کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
1773553 1021138 2011 22 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
CAMS: Cameras for Allsky Meteor Surveillance to establish minor meteor showers
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم فضا و نجوم
پیش نمایش صفحه اول مقاله
CAMS: Cameras for Allsky Meteor Surveillance to establish minor meteor showers
چکیده انگلیسی

First results are presented from a newly developed meteoroid orbit survey, called CAMS – Cameras for Allsky Meteor Surveillance, which combines meteor detection algorithms for low-light video observations with traditional video surveillance tools. Sixty video cameras at three stations monitor the sky above 31° elevation. Goal of CAMS is to verify meteor showers in search of their parent comets among newly discovered near-Earth objects.This paper outlines the concept of operations, the hardware, and software methods used during operation and in the data reduction pipeline, and accompanies the data release of the first batch of meteoroid orbits. During the month of November 2010, 2169 precisely reduced meteoroid trajectories from 17 nights have an error in the apparent radiant of the trajectory <2° and error in speed <10%. Median values of the error are 0.31° and 0.53 km/s, respectively, sufficient to resolve the intrinsic dispersion of annual meteor showers and resolve minor showers from the sporadic background. The limiting visual magnitude of the cameras is +5.4, recording meteors of +4 magnitude and brighter, bright enough to stand out from the mostly fainter sporadic meteors detected as under dense radar echoes.CAMS readily detected all established showers (6) active during the clear nights in November. Of the showers that needed confirmation, we confirm the theta Aurigids (THA, IAU#390), the chi Taurids (CTA, IAU#388), and the omicron Eridanids (OER, IAU#338). We conclude that the iota November Aurigids (IAR, IAU#248) are in fact the combined activity of the theta Aurigids and chi Taurids, and this shower should be dismissed from the list. Finally, there is also a clustering consistent with the zeta Cancrids (ZCN, IAU#243), but we cannot exclude that this is lower perihelion dust belonging to the Orionid shower.Data are submitted to the IAU Meteor Data Center on a semi-regular basis, and can be accessed also at http://cams.seti.org.


► CAMS (Cameras for Allsky Meteor Surveillance) is a newly developed meteoroid orbit survey.
► Goal of CAMS is to verify meteor showers in the IAU Meteor Shower Working List.
► Paper outlines concept of operations, the hardware, and the software methods.
► First results include 2169 orbits from 17 nights in November 2010.
► Three showers are confirmed, evidence for fourth, one is excluded as being duplicate.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Icarus - Volume 216, Issue 1, November 2011, Pages 40–61
نویسندگان
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