf00671522.

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31

Christou, Apostolos A. "PREDICTING MARTIAN AND VENUSIAN METEOR SHOWER ACTIVITY." Earth, Moon, and Planets 95, no. 1-4 (2005): 425–31. http://dx.doi.org/10.1007/s11038-005-9023-0.

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32

Ryabova, Galina O. "Model Radiants of the Geminid Meteor Shower." Earth, Moon, and Planets 102, no. 1-4 (2007): 95–102. http://dx.doi.org/10.1007/s11038-007-9180-4.

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33

Brown, P. "The Leonid Meteor Shower: Historical Visual Observations." Icarus 138, no. 2 (1999): 287–308. http://dx.doi.org/10.1006/icar.1998.6074.

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34

Ito, Takatoshi, Robert F. Engle, and Wen-Ling Lin. "Where does the meteor shower come from?" Journal of International Economics 32, no. 3-4 (1992): 221–40. http://dx.doi.org/10.1016/0022-1996(92)90018-f.

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35

Belkora, Leila. "Robert Frost and the Leonid Meteor Shower." Culture and Cosmos 27, no. 0102 (2023): 227–39. http://dx.doi.org/10.46472/cc.01227.0227.

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Robert Frost (1874–1963) enjoyed a lifelong interest in astronomy, and a number of his works refer to astronomical phenomena and to our propensity to look for meaning in them. Frost’s poem ‘A Loose Mountain (Telescopic)’, published in 1942, provides an apt—and humorous—description of the Leonid meteor shower. Aspects of the poem suggest Frost was inspired by the complex history of the Leonids, and in particular, the failure of the Leonid ‘storm’ to appear as predicted in 1899. Like the old constellation myths, the poem tells a story that helps us understand and remember a night-sky phenomenon.

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36

Koten, P., D. Čapek, P. Spurný, R. Štork, V. Vojáček, and J. Bednář. "Search for pairs and groups in the 2006 Geminid meteor shower." Astronomy & Astrophysics 656 (December 2021): A98. http://dx.doi.org/10.1051/0004-6361/202141809.

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Context. The existence of pairs and groups of meteors during meteor showers has been an open question for a long time. The double-station video observation of the 2006 Geminid meteor shower, one of the most active annual showers, is used for the search of such events. Aims. The goal of the paper is to determine whether the observed pairs of Geminid meteors are real events or cases of random coincidence. Methods. The atmospheric trajectories of the observed meteors, photometric masses, and both time and spatial distances of meteoroids in the atmosphere were determined using a double-station vid

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37

CHEN, Jinsong, Baiqi NING, and Weixing WAN. "Observation on Meteor Velocities of the Quadrantid Meteor Shower by Using the Wuhan Meteor Radar." Chinese Journal of Space Science 26, no. 2 (2006): 118. http://dx.doi.org/10.11728/cjss2006.02.118.

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38

Younger, J. P., I. M. Reid, R. A. Vincent, and D. J. Murphy. "Meteor shower velocity estimates from single-station meteor radar: accuracy and precision." Monthly Notices of the Royal Astronomical Society 425, no. 2 (2012): 1473–78. http://dx.doi.org/10.1111/j.1365-2966.2012.21632.x.

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39

YANG, H., C. PARK, and M. PARK. "Analysis of historical meteor and meteor shower records: Korea, China, and Japan." Icarus 175, no. 1 (2005): 215–25. http://dx.doi.org/10.1016/j.icarus.2004.10.007.

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40

Brown, P. "Recent Visual Observations of the Leonid Meteor Shower." Highlights of Astronomy 11, no. 2 (1998): 1013–14. http://dx.doi.org/10.1017/s153929960001947x.

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We know the Leonid shower primarily from its record of visual appearances over the last millenium. The period of the stream and its status as a cosmic phenomenon are all intimately linked to historical visual observations of the stream. The advent of modern observational techniques in meteor astronomy such as radar and photography has not decreased the value of visual recordings of the stream; on the contrary, visual observations form our primary means of long-term monitoring of the shower.

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41

Ryabova, G. O. "The Geminid meteor shower radiant: a mathematical model." Monthly Notices of the Royal Astronomical Society 507, no. 3 (2021): 4481–86. http://dx.doi.org/10.1093/mnras/stab2286.

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ABSTRACT The origin of the Geminid meteoroid stream and its parent body the asteroid (3200) Phaethon is still under discussion. The observed bimodal activity profile of the Geminid shower agrees with a cometary scheme of the stream formation. We show that the radiant areas for meteors of different magnitudes may also be used to provide arguments supporting or undermining the cometary hypothesis. We used semi-analytic and numerical models of the stream. The resulting model radiants for meteors of various magnitudes (masses) have peculiar patterns that might be detected in a real shower.

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42

Kozak, P. M., and J. Watanabe. "Meteors with extreme beginning heights from observations with high-sensitivity super-isocon TV systems." Monthly Notices of the Royal Astronomical Society 497, no. 4 (2020): 5550–59. http://dx.doi.org/10.1093/mnras/staa2183.

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ABSTRACT Meteors with extremely high altitudes are considered. Parameters of seven meteors having anomalous beginning heights recorded with highly sensitive super-Isocon TV systems are presented. One 1993 Perseid meteor, one 2001 sporadic meteor and five meteors from the 2002 Leonid storm had beginning heights in the range 135–145 km. The sporadic meteor is used to demonstrate the methods of data processing and observation precision results. The original TV meteor images, photometric calibration curves and meteor light curve are shown. Light curves are shown for the Leonid shower meteors as we

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43

Hajduková, M., та L. Neslušan. "Modeling of the meteoroid stream of comet C/1975 T2 and λ-Ursae Majorids". Astronomy & Astrophysics 627 (липень 2019): A73. http://dx.doi.org/10.1051/0004-6361/201935630.

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Aims. We study the meteoroid stream of the long-period comet C/1975 T2 (Suzuki-Saigusa-Mori). This comet was suggested as the parent body of the established λ-Ursae Majorid meteor shower, No. 524. Methods. We modeled 32 parts of a theoretical meteoroid stream of the parent comet considered. Each of our models is characterized with a single value of the evolutionary time and a single value of the strength of Poynting-Robertson effect. The evolutionary time ranges from 10 000 to 80 000 yr. It is the period during which the evolution of the stream part is followed. In each model, the dynamical ev

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44

Lindblad, B. A. "Meteor Studies." International Astronomical Union Colloquium 98 (1988): 170–72. http://dx.doi.org/10.1017/s0252921100092733.

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Historically meteor astronomy is one area where amateurs have always been able to make significant contributions. In fact, in the 19th century, it was amateur naked eye and telescopic observations which laid down much of the foundations of meteor astronomy. References to this work can be found in any textbook on meteors. The 19th century observers concentrated on counting meteors, estimating magnitudes and plotting the meteor paths on star maps. Their main interest was to determine hourly rates and shower radiants. An important milestone was Denning’s radiant catalogue (Denning 1882), which in

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45

Selvamurugan, R., C. V. Devasia, A. R. Jain, C. Raghava Reddi, P. B. Rao, and R. Sridharan. "Observations on Stratospheric-Mesospheric-Thermospheric temperatures using Indian MST radar and co-located LIDAR during Leonid Meteor Shower (LMS)." Annales Geophysicae 20, no. 11 (2002): 1869–76. http://dx.doi.org/10.5194/angeo-20-1869-2002.

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Abstract. The temporal and height statistics of the occurrence of meteor trails during the Leonid meteor shower revealed the capability of the Indian MST radar to record large numbers of meteor trails. The distribution of radio meteor trails due to a Leonid meteor shower in space and time provided a unique opportunity to construct the height profiles of lower thermospheric temperatures and winds, with good time and height resolution. There was a four-fold increase in the meteor trails observed during the LMS compared to a typical non-shower day. The temperatures were found to be in excellent c

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46

Campbell-Brown, M. D., G. Stober, C. Jacobi, J. Kero, A. Kozlovsky, and M. Lester. "Radar observations of Draconid outbursts." Monthly Notices of the Royal Astronomical Society 507, no. 1 (2021): 852–57. http://dx.doi.org/10.1093/mnras/stab2174.

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ABSTRACT The Draconid meteor shower shows strong bursts of activity at irregular intervals, with nearly no activity in intervening years. Five outbursts of the Draconid meteor shower were observed with specular meteor radars in Canada and Europe between 1999 and 2018. The outbursts generally lasted between 6 and 8 h, and most were not fully visible at a single geographical site, emphasizing the need for observations at multiple longitudes for short-duration shower outbursts. There is at least a factor of two difference in the peak flux as measured on different radars; the initial trail radius

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47

Wu, Z., and I. P. Williams. "The Perseid meteor shower at the current time." Monthly Notices of the Royal Astronomical Society 264, no. 4 (1993): 980–90. http://dx.doi.org/10.1093/mnras/264.4.980.

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48

Neslušan, L., Z. Kaňuchová, and D. Tomko. "The meteor-shower complex of 96P/Machholz revisited." Astronomy & Astrophysics 551 (February 27, 2013): A87. http://dx.doi.org/10.1051/0004-6361/201220299.

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49

Jenniskens, Peter, and Jérémie Vaubaillon. "An unusual meteor shower on 1 September 2007." Eos, Transactions American Geophysical Union 88, no. 32 (2007): 317–18. http://dx.doi.org/10.1029/2007eo320001.

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50

Peng, Bozhen, Dingyi Sun, Qifei Cui, and Chun Yin Yip. "Meteor Shower Scale Prediction Using Random Forest Classification." Journal of Physics: Conference Series 1486 (April 2020): 052007. http://dx.doi.org/10.1088/1742-6596/1486/5/052007.

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