The result of Orionids
This page provieds the result of Orionids by radio meteor observations all over the world.
Annual Variations
Annual Variation List
Annual Variation Graphs
Information (as following list)
| Year | source | Comments (Time:UT) |
|---|---|---|
| 2021 | WorldWide | No clear activity. But some activity was detected around λ⊙=208°.5 |
| 2020 | WorldWide | No clear activity. |
| 2019 | WorldWide | No clear activity. But some activity was detected around λ⊙=210° |
| 2018 | WorldWide | No clear activity. |
| 2017 | WorldWide | No clear activity. |
| 2016 | WorldWide | No clear activity. The estimated visual ZHR was under 30. |
| 2015 | WorldWide | No activity, basically. But some activity was detected around λ⊙=206°.7 |
| 2014 | WorldWide | No activity. The activity level showed usual activity. |
| 2013 | WorldWide | The Orionid activity using radio meteor observation was gone. |
| 2012 | WorldWide | The activity had weak level and wide FWHM. |
| 2011 | WorldWide | The activity level was weaker and weaker. |
| 2010 | WorldWide | The activity level was weaker than 2009. The peak time was earlier. |
| 2009 | WorldWide | The peak time and level were same as 2008. Long Echoes peak was later. |
| 2008 | WorldWide | The peak was around λ⊙=208°.5. It was less than 2006 and 2007. |
| 2007 | WorldWide | The activity level and peak time were same as 2006 Orionids. |
| 2006 | WorldWide | The activity was higher than annual year. The peak was λ⊙=208°.0. |
| 2005 | WorldWide | Although the clear activity was not seen, the center of activity was λ⊙=209° |
| 2004 | WorldWide | It was not only unclear peak but also unclear activity. |
| 2003 | – | UnderConstruction |
| 2002 | – | UnderConstruction |
| 2001 | Misato Obs | The peak was unclear (20th?) |
| 2000 | Misato Obs | The peak was 23rd with HR42. |
| 1999 | Chigusa HS | The peak was 21st-22nd with HR26 |
Introduction
Introduction and observing conditions are provided this content.
Introduction of Orionids