All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Three Peaks of 2011 Draconid Activity Including that Connected with Pre-1900 Material

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00433643" target="_blank" >RIV/67985815:_____/14:00433643 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1007/s11038-014-9435-9" target="_blank" >http://dx.doi.org/10.1007/s11038-014-9435-9</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1007/s11038-014-9435-9" target="_blank" >10.1007/s11038-014-9435-9</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Three Peaks of 2011 Draconid Activity Including that Connected with Pre-1900 Material

  • Original language description

    A Draconid meteor shower outburst was observed from on board two scientific aircraft deployed above Northern Europe on 8th October 2011. The activity profile was measured using a set of photographic and video cameras. The corrected hourly rates reached avalue of almost 350. The brighter meteors peaked about 15-20 min earlier than the dimmer ones. This difference can be explained by different directions of the ejection of the meteoroids from the parent comet. One of the instruments was even able to detect meteors connected with the material ejected from the parent comet before 1900 and thus confirmed the prediction of the model, although it was based on uncertain pre-1900 cometary data. Another small peak of the activity, which was caused by material ejected during the 1926 perihelion passage of the parent comet, was detected around 21:10 UT. The mass distribution index determined using the narrow field-of-view video camera was 2.0 +/- A 0.1. This work shows that the observation of met

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2014

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Earth, Moon, and Planets

  • ISSN

    0167-9295

  • e-ISSN

  • Volume of the periodical

    112

  • Issue of the periodical within the volume

    1-4

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    17

  • Pages from-to

    15-31

  • UT code for WoS article

    000339720000003

  • EID of the result in the Scopus database